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Contents
Vol.38, No.06
June 2025
18 The 2025 Avalon Airshow
This year’s airshow, again held near Melbourne, featured quite a bit of new
technology, especially new drones and defences against hostile drones.
There was also some new space and satellite technology on display.
By Dr David Maddison, VK3DSM
Aerospace exhibition report
42 Altium Designer 25 review
Altium Designer 25 is the latest version of the EDA (electronics design
automation) software that we use for our PCB designs. This new version
supports chip-on-board routing, signal integrity checking plugins and more.
By Tim Blythman
EDA software review
58 Douk hybrid valve amp review
This well-presented amplifier combines a dual triode preamplifier with a
100W per channel Class-D power amplifier. It’s intended to give the benefits
of both technologies, and includes tone controls and a power meter.
Review By Allan Linton-Smith
Hifi review
Page 35
Hot
Water
System
Solar Diverter
SSB Shortwave
Receiver
70 Precision Electronics, Part 8
In this penultimate entry in the series, we look at how voltage references
work, as they are critical to the precision of both ADCs and DACs. In turn,
they are part of most modern measurement and control systems.
By Andrew Levido
Electronic design
35 Hot Water System Solar Diverter
Page 46
2
Editorial Viewpoint
5
Mailbag
30
Subscriptions
82
Online Shop
86
Circuit Notebook
88
Serviceman’s Log
94
Vintage Radio
74 Easy-to-make Outdoor Subwoofer
101
Ask Silicon Chip
Made using a prebuilt enclosure, this subwoofer can be used indoors or
outdoors; for example, in a patio area. It’s attractive, inexpensive and can
add substantial bottom end to most sound systems!
By Julian Edgar
Audio project
103
Market Centre
104
Advertising Index
You can save a lot of money with this device! It lets you use excess solar
power generation to power your electric water heater. Crucially, it’s a lot
less expensive to put together than an equivalent commercial unit.
By Ray Berkelmans & John Clarke
Solar energy project
46 SSB Shortwave Receiver, part 1
This superhet-based shortwave receiver supports USB and LSB decoding
and has digital tuning from 3MHz to 30MHz. It’s controlled by an Arduino and
has AGC, decent noise performance, an antenna tuning adjustment & more.
By Charles Kosina
Radio receiver project
62 DIY 433MHz Receiver Module
A companion to the 433MHz Transmitter Module we published in the April
issue, this receiver matches or beats the performance of typical prebuilt
modules. It also has a handy RSSI (signal strength) output.
By Tim Blythman
Radio control project
siliconchip.com.au
Australia's electronics magazine
1. Detecting smokers with a MaixCam
2. Non-contact EMF detector
3. Advanced SMD Test Tweezers case
A 1970s Little General by Fred Lever
June 2025 1
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Editorial Viewpoint
PCB assembly pitfalls
Now and then we get requests to supply circuit
boards with some or all parts pre-soldered to them.
While it seems like an attractive idea on the surface,
we generally have not done it for a few reasons.
The first is the financial risk involved. We would
have to pay for the PCBs to be made, plus the (potentially expensive) parts, then for the assembly, all before
we know how many we are going to sell.
However, my biggest concern was the things that could go wrong in the
process. What if the parts or the boards we receive are faulty, or even the soldering? Regardless of whether we picked up these problems before or after
they reached customers, we’d be unlikely to recover any of the money we
had spent. We would either have to abandon it altogether, or start over and
hope to avoid the same problems the second time.
There’s also the fact that acting as a quasi-manufacturer distracts us from
the task of publishing the magazine, which is considerably more important.
When the Pico 2 Computer project was published in our April issue, we
knew that the designers had built multiple prototypes that worked. They
also provided us with all the files we’d need to get boards made, and even
instructions on how to go about ordering them. So, I thought it was finally
time to give it a try. After all, they had practically handed it to us on a plate!
What none of us were expecting was that JLCPCB (the company we paid to
assemble the Pico 2 Computer boards) had been delivered a batch of apparently defective CH334F USB hub chips. They started using those to assemble
boards just before we ordered a large number from them.
These are the hardest chips to solder or desolder on the whole board. And,
of course, there is apparently no other source of these chips than JLCPCB
and their supplier, LCSC. So we couldn’t order parts from a different batch
in the hope that they would function correctly.
This could have been a disaster. It was lucky that someone else had ordered
some boards not long before we did, found they didn’t work, and contacted
Peter Mather (the Pico 2 Computer PCB designer) for help. He swapped the
CH334F chips between one of the new boards and a known good one, and
found that the fault followed the chip, confirming that was the problem.
It was also very fortuitous that there was an easy way to work around this
problem. The defective part of the chip was involved in sensing an over-
current condition on the USB ports and cutting power to them. This was
sensed via a resistive divider. Removing the two resistors in that divider
disabled the function, and the chips then worked perfectly.
The board has a PTC thermistor as a second line of defence to limit the
current drawn from the USB ports if there is a fault. So disabling this active
current monitoring feature isn’t really a problem.
We had to remove the resistors from all the assembled boards we received
and added notes to the kits explaining that. This approach allowed us to
salvage those boards and avoid a bad experience for our customers.
Ordering these Pico 2 Computer boards was a way for us to ‘dip our toes
in the water’ with regards to possibly providing assembled PCBs in future
when necessary. I don’t want to do this as a matter of course, because I think
it side-steps an important part of hobby electronics; it’s mainly when we can’t
avoid using chips that most people would struggle with soldering.
Inevitably, more and more new chips only come in packages like QFN and
BGA. That’s simply the way that electronics is heading.
In summary, I like the idea of having boards professionally assembled, but
we must proceed with caution. There is still a lot that can go wrong, as this
experience demonstrated.
by Nicholas Vinen
9 Kendall Street, Granville NSW 2142
2
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MAILBAG
your feedback
Letters and emails should contain complete name, address and daytime phone number. Letters to the Editor are submitted on the condition that
Silicon Chip Publications Pty Ltd has the right to edit, reproduce in electronic form, and communicate these letters. This also applies to submissions to “Ask Silicon Chip”, “Circuit Notebook” and “Serviceman’s Log”.
Garbage & Recycling Reminder project is still relevant
I have been reading Silicon Chip for many years now. I
look forward each month to a copy in my letterbox. After
a quick look through, I begin my reading. When travelling
by train, I find your magazine becomes my first choice of
what to take to read. I enjoy the Serviceman’s Log and some
of the many project articles.
I would like to suggest a simple project that could have
commercial applications.
I live in Brisbane and our local garbage service provides
up with three bins, one collected every week and the other
two on alternative weeks. After some time, it becomes a
bit confusing which bin to put out with the main garbage
bin each week.
I would like a simple real-time device that flashes
coloured LEDs on the day that a particular bin needs to go
out. For example, a red LED for garbage day, green LED for
the garden waste collection and a yellow LED for the recycling collection. There would need to be a setup section to
set the date etc and to select the day of the week that the
garbage is to be put out on the curb side.
This might fit under the Mini Projects heading, or become
a standalone project. Thank you for the wonderful magazine.
Warren Rose, Joyner, Qld.
Comment: thanks for the suggestion. The Garbage &
Recycling Reminder project (January 2013; siliconchip.
au/Article/1315) is pretty much what you are asking for.
It has four differently coloured LEDs. We think it would be
suitable for your needs and probably doesn’t need to be
updated, despite being published over 10 years ago now.
Smartphone reminder apps are also available.
More on staying with Windows 10
I wholeheartedly agree with your stance regarding
‘upgrading’ to Windows 11. Your statement “... Windows
10 does everything I need, so why would I want to switch
to something new?” says it all. If it ain’t broke, don’t fix it.
After nearly 10 years of use on millions of computers,
one should think that Windows 10 is reliable and stable.
I have no intention of moving to another round of chaos
just because Microsoft thinks I should. And, it seems, Microsoft will not allow me to do so as two of my systems are
regarded as not suitable for Windows 11.
Should one be forced into installing Windows 11, an
internet search reveals there are ways to install it without
a Microsoft account. A workaround is once Windows is
installed, create a local account with Administrator privileges and use it instead. I was given a computer with Windows 11 installed. It is not connected to the internet and I
have full control of it using the local account.
siliconchip.com.au
While on the subject of accounts, a good practice is
to create user accounts and use them for all day-to-day
work. Only use the administrative account for installing software or other administrative tasks. Often, even
this is not required as Windows will ask for administrative privilege when required, even though logged on as a
non-privileged user.
This computer has separate accounts for myself and
my wife. This allows individual settings for software such
as browsers. Also, having unprivileged accounts adds a
layer of security. Most viruses that try to take control of a
machine rely on running as an administrator.
I’m looking forward to the day when I don’t have to look
at those circulating balls and an inaccurate percentage of
work completed.
Alan Cashin, Islington, NSW.
A trap to avoid when cutting audio cables
I decided to use stereo RCA audio cables for an Arduino project. Like Julian Edgar (“Audio Mixing Cables”,
March 2025; siliconchip.au/Article/17787), I planned to
cut purchased cables. However, in my case, the plan was
to have bare wires at both ends. I bought quality cables
from a local source.
Provided I used the one cable for both halves of a given
project, everything worked OK. However, I built multiple
units, and when I mixed up the devices at the ends of the
cable, I found that my project sometimes didn’t work.
I tracked the problem to the cable – specifically the
colour-coding of the wires versus the connectors. The shield
conductor appears to be safe, but the left/right connector/
colour-code relationship wasn’t. The cables were wired
correctly end-to-end (so the cable would work perfectly if
not cut open), but the signal wires were sometimes wired
to the wrong pin of the connector.
The bottom line is: if you cut open such a factory-produced
cable, even high-quality ones, check that the colour-coding
of the wires is correct relative to the connector.
John Evans, Macgregor, ACT.
How to store extension cords
Regarding your Editorial Viewpoint in the June 2024
issue, if any flexible lead is regularly bent, especially on a
tight radius, will break the individual fine strands of each,
which can then penetrate the insulation.
While working as a maintenance electrician on robotics,
this was a common occurrence. These faults were often hard
to find due to the strands being very fine. They would act as
fuses, and the short would blow clear, with the robot then
able to run again until the next two strands happen to touch.
Australia's electronics magazine
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There are cables that are less prone to this, but they can
be expensive.
With extension leads, the best way to prevent this is
to have them on a drum or roll them neatly and flat and,
when unwinding them, do not hold each end of the cord
and pull it out. This will regularly put tight bends in the
cord, making it prone to fracture.
Peter Zarebski, Knoxfield, Vic.
More on fluidic computers
I noticed you have been discussing fluidic computers lately. At an open day in 1970, at the PMG Research
Laboratories displayed a simple fluidic computer, as shown
in the newspaper clipping below. Digital ICs rapidly killed
this technology!
Bob Backway, Belgrave Heights, Vic.
Serial driver trick for Windows 7
I have successfully assembled the Programmable Frequency Divider kit that I purchased from Silicon Chip a
week or so ago (SC6959). I plugged it into my Windows 7
PC and the driver was successfully installed, but I couldn’t
get Tera Term Pro to connect to its serial port. The Frequency Divider comes up as “Win USB generic device” in
the Control Panel devices list.
I plugged an Arduino into the PC and it comes up under
“PORTS (COM & LPT)” and shows the Arduino connected
to COM4.
I then did what I should have done at the start; I tried it
on my Windows 10 PC. The driver instantly installed and
Tera Term could communicate with the Frequency Divider
project. I then copied the drivers folder from the Windows
10 PC onto a USB drive and transferred it to the Windows
7 PC drivers folder.
I went through the device manager and updated the
driver. I then selected the driver manually from a list of drivers. Scrolling through the list of manufacturers, I selected
Microchip and got the warning about it not being recommended. I hit next and the driver successfully installed on
the Windows 7 machine. Then it was all good. Thanks for
a clever bit of test gear.
Geoff Coppa, Toormina, NSW.
Just because it’s AI doesn’t mean it’s right
I find these days that Google searches usually offer an
AI answer at the top of the results. I frequently find that
this answer has errors in it, even on technical or scientific
matters. Just because it comes from AI doesn’t mean it’s
true. In fact, AI is less trustworthy than most legitimate
sources of information.
It is concerning that many professionals in science, engineering, law, medicine, journalism and business now rely
on AI to do their thinking for them. It is also used to write
summaries of meetings and even medical consultations. A
lot could go wrong there!
It’s only a matter of time before there is a major engineering or medical disaster that will be attributable to what the
AI said or told someone to do.
If you don’t have knowledge on a subject, don’t rely on
an AI to inform you. It will just make you more stupid.
Dr David Maddison, Toorak, Vic.
Using op amps for industrial control
Thank you for the very interesting article on the
History of Operational Amplifiers (August 2021;
siliconchip.au/Article/14987). When I finished studying
electronics in 1967, absolutely nothing was mentioned about
op amps! We only experimented with valves (mostly) and
some transistors at school.
When I started working in 1968, I only worked with
transistors and relays in safety systems for steam turbines.
However, suddenly the guy working with steam turbine
control moved to another office, and I had to very quickly
try to get some knowledge about op amps. I bought some
amplifiers and started experimenting at home.
8
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I then worked a lot with them from the beginning of
1970 until about 1980. We used them for control of steam
turbines with 2-500MW of output power.
The first op amp I came in contact with was the LM709.
However, it had a drawback that if fed with a little bit too
high an input voltage, it sometimes ‘locked’ either at maximum output or minimum output, and it was then only
possible to get it working again by removing the supply
voltage for a while. When we changed to the LM301, this
problem was solved.
I fully agree with your conclusion that the op amp is a
very flexible device. Once again, thanks for very interesting reading!
Urban Ekholm, Sweden.
Success building numerous DIY test instruments
As an avid reader of Silicon Chip since your very first
issue in 1987, I wanted to share feedback on my recent
experiences with building a number of your projects over
the past 6 months.
I am currently redeveloping the David Tilbrook ETI Series
5000 Control Preamplifier from 1981 as a nostalgia project.
The idea came about after I acquired a rusty old built-kit
from a friend, before deciding to strip the boards and wiring, and replace them with new.
My spare time has been absorbed with many iterations of
Tilbrook’s original design, and I am now drawing close to
completion. In essence, the project morphed into a multiboard redesign using KiCAD (as reviewed in your Open
Source feature in the February 2025 issue). What a learning
curve! Some two years later, I am now bench testing the
changes using several Silicon Chip test equipment projects.
I recently completed the Intelligent Dual Hybrid Power
Supply by Phil Prosser (February-March 2022; siliconchip.
au/Series/377). I have been building kits since the late
1970s, and had the privilege of managing Jaycar’s kit department for many years in the 1990s, working closely with
Silicon Chip in getting the magazine’s projects to market.
During that time, I built countless audio projects as
demo units in Jaycar stores and as a general check. For the
larger projects, I rewrote construction articles and added
step-by-step guides with the goal of providing less experienced constructors with the confidence to successfully
build complex audio kits (the magazine obviously has limited space for such in-depth guides). It was hard work, but
it was incredibly fun!
Your Dual Hybrid PSU design was by far the most enjoyable project I have assembled in many years, forcing me to
learn new techniques such as SMD soldering (including
‘drag soldering’ for the fine-pitch microcontroller), tapping
M3 holes for the heatsink, sheet metal bending, precision
hole cuts and so on.
Unfortunately for me, this was one project that didn’t
fire up the first time. I had inadvertently swapped the
specified LM2575-5.0V regulator with the adjustable version and hadn’t noticed its ADJ suffix! I believed that the
LM2575 was faulty because it was providing just 1.5V output (which is actually correct for the adjustable version).
After replacing these devices with the correct 5V versions, the two switch-mode modules sprang to life. However, I still had work to do. The microprocessor control
board was not working as expected and, after borrowing a
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friend’s digital microscope to inspect the board at a microscopic level, I discovered that a tiny metal fragment behind
the micro was shorting-out pins.
I found this almost by accident, and very near me wanting to give up the whole affair. With the otherwise invisible fragment now removed, the supply sprang to life and I
now have a phenomenal piece of bench equipment.
While it certainly cost more than what I could buy a
similar dual tracking supply for from China, I now have
newfound skills and deeper knowledge of switch-mode
PSU design and fault-finding. To me, that’s priceless. A key
lesson was that seasoned constructors shouldn’t be cocky
when approaching a build that, on the surface, appears
straightforward!
Thanks to your magazine, I now have a bench brimming
with new test gear in support of my audio project. I also
built the WiFi DDS Function Generator by Richard Palmer
(May-June 2024; siliconchip.au/Series/416) and incorporated John Clarke’s DC Supply Protector within the case
(June 2024; siliconchip.au/Article/16292).
I also plan to build the combined LC/ESR Meter by Steve
Matthysen (August 2023; siliconchip.au/Article/15901)
over the coming days, as well as Jim Rowe’s Digital Audio
Millivoltmeter (October 2019; siliconchip.au/Article/
12018). These, along with a newly acquired Rigol DSO,
will allow me to push ahead with confidence.
Thanks to your magazine and its contributors for fuelling
my passion for this incredible hobby that has afforded me
a career of 40+ years within the industry. I view your magazine’s ongoing success as crucial. That’s why I recently
decided to become a subscriber, and will continue to be
for many years to come.
Tim Rimington, North Manly, NSW.
Alternatives to centrifugal switches for motors
Regarding the discussion on speed controlling induction
motors with centrifugal switches (eg, January 2025 issue,
Mailbag, page 6), the ‘start capacitor’ is typically switched
out of the circuit at 30% of the maximum motor rotational
speed (RPM). The start winding has a thinner wire gauge
than the run winding and must be switched out as soon
as possible.
If it cannot reach the threshold RPM or it falls below it
during operation, the thermal switch mounted on the case
of the motor will trip and disconnect all the power to the
motor to save the start winding from burning out. These
motors are not designed to operate at low speeds. If you
want a lower speed than 30% (including a safety margin),
use a three-phase motor or a gearbox.
An interesting aside to this topic is that of electronic
motor capacitor start switches. They range from simple
timers that just give a time delay before switching out the
capacitor to complicated back-EMF sensing circuits used
to switch out the capacitor.
These switches are externally mounted, requiring the
installation of a wire from the start winding inside the
motor to the electronic switch outside the motor. They can
be retrofitted as a substitute for a failed internal mechanical switch.
For details about this subject, go to https://www.
stearnsbrakes.com/products/electronic-start-switches/
sinpac. These ‘SINPAC switches’ include multiple-
capacitor switches, reversing switches, capacitor
12
Silicon Chip
Australia's electronics magazine
siliconchip.com.au
siliconchip.com.au
Australia's electronics magazine
June 2025 13
start and run switches. All the wiring diagrams of the
different motor configurations they are used in are
available.
Advising someone about a motor may be a complex
business without at least using these diagrams to sort out
which type of motor is under consideration and research
into their characteristics.
I hope this helps. Don’t forget that electronics is fun!
Norman Boundy, Taylors Lakes, Vic.
Estimating transformer’s current capacity from its core size
I was interested in the question from B.P. of Dundathu,
Qld, in the April Ask Silicon Chip column, on how the
current rating of mains transformers relates to the size of
the wire in the secondary winding(s). This reminded me
of a very useful graph I have had since my brother gave it
to me in the late 1960s. He was doing an electrician’s training course in Adelaide at the time.
The graph shows the relation between the volt-amp (VA)
rating of a 50Hz transformer and the cross-section area of
the core; in particular, the area of the middle section of
an E-I transformer. Most non-toroidal power transformers
are of this type.
The area can be easily obtained by measuring the height
of the ‘stack’ of laminations and multiplying it by the width
of the centre leg of the E core. This gives you the area of
the core in, say, cm2. The graph from the 1960s is in square
inches, but it shows that the area of the core of a 100VA
transformer would be about 11.6cm2.
The graph is printed on paper with a log-log scale, but it
Silicon Chip - June .pdf
1
2/5/2025
12:25 pm
shows that the VA rating is directly proportional to the core
area. Double the core area, and the power rating is doubled.
Thus, if your correspondent can measure the area of the
transformer core, he/she can get a good approximation to
its power rating and dividing that by the secondary voltage will result in the rated secondary current.
Keith Gooley VK5OQ, One Tree Hill, SA.
Pico 2 USB connection problem was a failed solder joint
I built the Pico 2 Computer from your kit but the Pico2
wouldn’t go into bootloader mode. I knew it wasn’t a
problem with the cables or computer because, using the
same cables, a Pico 1 happily goes into bootloader mode.
Of course, I held BOOTSEL down as I connected the USB
cable.
I asked Geoff Graham for help; he thought it was a soldering problem with one of the pads that connects the Pico
2’s USB terminals to the Pico 2 board, or the soldering of
the USB socket used for programming.
I used a piece of tinned copper single-core wire pushed
into each hole, then cut it off to establish a bridge between
the PCB and the Pico 2, in case there was a gap that was
enough to discourage solder from joining them. That
worked!
Now I can wander down memory lane to when I first had
to use BASIC in 1978 while in the RAAF, using a Hewlett-
Packard HP9830 to manage aircraft repairable spares. BASIC
was not my first computer language – when I was studying
Aeronautical Engineering at RMIT in the early 1970s, we
had to use ALGOL 65. Fun times!
Thanks to Geoff Graham for taking the time to help me.
SC
Neil Biggar, Medowie, NSW.
®
Since introducing D-STAR in 2001, Icom has consistently pushed the
boundaries to refine and elevate the D-STAR experience.
14
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Australia's electronics magazine
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Report by
Dr David Maddison,
VK3DSM
The Australian International Airshow is held in Avalon, Victoria (near
Melbourne) each year and showcases the latest in aviation and
related technology. It features more drones each year, but there was
other interesting technology on show, too.
I
have reported on previous Avalon Airshows in the May 2013,
2015, 2019 & 2023 issues, so this
is my fifth report. It won’t include
aircraft or equipment I have reported
on before unless there have been significant developments since then. I
can’t describe everything I saw at the
airshow; there was simply too much,
so the following are the highlights of
this year’s show.
According to the organisers, over
200,000 people attended over six
days of the event. 350 aircraft were
displayed and there were 902 exhibitors from 28 countries. 291 delegations
attended from 43 nations, including
20 chiefs of air forces or similar, 65
conferences, symposia and presentations were held.
The show was enormous in scope,
as usual, and it was pleasing to see a
significant turnout from the Australian
aerospace industry. Here are the most
interesting exhibits alphabetically:
18
Silicon Chip
Airspeed Irukandji target
The Airspeed Irukandji (Fig.3, https://
airspeed.com.au/) is a supersonic practice target under development for the
RAAF. It uses an Australian-made solid
rocket motor, developed in conjunction
with Thales Australia and Defence Science and Technology Group.
It is said to be aerodynamically similar to the Beechcraft AQM-37 target
(not used by Australia), which was in
use from 1963 to 2022. That one relied
on difficult-to-handle hypergolic propellant (two components that spontaneously combust when brought into
contact). Airspeed is based in Mawson
Lakes, SA and testing is being performed
at the RAAF Woomera Range Complex.
ALADDIN Drone
The Aircraft Launched Aerial Delivery Drone (Fig.2) by Sovereign Propulsion Systems (www.sovps.com.au)
based in Seaford, SA is a drone that
can deliver payloads of 20–30kg for
Australia's electronics magazine
defence, search and rescue or disaster
relief applications. It is designed to be
launched out the back of an aircraft
such as a C-130 Hercules.
It has a six-minute flight time with
a 30kg payload, or a 25-minute flight
time with a 5kg payload, but no
range is specified. Maximum take off
weight is 65kg and the motors produce
39.6kW of power. The ‘drone head’ is
separate from the ‘payload module’;
the latter can be designed by third
parties for any required applications.
For rescues at sea, the ALADDIN
payload can be delivered directly to
the party being rescued, such as a
stricken boat, rather than the present
situation of dropping supplies in a
“helibox” package into the water for
the party to retrieve by themselves.
Ascent Aerosystems
Ascent Aerosystems is a US company that specialises in coaxial drones
(https://ascentaerosystems.com/).
siliconchip.com.au
Fig.1: a cutaway view of the
Aussie Invader 5R land speed
record attempt car.
Fig.2: the ALADDIN Air Launched
Delivery Drone on top of a 4WD.
Coaxial rotor drones have advantages over traditional quadcopter or
6/8-multirotor designs due to greater
ruggedness for commercial, military
and rescue operations. They are also
easy to store with folding rotor blades
and a cylindrical shaped body.
Guidance is achieved by adjusting
the pitch of the rotors and their differential speed.
The Helius model (Fig.4) weighs
249g, has a body size of 275 × 75 ×
53mm, a rotor diameter of 300mm,
flies up to 72km/h, a mission duration of 30+ minutes, carries a 12.3
megapixel low-light camera and has
a suggested price of US$4,499 (about
$7000).
The Spirit model (Fig.5) is 305mm
tall; its body is 106mm in diameter,
while the rotor diameter is 648mm.
Its maximum payload is 3.0kg and
the maximum take-off weight is
6.1kg. With two batteries installed,
mission duration is 58 minutes with
siliconchip.com.au
Fig.3: the
Australian
Irukandji
target drone
uses a solid
rocket motor.
Fig.4: the
Ascent
Aerosystems
Helius Nano
UAV uses
a coaxial
rotor design.
no payload or 32 minutes with maximum payload. Its top speed is over
100km/h.
You can see a video of the Spirit
model at https://youtu.be/J1tJGhiNrG0
and another about the Helius model
at https://youtu.be/6X_LIZwTXUM
Aussie Invader 5R
This beautiful vehicle is a contender
for the world land speed record, with
hopes of achieving 1,600km/h (see
Fig.1 & https://aussieinvader.com/).
The vehicle is rocket powered; its
Australia's electronics magazine
Fig.5: the Ascent
Aerosystems Spirit is larger
but also has coaxial rotors.
June 2025 19
Glossary
• UAV: Unmaned Aerial Vehicle, an
aircraft that flies autonomously or
by remote control (including what is
commonly referred to as “drones”).
• UAS: Unmanned Aircraft System, a
broad term that includes UAVs, plus
the ground control station, communications equipment and other support systems.
• VTOL: Vertical Take Off and Landing
propellant is white fuming nitric acid
(WFNA) as the oxidiser and turpentine as the fuel.
That propellant mixture is hypergolic, meaning the two components
spontaneously combust when combined. The combined weight of the
propellant is 2.8 tonnes, which will be
mostly consumed in 20 seconds. The
liquids are pressure-fed at about 70bar
(68 atmospheres) with no pumps for
the sake of simplicity.
The motor develops over 28 tonnes
of thrust and, after 20 seconds, the
vehicle will be travelling at 1600km/h
or 1km every 2¼ seconds.
At the expected speeds, there are
a range of physics and aerodynamic
behaviours that come into play; if
this record attempt is successful, it
is likely to stand for a very long time
as technology is being pushed to the
limit.
Currently, the Aussie Invader team
is looking for a long enough track to
run the record attempt. It cannot be a
salt lake due to a lack of grip; it needs
to be a desert-baked mudflat surface
at least 25km long; level, smooth and
straight, into which the wheels can
sink in by about 2.5cm to give extra
traction and stability. Sites are being
investigated in Australia (ideally),
South Africa and the United States.
Fig.6: a model of the ASA Roo-ver.
Australian Space Agency
(ASA) Roo-ver
The Roo-ver (see Fig.6 & https://
www.space.gov.au/meet-roo-ver) is
an Australian-made lunar rover that
is expected to go to the moon on an
Artemis mission. Artemis is a NASA
program to re-establish a human presence on the moon. The Roo-ver will
weigh about 20kg and be about the
size of a typical suitcase (as the ASA
describes it).
It will be controlled from Earth to
collect lunar soil and help to develop
capabilities necessary for an ongoing human presence on the moon.
Its mission duration is 14 days. The
lunar soil, also known as regolith,
will be studied as a source of oxygen to breathe and as an element of
rocket fuel.
The industry consortium building
the rover is called ELO2 and comprises start-ups, small- to medium-
size enterprises, major resource companies, universities and others. Roover is expected to go to the moon
later this decade. You can watch a
video about it at https://youtu.be/
hZ7Lb4VJbR4
Fig.7: the DroneSentry-X
Mk2 for detecting and
optionally defeating drones.
The Babcock Language
Translation System
The Babcock Military Aviation
Language Translation System is proposed to solve the apparent lack of
language comprehension of aviators
within some of Australia’s military
coalition partners.
However, according to the International Civil Aviation Organization
(ICAO), English is the mandated language for all aviation radio communications and procedures worldwide, at
least within civil aviation. Pilots are
expected to be proficient in “Aviation English”. The prevalence of the
language problem was not stated by
Babcock.
The translation system “… utilises
neural machine processing and edge
processing to deliver real-time translation of pilot-pilot, pilot-ATC, and
pilot-ground staff communications.
… This system employs aviation
Fig.10: a rendering of the Quickstep Brolga with DROPS
payload. Source: https://www.quickstep.com.au/qaam/
Fig.11: the Corvus Launcher V1 with an Innovaero Owl-B.
20
Silicon Chip
Australia's electronics magazine
siliconchip.com.au
Fig.9: an artist’s concept of the
Hypersonix DART. Source: https://
www.hypersonix.com/resources/
Fig.8: DroneSentry’s
medium-range product.
contextual understanding and deep
learning architectures to reduce the
cognitive burden of translation.”
Quickstep Brolga
Quickstep is an Australian company that received an Airshow award
for their electric multi-mission UAS
QU-1A Brolga (Fig.10 & https://www.
quickstep.com.au/qaam/). It has a 6m
wingspan, VTOL capability, can carry
payloads of 20–30kg for up to 100km.
Its automated payload interface can
find, identify and attach to the correct
payload. The payload container is a
proprietary system by TB2 Aerospace
(https://tb2aerospace.com/) called
Drone Recharging Operational Payload System (DROPS).
They also have a QU-3A Protean
model with a 45kg payload capacity, 750km range at 160km/h and a
hybrid powertrain using conventional
fuels and with onboard batteries for a
15-minute hover or payload exchange
time. For more details, see the video at
https://youtu.be/5vpbRwzottQ
Corvus Technology drone
launcher
Non-VTOL UAVs need some horizontal speed for launching, like
conventional winged aircraft. Corvus Technology Solutions (https://
corvustechnologysolutions.com/)
from Bayswater North, Vic, offers an
Australian-made Electronic Launch
System for any fixed-wing UAV.
The Corvus Launcher V1 (Fig.11)
siliconchip.com.au
can launch up to 360 UAVs per
hour, including ‘swarms’. It is silent,
battery-operated and mobile. It can
launch UAVs weighing up to 31kg at
around 90km/h. A custom cradle is
required for each type of UAV.
The Corvus Launcher V2 is under
development. It will be able to launch
120kg UAVs at up to 90km/h and
UAVs under about 20kg at 180km/h.
DroneShield
Small consumer or commercial
drones are increasingly being used
for hostile or unlawful acts such as
smuggling, airport disruption or terrorist attacks. DroneShield (www.
droneshield.com) is an Australian
company that specialises in C-UxS
(Counter Unmanned Systems), ie, the
ability to detect and disable drones.
They detect drones by a combination of radar and electro-optical sensors, using artificial intelligence to
identify hostile drones and to disrupt
their control, navigation and video
data links.
DroneSentry-X Mk2 (Fig.7) is suitable for mobile operations, such as
mounting to a vehicle or on a tripod
in the field. It has a detection range of
up to 3km and a disruption range up
to 500m. It weighs 46kg.
DroneSentry (Fig.8) is a modular
solution for close, medium or longrange detection (depending upon
configuration) and optionally defeating drones. It uses optical, radar, and
radio frequency (RF) sensors, edge
Australia's electronics magazine
computing systems and software to
produce comprehensive detection and
optional countermeasure solutions.
Information from these sensors is
correlated to provide maximum situational awareness for automatic
identification and response to UxS
intrusions or threats. DroneOptID is
DroneShield’s AI-driven computer
vision technology. It can also help to
determine the drone’s payload, modifications and effectiveness of countermeasures being applied to it.
The medium-range DroneSentry
product (shown in Fig.8) features four
Echodyne EchoShield radars, an HDC
Ranger MR UC infrared (FLIR) sensor
and a CompassOne navigation system
to provide location, direction and
heading data.
It connects to the DroneSentry-C2
command and control software
for sensor fusion and incorporates
DroneSentry-X Mk2 detection and
(optional) defeat capabilities.
Hypersonix Launch Systems
The Hypersonic Launch Systems
(www.hypersonix.com) DART (Fig.9)
is a test bed for hypersonic flight
and testing anti-hypersonic weapons. DART is 3.7m long and can fly
at Mach 7 (seven times the speed of
sound) for up to 1000km while carrying a 9kg payload. It uses a SPARTAN
fifth-generation air-breathing hydrogen fuelled scramjet (supersonic combustion ramjet) engine.
It has a 3D printed airframe and
June 2025 21
weighs 300kg. DART is launched with
unguided sounding rockets or guided
rockets. It is fully manufactured at
Carole Park in Queensland.
Elbit Systems
Elbit Systems (www.elbitsystems.
com) had numerous products on display, including the following pilot
low-light vision and helmet display
systems (see Fig.13):
• the BriteNite II night-vision sensor
array (video at https://youtu.be/
y8xvk0G2R-E)
• X-Sight helmet mounted display
(HMD) for helicopter pilots (video
at https://youtu.be/2rMK6p6r0rs)
• HDTS (helmet mounted display and
tracking system) – video at https://
youtu.be/uih6hA2uDR0
Honeywell Aerospace 757-200
We were invited on a demonstration flight of Honeywell’s 757-200 test
bed aircraft, tail number N757HW,
the fifth production 757 ever made. It
started service with Eastern Airlines
in 1983 and joined Honeywell (https://
aerospace.honeywell.com/) in 2005.
They stripped out the cabin linings
and most seats, reducing its weight
by around nine tonnes, and modified
it to take various equipment racks,
engineering stations (Fig.12) a third
engine mount (Fig.14) to test engines
under development and various electronic equipment. It is used as a test
and demonstration platform for the
Honeywell Aerospace products.
The systems they demonstrated
include:
• Satellite communications, such as
L-band and Ka-band hardware. We
were connected via onboard WiFi
to the internet using the high-bandwidth Ka-band Viasat Global Xpress
(GX) network via Honeywell JetWave X hardware. We then connected to Inmarsat’s global L-band
LAISR network, giving 3+3Mbps
data rates via Honeywell’s Aspire
hardware.
• Smart-X, Honeywell’s portfolio
of runway safety products. These
include Runway Awareness and
Advisory System (RAAS) and
SURF-A. RAAS gives alerts to the
pilot during ground and air operations to avoid collisions, and
includes optional SmartRunway
and SmartLanding software. It uses
GPS to determine an aircraft’s 3D
position, track and ground speed
22
Silicon Chip
and uses a detailed validated runway database of 3500 airports.
It gives audio alerts to pilots, such
as which runway they are approaching or on, which taxiway they are
on, warns of short runways, distance remaining for a rejected take
off, take off flap position, warning of
a possible taxiway landing, distance
remaining and other alerts.
SmartRunway and SmartLanding use aircraft position data and a
runway database to prevent runway
excursions or incursions.
SmartRunway prevents incidents
on the ground such as crossing the
wrong runway, crossing a runway
without clearance, or taking off from
a taxiway or short runway, or with
the wrong flap setting. SmartLanding
prevents incidents like running off the
end or the side of a runway, an off-
runway landing, landing on the wrong
runway or landing on a taxiway.
SURF-A enhances these by taking
data from the ADS-B Out (Automatic
Dependent Surveillance Broadcast
Out) equipment, using advanced
algorithms to identify any possible
collision and alerting the pilots.
ADS-B Out uses GPS and other sensors to give accurate position that is
broadcast to other aircraft (it is more
accurate for positioning than radar).
• Weather radar; the aircraft was
equipped with Honeywell’s next-
generation Intuvue RDR-4000 3D
weather radar that uses volumetric
scanning and pulse compression
technologies to provide a complete
view of the weather from sea level
to 18,300m altitude, with a 590km
detection range.
This allows for better avoidance of
adverse conditions; using it, a 50%
reduction in aircraft lighting strikes
was reported, and less pilot fatigue.
• Traffic Alert and Collision System
(TCAS) is a suite of systems that
operate independently from groundbased Air Traffic Control (ATC) for
collision avoidance. TCAS involves
two-way communication with other
aircraft equipped with appropriate
transponders. This enables a 3D map
to be produced, allowing each aircraft’s range, altitude and bearing to
be determined and establish whether
a possibility of a collision exists.
If a collision possibility exists,
the TCAS responders negotiate an
appropriate avoidance manoeuvre. The TCAS system also listens
for ADS-B information transmitted
from other aircraft. TCAS is mandated for aircraft over 5700kg take
off weight or that carry more than
19 passengers. Honeywell offers several TCAS solutions.
IAI APUS 25 long endurance
quadcopter
IAI (www.iai.co.il) has developed
a long-endurance quadcopter called
the APUS 25 (Fig.16), which has an
endurance of up to eight hours with no
payload. It achieves this using a single constant-RPM multi-fuel internal
Fig.12: an engineering test station in Honeywell’s 757. Note the stripped interior.
Australia's electronics magazine
siliconchip.com.au
combustion engine that drives four
variable-pitch rotors. It has a maximum payload capacity of 10kg (with
reduced endurance) and a maximum
takeoff weight of 25kg.
With a 5kg payload, its endurance
is five hours; electrical power of up to
300W is available to power payloads.
It can reach altitudes of 3353m and
can hover for extended periods due
to a liquid-cooled engine requiring
no airflow, so it can be used for persistent surveillance.
It has a maximum speed of 42 knots
(78km/h) and can operate in high
wind speeds, to 23 knots (43km/h). It
is suitable for various missions, such
as bushfire surveillance, and can perform disaster management, among
many other tasks. Multiple sensor
options are available. For more information, see the video at https://youtu.
be/9lQ3ohSG9ss
Fig.13: the BriteNite II night-vision sensor array, X-Sight helmet mounted
display and HDTS helmet-mounted display and tracking system.
Fig.14: Honeywell’s 757-200 has a third
engine mount for testing engines under
development.
Innovaero
Innovaero (https://innov.aero/) is a
Perth-based company. They are now
51%-owned by BAE Systems Australia and work jointly on various
projects. Among their products on
display were the STRIX Uncrewed
Aerial System (UAS), which we covered in the May 2023 article on the
Airshow of that year (siliconchip.au/
Article/15773).
Then there was the Owl A (Fig.15),
a precision loitering munition that
can carry a 1.5kg warhead and has a
range of 45km.
A loitering munition, also known
as a kamikaze drone, is a drone carrying a warhead that flies to an area of
interest, then waits in a holding pattern, looking for a target. If a target is
acquired, it is engaged. If no target is
acquired, the drone can return to base
to be recharged or refuelled for use on
another occasion.
The Owl B loitering munition
(Fig.17) is electrically powered and
designed to loiter for 30 minutes at
a range of up to 100km and return if
no target is acquired. Alternatively, it
Fig.16: the APUS 25 long endurance
quadcopter. Source:
https://www.iai.co.il/p/apus-25
siliconchip.com.au
Fig.15: the Owl A loitering
munition.
Fig.17: the Owl B loitering munition on a Corvus Launcher V1.
Australia's electronics magazine
June 2025 23
can have a maximum range of 200km
with no return capability.
Jabiru cargo drone
Fig.18: Jabiru’s JCQ50
cargo drone with a
JMIC trunk container
payload.
Fig.19: a rendering of
MIRAGE operating in ghost
decoy deception mode to
deceive an adversary’s
sensors. Source: https://
jackal-industries-dyfl0js.
gamma.site/
Fig.20: Kratos target drones; the MQM-178 Firejet
is in the front, with the BQM-177i behind it.
Bundaberg, Qld-based Jabiru
(https://jabiru.aero/) are well-known
in the recreational aviation and training markets for their one-to-four
seat composite light aircraft. At the
airshow, they displayed their new
JCQ50 “Donkey” cargo drone (Fig.18).
It is being developed with the support of the Australian Department of
Defence. The drone can carry a 50kg
payload up to 150km at a speed of
105km/h.
It has an unusual arrangement of
coaxial rotors for lift, powered by a
petrol engine, plus four electrically
powered twin rotors on booms (similar to a traditional quadcopter) for
steering, with electrical power for
them generated by the petrol engine.
This greatly simplifies the design of
the vehicle, as there are no complex
mechanisms as required for a traditional helicopter rotor.
The Donkey can be disassembled
and two can be carried in a standard
full-size JMIC trunk, a container used
by the Australian Defence Force and
other militaries (1016 × 609 × 406mm).
Donkey drones can be flown using
real-time remote control or in an
autonomous mode. They are powered by a petrol engine in a twin-V
four stroke configuration that produces 26.5kW.
Jackal Industries MIRAGE
Jackal Industries’ MIRAGE (Fig.19)
is an adaptable military drone that can
be reconfigured between the roles of
ISR (intelligence, surveillance, reconnaissance), deception and electronic
warfare/jamming.
Kratos target drones
Kratos had two target drones on
display: the MQM-178 Firejet and the
BQM-177i (see Fig.20).
The Firejet simulates of a variety of
threats. Its specifications are:
• Length: 3.3m
• Wingspan: 1.9m
• Dry weight: 59kg
• Engine thrust: 37kg
• Maximum launch weight: 145kg
• Internal payload capacity: 32kg
• Wingtip payload: 18kg total
• Wing station payload: 31.8kg total
• Top speed: Mach 0.69
Fig.21: the Phoenix
Jet target drone by Air
Affairs Australia has
a top speed of over
600km/h.
24
Silicon Chip
Australia's electronics magazine
siliconchip.com.au
• Maximum altitude: 10,670m
• Fuel capacity: 64.4L
• Oil capacity: 1.9L (for making
smoke)
Neumann Space
impulse bit (the smallest amount of
thrust per pulse) of 236μNs and a total
impulse (total thrust produced over
time) of 1000N.
It measures 96 × 96 × 100mm and
weighs 1.4kg fully fuelled.
For more details, see the video titled
“Lab Sweet Lab - How the Neumann
Drive Works” at https://youtu.be/
4TVipU98g9s
ACRUX-2 (www.melbournespace.
com.au/projects) is a low-cost satellite rideshare program using a volunteer model to help students get satellites into space.
The aim of this program is to take
a photo of Melbourne from low Earth
orbit (LEO). To do this, they are building a 3U CubeSat and a ground station.
The Neumanm Space company
(https://neumannspace.com/), based
in Kent Town, SA, has developed the
Neumann Drive, an innovative lowthrust electric ion drive for satellite
propulsion. It can be used for satellite
orbit raising, station keeping, formation flying and deorbiting.
Unlike some other low-thrust propulsion systems, it uses solid metal
as the propellant rather than liquid or
gaseous fuel, which greatly simplifies
its design and improves reliability. It
is a Centre-Triggered Pulsed Cathodic
Arc Thruster (CTPCAT).
It uses a fuel rod of just about any
metal (including scrap metal from
space junk) that is solid at the temperatures likely to be encountered. It turns
the metal into a plasma using electricity, which is ejected to create thrust.
A capacitor bank produces a
cathodic arc discharge to produce
short (~200μs) pulses at high current
(~3kA) and modest voltage (~200V) to
turn the metal into a plasma.
This plasma exhaust becomes
detached from the spacecraft and
moves away at velocities of tens of
kilometres per second, imparting
momentum to the vehicle.
No accelerator grids are necessary, as with other systems, and the
plasma is overall electron-rich and
therefore electrically neutral, which
means there are no spacecraft charging
problems.
The ND-50 model (see Fig.22) is
designed for CubeSats and SmallSats. It interfaces with the spacecraft via CAN or RS422, has a supply voltage of 28V, has a power rating of 50W, a pulse rate of 0.42Hz, a
specific impulse of 1800–2000s, an
Fig.22: the ND-50 Neumann
Drive for spacecraft maneuvering.
Fig.23: the Point Blank loitering drone by IAI.
The BQM-177i is designed to emulate an anti-ship cruise missile and
can sea-skim at an altitude of 3.1m at
Mach 0.95. Its specifications are:
• Length: 5.2m
• Wingspan: 2.1m
• Dry weight: 281kg
• Engine thrust: 453kg
• Maximum internal payload: 45kg
• Maximum wingtip payload: 78kg
• Fuel capacity: 238.5L
• Oil capacity: 8L (for making
smoke)
Macquarie University SkyLift
Drone
Macquarie University received
an Airshow award for their SkyLift
Drone, which is designed for parcel
delivery in multi-story residences,
directly to a recipient’s balcony.
We would like to provide more
information on this drone project, but
there was no reference to it on their
website at the time of writing (www.
mqdronelab.com).
Melbourne Space Program
ACRUX-2 Rideshare
siliconchip.com.au
Australia's electronics magazine
Phoenix Jet
The Phoenix Jet (Fig.21) is a target
drone manufactured by Air Affairs
Australia (https://www.airaffairs.
com.au/products/phoenix-jet-uav/)
for use by the armed forces. Its specifications are:
• Top speed: 330+ knots (600+km/h)
• Endurance: 1 hour
• Range: 100km range
• Minimum altitude: 15m
• Maximum altitude: 6000m
• Maximum launch weight: 66kg
• Payload: 3.5kg
• Engine thrust: 40kg
• Wingspan: 2.2m
• Length 2.4m
• Launched by: catapult
• Recovered by: parachute
Point Blank VTOL Precision
Strike Missile
Point Blank (Fig.23) by IAI is a
hand-launched VTOL loitering drone
that has the ability to hover above an
area of interest and observe. The operator can decide to either engage a target or return to base. It weighs 10kg
and is about a metre long.
Praxis Aerospace
Praxis Aerospace (https://www.
praxisaerospace.com.au), based in
June 2025 25
Fig.25: a Robinson CubeSat PCB assembly.
Fig.24: Pyxis in flight, its nose cone
assembly and internal electronics.
Brisbane, won an Airshow award for
its Sparrowhawk swarming UAS crop
sprayer.
Pyxis
Pyxis received an Airshow award
for a small thrust vectoring rocket
(see Fig.24). Their objective is to “...
develop a low cost and scalable guidance and control package for Australian Defence and space”. It has a wide
variety of suggested uses.
RAAF MQ-28A Ghost Bat
The Ghost Bat (Fig.29) is an
unmanned Collaborative Combat
Aircraft (CCA) being developed by
Boeing Defence Australia and the
RAAF. It will perform a range of
missions traditionally performed by
fighter aircraft, as well as assisting
with operations of crewed fighter
aircraft.
It is the first Australian-designed
combat aircraft to be produced in 50
years. Its maximum operating range
is 3700km.
RAAF Transportable Land
Terminal system and HCLOS
The RAAF and other parts of the
Australian military use several satellite ground stations for communications: the Panther (0.6m dish), Hawkeye III Lite (1.2m dish) and Hawkeye
III (two 2.4m dishes) – see Fig.30. They
can use the X, Ka and Ku bands.
The RAAF also uses the Panther II
Very Small Aperture Terminal (VSAT)
portable satellite ground stations built
by L3Harris (www.l3harris.com) – see
Fig.31. These are used with Ka-band
transceivers built by EM Solutions
(www.emsolutions.com.au), based in
Tennyson, Qld and now owned by UK
company Cohort PLC.
The Panther and Hawkeye terminals communicate with the Wideband Global SATCOM system (WGS),
a high-capacity United States Space
Force satellite communications system that is also accessible by the
Australian military because Australia funded one of its satellites, WGS6. The militaries of Canada, Denmark,
the Netherlands, Luxembourg and
New Zealand also have access, as they
funded WGS-9 as well.
There is also the RAAF High Capacity Line of Sight (HCLOS), which can
provide communications up to 80km
with a bandwidth of 5MHz, 10MHz,
20MHz or 40MHz at 4.4–5.875GHz
with a power between 0.5W and 5W
(see the centre of Fig.30).
Rafael
Rafael (www.rafael.co.il) had several products on display. One of particular interest was an active ‘hard
kill’ system to destroy hostile drones.
Systems that disrupt radio data links
and GPS to bring down a drone are
ineffective against fully autonomous
drones using inertial or optical terrain-
following navigation.
Fig.29: the Boeing Ghost Bat uncrewed jet fighter with one of Australia's 12 EA-18G electronic warfare aircraft behind it.
26
Silicon Chip
Australia's electronics magazine
siliconchip.com.au
Fig.26: setting up a
Robinson CubeSat.
Fig.27: a Rafael Typhoon 30 remote
weapons station (on the left) in a
recent test to destroy hostile drones.
The sensors on top of the tower help
to guide it. Source: Rafael.
However, Rafael’s Typhoon 30 RWS
(Remote Weapon Station), shown in
Fig.27, can be configured to shoot
down hostile drones. Australia and
several other countries use this system. For more details, see the video at
https://youtu.be/IZf0HLwTym0
RedTail
Australian company RedTail Technology (www.redtailtech.com.au)
have developed a counter-drone technology called “The Katoomba”, based
on a high-power laser beam capable
of delivering sufficient damage to a
hostile drone to disable it (see Fig.28).
Its beam is directed with the aid
of AI to ensure no invalid targets are
engaged, and there is a high probability of a hit. It can be mounted on
various platforms and is mainly for
use against inexpensive commercial
(hobby) drones, otherwise classified as
Group 1 according to the US Department of Defense classification scheme.
Robinson Aerospace Systems
an Adelaide-based company that
makes educational CubeSat kits called
RASCubes for schools, universities
and companies to build these tiny
10 × 10 × 10cm satellites – see Figs.25
& 26.
Students from across the world are
also designing and building payloads
that will be part of Project Space Call
and go into Robinson’s RASCube-1,
which will be launched into space;
see siliconchip.au/link/ac5r for more
details.
Shield AI V-BAT
The Shield AI (https://shield.ai/)
V-BAT is a combustion engine powered drone that can take off and lands
vertically but the rest of the time, it
Fig.28: two views of The Katoomba
anti-drone laser system. Source:
www.redtailtech.com.au
Fig.31:
an RAAF
Panther
satellite
ground
station.
Robinson Aerospace Systems
(www.robinson-aerospace.com) is
Fig.30: the Hawkeye III
Lite communications
dish (left) with a
Hawkeye III (right).
The HCLOS mast
is in the centre.
siliconchip.com.au
Australia's electronics magazine
June 2025 27
Fig.33: a Stralis fuel cell assembly.
Source: siliconchip.au/link/ac5u
Fig.32: a group of V-BATs operating in a swarming (they call it a “Teams”
configuration). Source: https://siliconchip.au/link/ac5t
flies horizontally (see Fig.32). It has a
mission duration of 13+ hours, using
a ducted fan for propulsion. It can
also hover by transitioning from horizontal flight.
It can fly autonomously in environments where communications are subject to electronic warfare. It optionally
has AI pilot software called Hivemind,
which allows drone-swarming or what
they call “Teams”. This is powered by
an Nvidia GPU loaded into V-BAT’s
modular payload bay.
It is 2.7m long, with a 3.0m wingspan, has a gross weight of 57kg, a
maximum speed of 90km/h, a service
ceiling of 6100m and a payload capacity of 18kg. It has infrared cameras for
surveillance; many other payloads are
available, including for satellite communication.
SiNAB
SiNAB (www.sinab.com) is based
in Taren Point, NSW. One of their
products is the Phoenix Pod, for long
range day and night surveillance and
live air-to-ground comms (Fig.35). It
has several applications in military,
training and civil purposes such as
bushfire spotting, mapping, border
protection and disaster management.
It can operate independently of
aircraft systems, and just needs to be
attached to an aircraft stores pylon.
Stralis hydrogen-powered
generator
Stralis (www.stralis.aero) received
an Airshow award for the development of their next-generation
high-temperature proton exchange
membrane (HTPEM) fuel cell to power
electric aircraft instead of batteries
(see Fig.33). By running the fuel cell
at a high temperature, it is six times
lighter than the current state-of-theart.
They state that their hydrogenelectric aircraft will travel ten times
further than battery-electric alternatives, and will be 50% cheaper
to operate than fossil fuel-powered
aircraft.
The fuel cell can be used in new
clean sheet design, to replace batteries
in existing electric aircraft, or to retro
fit an aircraft powered by an internal
combustion engine with electric
propulsion.
Stratoship Australia
Fig.34: Swinburne’s hydrogenpowered VTOL SHADE drone.
28
Silicon Chip
Stratoship (https://stratoship.au/),
based in Brisbane, is developing a
high-altitude solar-powered aerial
platform called Stratoship (see
Fig.36). It is intended to be stationed
at 20km altitude for various purposes
such as agriculture, bushfire spotting,
Australia's electronics magazine
communications relay, defence, security, natural disaster management,
observation of transportation and
infrastructure, research and others.
20km high is above most clouds
and jetstreams (9–15km), with relatively low wind speeds, and around
10km above commercial air traffic.
The coverage area is huge; an aircraft
at that altitude can see in a radius of
about 500km.
Stratoship is designed to provide
persistent surveillance for periods
from weeks to months. For more
on this concept, see our article on
“High-Altitude Aerial Platforms” in
the August 2023 issue (siliconchip.
au/Article/15894).
Swinburne hydrogen UAS
Swinburne University of Technology has introduced hydrogen fuel cell
technology into two different UASs
(uncrewed aerial systems), in a project known as H22S (Hydrogen to the
Skies) – see Fig.34 and siliconchip.
au/link/ac5s
Tests showed comparable or
enhanced performance compared to
an electric or internal combustion
engine UAS with a comparable takeoff weight and payload capacity.
One vehicle had a payload capacity of 2kg, stored hydrogen in a 10L
tank at 350bar of pressure, had an
8kW motor with hydrogen fuel cells
producing 3kW continuous power or
5kW peak, and had supplementary
lithium batteries.
UNSW (Canberra)
Cybersecurity
The University of NSW (Canberra)
received an Airshow award for a proposal to enhance Air Force communications security through lattice-based
cryptographic protocols that are
siliconchip.com.au
resistant to decryption by quantum
computers.
Fig.35: the SiNAB Phoenix Pod
provides long-range day/night
surveillance and air-to-ground
comms.
VeloDX
VeloDX (https://velodx.com/) has
developed an integrated AI “system
of systems” that supports all elements
of all drone operations, both on the
ground and in the air. Their drones
are the HOLI (extended range loitering munition), POD (AI avionics suite
for on-drone operations) and CASTLE
(the human-machine interface).
Vertiia long range hybrid
VTOL
Vertiia (www.amslaero.com) is an
Australian long-range hydrogen-electric VTOL aircraft with a 1000km
range, 300km/h top speed and triple
redundancy (see Fig.37). It can carry a
500kg payload, refuel in ten minutes,
is quiet (with a 65–70dBA noise level)
and has 70% lower operating costs
than a helicopter.
Apart from hydrogen, it can also
run on SAF (aviation biofuel), diesel or jet fuel. It can be configured for
medical transport, cargo or passenger
use. On the 18th of November 2024,
Vertiia completed its first free flight by
remote control and on battery power
at Wellington, NSW.
It’s said to be the most complex
civil aircraft ever developed in Australia. They have received orders for
26 aircraft. Hydrogen testing begins
this year.
Fig.36: a Stratoship
test-inflated with
helium.
Fig.37: Vertiia’s hybrid VTOL
aircraft. Source: https://www.
amslaero.com/our-product
Wisk
Wisk (https://wisk.aero/) now a subsidiary of Boeing, is developing what
they say is the world’s first all-electric
VTOL autonomous four-passenger air
taxi (see Fig.38). Apart from cost savings by not having a pilot, they say
most aircraft accidents are caused by
pilot errors, so by removing the pilot,
they expect to enhance safety.
While the vehicle is autonomous,
there is human oversight over operations at a flight operations centre,
where a person will oversee the flight
of numerous vehicles. They are currently working to obtain US FAA
approval for this aircraft. Its specifications are:
• Wingspan: 15m
• Range (with reserves): 144km
• Speed: 110–120 knots (200–220km/h)
• Charging time: 15 minutes
Forward thrust is produced by tilting one set of propellers.
SC
siliconchip.com.au
Fig.38: a rendering of
the Wisk air taxi.
Australia's electronics magazine
June 2025 29
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30
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B 0006
Hot Water System
Solar Diverter
Part 1 by Ray Berkelmans
& John Clarke
Solar-optimised hot water system (HWS)
heating using power purely from excess
solar generation
Solar export data is obtained from the
inverter and updated every five seconds
Shows operational parameters on a
2.4-inch OLED screen
WiFi logging of operational
parameters to a ThingSpeak database
every five minutes
Automatic override if the HWS
temperature is still cold by the end
of the solar day
Night-time power-down
Active heatsink cooling
Email alert (one per day) if
communication with the inverter
is lost
Over-the-air program updates
via WiFi
Manual override switch
You can save a lot of money with
this device! It lets you use excess
solar power generation to power
your electric water heater. It’s
a lot less expensive to put
together than an equivalent
commercial unit.
siliconchip.com.au
Australia's electronics magazine
Background Image:
unsplash.com/photos/sunset-view-5YWf-5hyZcw
June 2025 35
S
olar hot water diverters enable you
to use surplus electricity generated
by your solar photovoltaic system to heat water. Commercial versions have been around for decades,
although they are pretty rare to find.
The main reason is price; brand-name
diverters often cost upwards of $900,
with some (eg, Fronius) close to double that!
At that price, it is hard to justify the
up-front cost in terms of the savings.
Thankfully, this Solar Diverter can be
built for a fraction of that price!
In this era of ever-diminishing solar
feed-in tariffs, it makes sense to maximise consumption of your own solar
power. The reality is that often, when
you have plenty of solar energy to
export, the grid does not need it!
As of February 2023, all new solar
installations in Queensland above
10kVA require a Generation Signalling
Device (GSD) to be fitted so that electricity distributors can remotely curtail your solar feed-in when required.
Even without this, residential supply
voltages can often exceed 250V AC on
sunny days, causing most inverters to
shut down. Other states are considering similar so-called ‘backstop’ mechanisms.
A simple timer to
divert power to
a load during peak solar times is a
good start to optimising the usage of
the available solar power. However,
excess solar power is a highly variable thing with passing, or persistent,
clouds decreasing solar output by an
order of magnitude or more.
If you have a conventional hot water
system with an electric element, this
project will help you make the most
of your solar generation on those challenging solar days (see Fig.1).
If you have splashed out on a fancy
whole-of-home battery system, this
project will be especially useful,
because it will prevent your HWS
from sucking your battery dry during
the night and during poor solar conditions!
How it works
Our solar diverter consists of an
ESP8266 WiFi-enabled microprocessor that connects to your solar inverter
and reads the solar export data directly
from it.
If more than 0.5kW of power is
being exported, the microprocessor
produces a pulse-width-modulated
(PWM) signal with the duty cycle
being a percentage of the available
export power to the maximum power
demand of the HWS element.
We have an Aquamax 250L HWS
system fitted with a 3.6kW electric
heating element. So, for example, if
1kW of solar export power is available,
the duty cycle is set to 14% ([1kW –
0.5kW] ÷ 3.6kW). The duty cycle increments and decrements in steps of 2%
from 0 to 100% with each program
cycle, providing hysteresis during
highly variable conditions.
The PWM signal passes to a
zero-crossing detection (ZCD)
opto-coupler. This converts the PWM
signal to a timing suitable for switching a Triac with the AC mains waveform. A Triac typically needs to be
switched in synchrony with the sinusoidal(ish) mains waveform, switching it on near the zero voltage point
(zero crossing), either from positive to
negative or vice versa.
To do otherwise would cause unacceptably high peak currents and excessive electromagnetic interference
(EMI). Before zero-crossing detection
opto-couplers came along, the timing
of power switching is something that
had to be handled in software, with
voltage monitoring and interrupts or
with much more involved hardware
setups. With the ZCD opto-coupler,
we are spared from such complexity!
Obtaining solar export data
The solar export data is extracted
from your solar inverter by reading
the relevant register over WiFi using
the Modbus communication protocol. Before setting off to build this
project, you will need to establish
if your inverter supports Modbus and, if so, which register(s) contain(s) the solar
export data needed.
The finished and wired
Hot Water System
(HWS) Solar Diverter.
Note the two visible
acrylic covers (green
and clear acrylic),
which are placed
to prevent contact
with high-voltage
components.
36
Silicon Chip
Australia's electronics magazine
siliconchip.com.au
Fortunately, most modern inverter
manufacturers have subscribed to the
SunSpec Alliance, which sets open
information standards for the Distributed Energy Resource industry. You
can see if your inverter manufacturer
is part of the alliance by checking the
membership at https://sunspec.org/
members/
Even if you don’t see your inverter
manufacturer listed, not all hope is
lost. For example, my manufacturer,
SolarEdge, is not listed, yet they still
comply to the SunSpec Modbus standard and provide a very detailed
Application Note (siliconchip.au/link/
ac4z) to guide users through the hundreds of registers.
You will need to do some research
to find out which register addresses
are used by your inverter. Be aware
that some models don’t have Modbus enabled by default. Check your
inverter instructions and/or with your
solar installer.
To test whether your inverter is
compliant, and to explore its data registers, you can download a Modbus
simulation tool such as Modbus Poll
(www.modbustools.com), which has a
free 30-day trial. Under the “Connection” tab, you simply enter the LAN IP
address for your inverter (check your
network client list in your router),
together with your server port.
Most inverters use a default port of
502, but SolarEdge uses 1502. Under
“Setup → Read/Write Definitions”,
select the slave ID (the default is 1)
and enter a start register address like
40001. After hitting OK, Modbus Poll
will then display the content of the
next ten registers.
Until recently, my inverter was a
three-phase Solar Edge SE-10K model.
Since our house and HWS are connected to phase C, the most relevant
register is 40209: “Phase C AC Real
Power”. Readings are displayed in
watts (int16) with solar export shown
as positive values and grid import as
negative values.
During development of this project, we upgraded our solar system
to a Sigenergy 5-in-1 battery with an
integrated 25kW, 3-phase inverter. It
stores its export data as 32-bit integer (int32) values, which are spread
across two registers. For us, they are
30056 & 30057.
Its export values are the opposite
of the SolarEdge’s: negative for export
and positive for import. The SigEnergy
siliconchip.com.au
Fig.1: this shows why having a HWS Solar Diverter may be required to
make the most of your solar power during highly variable solar conditions.
Modbus protocol can be found at
siliconchip.au/link/ac50
WiFi
It is worth ensuring you have an
adequate WiFi signal at the point
where you intend to mount the Solar
Diverter. There are many free smartphone apps that will show your WiFi
signal strength. You will need at least
-70dB for a reliable WiFi connection.
Otherwise, you may need to invest in
a WiFi range extender.
HWS element
The other check you should make
before launching into construction is
to ensure that your HWS has a resistive heating element and is not a heatpump or another type of HWS. If it
has an element, its specification will
be written on the compliance plate,
possibly near the base of the HWS.
A rating of 3600W or less will confirm that this design is suitable for
your HWS.
Circuit details
The full circuit is shown in Fig.2.
MOD2 is the microprocessor module
that communicates with the inverter
and generates the PWM signal from its
GPIO14 pin. That is fed to OPTO1, a
MOC3083 zero-crossing opto-coupler
Australia's electronics magazine
Triac driver. This features a low 5mA
trigger current (IFT) and high isolation,
with a rated peak blocking voltage of
800V between the line and control
circuitry.
Current flowing through OPTO1’s
internal LED generates an infrared signal that triggers the monolithic silicon
detector, then its internal Triac and
finally the external Triac to switch the
HWS load. The 360W resistor on pin
1 of OPTO1 was chosen to supply the
necessary current to trigger the LED.
This is calculated as (3.3V – 1.5V)
÷ 5mA, where 3.3V is the supply
voltage, 1.5V is the LED forward voltage and 5mA is the trigger current.
When a sufficient LED current (IFT)
is supplied and the AC line voltage
approaches the zero point, the Triac
driver latches on. This introduces a
gate current in the main Triac, triggering it from the blocking state into
full conduction.
The main Triac here is a BTA41800B, capable of handling up to 40A
RMS; more than ample for our ~15A
RMS heating element load.
We recommend fitting the 360W
resistor at pin 6 of OPTO1, as it prevents the Triac driver from being damaged in applications where the load is
inductive. It helps to limit the gate trigger current (Igt) if there is a transient
June 2025 37
Fig.2: the HWS Solar Diverter circuit is based around MOD2, an ESP8266 microcontroller with WiFi. IC1-IC3 provide a
way to monitor the current drawn by the HWS while OPTO1 and TRIAC1 provide PWM control of the HWS element, so
its power draw can be modulated.
in the mains waveform while the Triac
driver was off.
The 330W (1W) Triac gate resistor provides better noise and thermal immunity when the internal gate
impedance of the Triac is high, which
is the case for sensitive-gate Triacs.
These resistors are 1W types mainly
for their voltage rating.
An externally mounted 20A 250V
override switch (S2) allows you to
bypass all electronic control circuitry,
if required, and force the HWS element on.
38
Silicon Chip
Current monitoring
While current sensing isn’t an essential part of the circuit, it provides a
helpful insight into how well the circuit is working.
The main current-sensing element
is an ACS770LCB-050B 50A bidirectional current sensor (IC1). A TLC2272
dual operational amplifier (IC2) buffers the output of the current sensor,
feeding an ADS1115 16-bit analog-todigital converter (ADC), IC3.
So IC1 converts the load current
into a voltage which is buffered by
Australia's electronics magazine
IC2, then converted to a digital value
by IC3 and passed to the microcontroller. The ADS1115 is the fastest available ADC that communicates using an
I2C serial bus, with a sampling rate of
up to 860 samples per second. This
is about the minimum acceptable for
accurately sampling the AC current
waveform.
Since each complete AC sinewave
lasts 20ms, this provides us with a bit
over 16 samples per full wave. When
measured over 100 cycles (two seconds), that gives us a fair estimate
siliconchip.com.au
Fig.3: the PCB is populated
with a mixture of SMD and
through-hole components.
Note the three acrylic covers
over OPTO1, IC1 and the
mains terminals that prevent
accidental contact with
high-voltage parts. During
assembly, be careful to fit
OPTO1, IC2 and IC3 with the
correct orientations; other
parts are polarised, but their
correct orientations should
be obvious.
between IC3 and MOD2.
This is performed by general-
purpose N-channel Mosfets
Q2 & Q3, plus a few 10kW
pull-up resistors.
They reduce the voltage
levels of the SCL and SDA
lines from 5V at IC2 to 3.3V
at MOD2 & MOD3, while still
allowing bi-directional communication.
Two temperature sensors (DS18B20s) connect via
CON5 and CON6 for monitoring the HWS and heatsink
temperatures.
CON2 provides a connection for a light-dependent
resistor (LDR), which allows
our circuit to go into sleep
mode when the sun goes
down.
Momentary switch S1
and associated 47kW resistors and a 100nF capacitor
form the reset circuitry of
the ESP8266. The CON10
header and jumper JP1 provide a means for programming the microcontroller on
the ESP8266 module.
Power supply
of the current flow. ADCs that communicate using an SPI serial bus can
sample faster, but require a few extra
pins on the microprocessor, which we
don’t have.
Since we already have another I2C
device in our circuit, the 2.4-inch,
128 × 64 pixel monochrome OLED
siliconchip.com.au
screen, communication with both
devices required just two of MOD2’s
pins (GPIO4 & GPIO5).
The current sensing components
operate at 5V to give sufficient resolution, while the microcontroller
is strictly a 3.3V-tolerant device, so
we need some digital level shifting
Australia's electronics magazine
DC power for the circuit is
derived from a PCB-mounted
230V AC to 5V DC power
supply (MOD1), which has a
250mA fuse (F1) in case of a
fault. The 5V rail powers the heatsink
fan (FAN1, connected via CON4) and
the components involved in sensing
the current drawn by the HWS element.
CON3 provides a handy way of powering the circuit with a 5V DC power
supply, or a 3.7V (nominal) Li-ion/
LiPo battery, so programming and
testing can be done without having to
connect AC mains power.
June 2025 39
The 3.3V rail is derived from the
5V DC bus via low-dropout linear
regulator REG1 (AP7365). Other LDO
regulators in the same SOT-23-5 package would be equally suitable (eg,
ME6211, MCP1802T or TPS7A2033),
provided they can supply at least
250mA and have a compatible pinout.
Construction
The first step is to create the PCB
assembly, which can then be mounted
in a plastic box and wired up. The Solar
Diverter is built on a double-
sided,
plated-through PCB with a red solder
mask that’s coded 18110241 and measures 134 × 207.5mm. It is installed
within an enclosure measuring 222 ×
146 × 55mm. The locations of components on the PCB are shown in Fig.3.
Many (but not all) of the components used are surface-mount types
that can be soldered by hand using
a fine-tipped soldering iron. Starting from the smallest component and
working up to the largest, solder one
end first (for capacitors and resistors) or one lead first (for the ICs and
MOD2).
Make sure the component is lined
up with the other pad or pads; if necessary, remelt the initial solder joint
and gently realign the part before soldering the remaining pins. If any solder bridges form between IC leads,
they can be cleared using solder wick.
Adding a small amount of flux paste
from a syringe will make both soldering and clearing bridges easier.
For MOD2, apply solder over the
outside edges of the pads on this module to join them to the PCB pads, treating it like the large surface-mounting
part that it is.
For the through-hole parts, such as
the 1W resistors, switch S1, OPTO1
and IC1, insert the leads through the
associated PCB holes and solder them
on the underside of the PCB. All polarised parts, including OPTO1, IC2 and
IC3, must be orientated as shown in
Fig.3 for the circuit to work.
IC1 has large, high-current leads
that must be soldered on both the top
and bottom sides of the PCB to ensure
low-resistance connections.
The three 45A two-way barrier terminal connectors (CON7, CON8 &
CON9) require sufficient solder and
heat for the solder to flow over the full
underside pad and to the connector
terminals to provide low-resistance
connections.
40
Silicon Chip
Parts List – Hot Water System Solar Diverter
1 double-sided plated-through PCB coded 18110241, 134 × 207.5mm
1 ABS enclosure, 222 × 146 × 55mm
[Jaycar HB6130 (ABS) or HB6220 (Polycarbonate)]
1 100 × 110 × 33mm heatsink cut to 100 × 70 × 33mm
[Altronics H0563 with half the fins cut off (see text)]
1 40mm 5V fan (FAN1) [Altronics F1110 or DigiKey 102-4361-ND]
1 M205 fuse holder with cover (F1) [Altronics S5985]
1 M205 250mA fast-blow fuse (F1)
1 Light-dependent resistor (LDR1) [Jaycar RD3480, Altronics Z1619]
1 SPST pushbutton two-pin switch (S1) [Jaycar SP0611, Altronics S1127]
1 20A 240V AC IP66 weatherproof switch (S2) [Bunnings I/N 4430626]
1 3-6.5mm cable gland, for LDR and TS2 wiring
1 OLED display bezel (see text and Fig.5 next month)
Connectors
1 4-pin JST XH header with 2.54mm spacing plus matching plug (CON1) *
3 2-pin JST PH headers with 2mm spacing plus matching plugs
(CON2-CON4) *
2 3-pin JST XH headers with 2.54mm spacing plus matching plugs
(CON5, CON6) *
3 45A 600V 2-pin barrier connector strips, 0.5-inch/12.7mm pitch (CON7-9)
[DigiKey YK7010223000G-ND]
1 3-way polarised pin header with 2.54mm pin spacing (CON10)
1 2-way pin header with 2.54mm pin spacing (JP1)
1 jumper shunt (JP1)
* all available in the Jaycar PT4457 JST Connectors Kit
Hardware
1 3mm-thick sheet of clear acrylic, 340 × 307mm (for weather shield)
1 acrylic or fibreglass piece, 106 × 79.5 × 3mm (see Fig.5 next month)
1 acrylic or fibreglass piece, 32.5 × 15 × 1.5mm (see Fig.5 next month)
1 acrylic or fibreglass piece, 26 × 33 × 1.5mm (see Fig.5 next month)
1 transistor clamp to secure TS1 to the heatsink [Jaycar HH8610]
2 5.3mm inner diameter crimp eyelets suitable for 2.5mm2 wire
1 M4 × 15mm panhead machine screw
1 M4 × 10-12mm panhead machine screw
4 M3 × 12mm tapped spacers
8 M3 × 6.3mm tapped spacers
2 M3 × 20mm panhead machine screws
2 M3 × 15mm panhead machine screws
6 M3 × 12mm panhead machine screws
2 M3 × 10mm panhead machine screws
13 M3 × 5mm panhead machine screws
2 M4 star washers
6 M3 flat washers
3 M4 hex nuts
10 M3 hex nuts
This is what you
will typically see
displayed on the
OLED screen. It
is mounted to the
lid of the case
as shown in the
photo opposite.
We have glued
it onto the case
for a flush fit,
but you might
prefer to use
the standoffs to
screw it in.
Australia's electronics magazine
siliconchip.com.au
2 20mm or 25mm corrugated conduit glands
[Bunnings I/N 4330875 or 4330876]
1 small tube of thermal paste
Cable & conduit
3 lengths of 4-core shielded cable for the DS18B20 temperature sensors
and LDR, length to suit installation [Jaycar WB1510, Altronics W3040]
3 lengths of 2.5mm2 round cable or 2.5mm2 flat twin and Earth for S2,
mains input and mains output wiring [Bunnings I/N 4430139 or 4430080]
lengths of 20mm or 25mm conduit, to suit installation
Modules
1 Meanwell IRM-03–5 5V/3W AC-to-DC converter (MOD1)
[DigiKey 1866-3020-ND]
1 ESP8266 – ESP-12F programming and development board (MOD2)
[AliExpress, eBay]
1 2.42-inch 128×64 I2C OLED display module (MOD3)
[AliExpress 1005006267098554 or 1005006267098554]
Semiconductors
1 ACS770LCB-050B-PFF-T bidirectional current sensor (IC1)
[DigiKey 620-1541-5-ND]
1 TLC2272CD dual op amp (IC2) [DigiKey 296-1305-2-ND]
1 ADS1115DGSx 16-bit ADC (IC3) [DigiKey 296-24934-2-ND]
1 MOC3083M opto-isolated Triac driver (OPTO1) [DigiKey MOC3083M-ND]
2 DS18B20 temperature sensors (TS1, TS2)
[DigiKey 4518-DS18B20-ND, Altronics Z7280]
1 AP7365-33WG-7 3.3V linear regulator (REG1) [DigiKey AP7365-33WG-7]
3 BSS138 N-channel Mosfets, SOT-23 (Q1-Q3)
[DigiKey 4530-BSS138TR-ND]
1 BTA41-800BQ 800V 40A Triac, TO-3P (TRIAC1)
[DigiKey BTA41-800BQ-ND]
Capacitors (all SMD M2012/0805-size X7R ceramic)
1 22μF 6.3V
2 10μF 16V
1 1μF 50V
5 100nF 50V
Resistors (all SMD M2012/0805-size ⅛W unless noted)
2 47kW
5 10kW
1 6.8kW
1 4.7kW
1 2.2kW
1 360W
1 360W axial 1W [DigiKey 738-RSMF1JT360RCT-ND]
1 330W axial 1W
1 120W
MOD1 (the 230V AC to 5V DC converter) and fuse holder F1 can be
installed now. With the holder soldered to the board, insert the M205
250mA fuse, then the transparent
cover can be clipped over the top.
Connectors
There are several different types of
connectors used on the PCB. These
include a 4-pin XH JST plug and socket
with 2.54mm spacing for CON1; 2-pin
PH JST connectors with 2mm spacing
for CON2, CON3 & CON4; and 3-pin
XH JST connectors with 2.54mm pin
spacings for CON5 & CON6. These are
available in the Jaycar JST Connectors
Kit (PT4457) or separately from online
suppliers.
The 3-way pin header with 2.54mm
pin spacing for CON10 and the 2-way
pin header with 2.54mm pin spacing
for JP1 are standard headers available
in strips.
Heatsink & Triac mounting
The Altronics H0563 heatsink is
supplied with cooling fins on either
side of a central flat area for mounting
power transistors in TO-3 packages.
For our design, one side of the heatsink
with fins will need to be removed so
the TO-3P packaged Triac can mount
on the central flat area. Cut it off using
a hacksaw, leaving a 30mm wide flat
section next to the fins (see Fig.3).
Use the PCB as a template to mark
the six holes required, then remove
the heatsink and drill them. Place the
heatsink on the PCB and check they
all line up. Bend the Triac leads at
right angles so it can be mounted tabdown onto the heatsink with the leads
inserted into the PCB pads.
The Triac tab is electrically isolated
from the A1 and A2 leads, so an insulating washer is not required. Apply
a thin layer of thermal paste (heatsink
compound) between the Triac tab and
the heatsink to improve heat transfer.
Secure the Triac with an M4 machine
screw and nut, then solder the Triac
leads to the mounting pads on the PCB.
Next month
Warning: Mains Voltage
This Solar Diverter operates directly from the 230V AC mains supply; contact with any live
component is potentially lethal. Do not build it unless you are experienced working with
mains voltages. A licenced electrician is also required to install the project.
At this stage, we are ready to prepare the case to install the PCB, wire
it up and start testing. We’ll have the
details on how to do that in the final
article next month, with detailed testing instructions, as well as information
on the final installation, setup, calibration and use.
SC
June 2025 41
Altium
Designer 25
Review by Tim Blythman
Altium Designer 25 is the latest version of the EDA (electronics design automation) software
that we use for all of our PCB designs. This new version was released late in 2024, and we
have spent some time putting it through its paces. Here is what we have found.
W
e have used related products for our
PCB designs for over 30 years, starting with Protel Autotrax! So
we were keen to see what has been
updated since our review of Altium
Designer 24 from August last year
(siliconchip.au/Article/16425).
Since that article was written, there
is the news that Renesas Electronics
has acquired Altium; the acquisition
was completed in August 2024. Renesas is a Japanese semiconductor manufacturer that includes the semiconductor operations of companies like
Hitachi, Mitsubishi and NEC.
That marks an interesting geographical history for Altium, with Protel
Systems Pty Ltd originally founded
as an Australian company. For many
years, it has been headquartered in San
Diego, California.
We’re most familiar with Renesas
Electronics as the manufacturer of the
RA4M1 microprocessor used in the
new Arduino Uno R4 microcontroller board we reviewed in December
2023 (siliconchip.au/Article/16047).
The Raspberry Pi 5 also uses a Renesas power management IC.
AD25 overview
Altium Designer 25 looks and feels
much the same as previous versions,
but like many modern applications, it
is constantly evolving. This time we
are looking at version 25.0.2.
The webpage at www.altium.com/
documentation/altium-designer/new
lists details of the various version
updates and the versions (and subversions) to which they apply. So you can
42
Silicon Chip
easily see which version has a particular feature.
Some features that are present are
disabled by default but can be turned
on via the Advanced Settings window
of Preferences. Others are available
as Extensions, which can be installed
from the Extensions and Updates window. Such features may still be at the
beta testing stage.
Beta testing means that the feature
is essentially complete but not fully
tested. It may still be changed if users
find bugs. It is a good way to get early
access to novel features, and there is
usually the ability to toggle these features on and off.
Just as with previous versions, it is
possible to install multiple versions of
Altium Designer alongside each other.
You might like to do this to try out the
features in a new version without committing to it until you are happy with
the changes.
Amongst other videos, the new features are also presented at the Altium
Academy YouTube channel (www.
youtube.com/<at>AltiumAcademy).
These and other training materials are
also available on the Home Page of the
Altium Designer application.
Performance
Altium Designer 25 claims to have
much improved performance, especially with large designs. Our designs
are typically on the smaller and less
complex side, so we’re not really able to
put this aspect to the test. But we were
certainly happy with its responsiveness
in the time we’ve been using it.
Australia's electronics magazine
This applies to many aspects of
Altium Designer, including the schematic and PCB editors, and Draftsman,
as well as in collaborative tools like
Altium 365 and PCB CoDesign.
Operations like opening documents, repouring polygons, placing
stitching vias and bulk copying and
pasting have all been sped up. These
improvements have been brought
about through better memory management and caching of data where
possible.
On a related note, recent versions of
Altium Designer (starting with 24.8)
use the newer .NET 6 software framework. Previously, Altium Designer
used Microsoft’s proprietary and now
obsolete .NET Framework 4.8. Unsurprisingly, .NET 6 is also faster.
Interestingly, .NET 6 is fully opensource. It is intended to be modular and works across multiple platforms (including Windows, Linux and
macOS). Dare we wonder if this is the
first step of being able to run Altium
Designer on a Linux PC or Mac?
The SI Analyzer by Keysight
Another extension that sounds quite
handy is the Signal Integrity Analyzer
by Keysight, although this is another
one that we probably won’t ever need
to use due to our modest designs. As
the name suggests, it is intended to
perform signal integrity analysis on
high-speed designs. Fig.1 shows the
phases of such an analysis.
It can calculate things such as
impedance, delay, insertion loss and
return loss based on the PCB layout.
siliconchip.com.au
Fig.1: the Signal Integrity Analyzer by Keysight
can be used post-layout to validate signal integrity
and provide checks on parameters such as
impedance, delay, insertion loss and return loss.
This will be very handy to validate high-speed
designs before committing to PCB manufacture.
Source: www.altium.com/documentation/altiumdesigner/new?version=24#sianalyzer-by-keysight-openbeta-24-10
Fig.2 (below): this trace is
‘necked down’ to fit through
a narrow gap between other
pads; we did this manually,
using an older version of
Altium Designer. The new
auto-shrink feature allows
this to be done automatically
during interactive routing.
This can help to validate the PCB
before it is committed to manufacture. Signal Integrity Analyzer is currently a beta feature and requires the
SI Analyzer by Keysight extension to
be installed; there is a free 14-day trial
available for this feature.
Routing
When routing the traces on a board,
it is sometimes necessary to use a track
narrower than the preferred width to fit
through a congested or tight area. This
is often described as ‘necking down’,
where the trace is narrowed down to
a thin neck just long enough and narrow enough to fit.
Previously, you would have to do
this manually, but there is now an
option to auto-shrink the width to the
minimum you’ve set.
This will be handy, since manually
creating a neck can be a fiddly process, especially if you want the result
to be neat. In addition, a new design
rule allows the neck to have a maximum specified length, to avoid having too much resistance or increased
fragility.
siliconchip.com.au
Currently, both these features are
in beta and need to be activated in
Advanced Settings. The auto-shrink
feature is enabled with the “PCB.Routing.EnableAutoShrinking” option,
while the neck-down rule follows
the “PCB.Rules.RoutingNeckdown”
setting.
There is also an option to centre
traces when routing. Typically, the
auto-router will place traces at the
minimum allowed clearance from the
nearest track, but spreading the traces
out may be preferred. It can also make
the routing neater, since the traces will
be spread out more evenly.
This is also a beta feature and is
set with the “PCB.EnableTraceCentering” advanced setting. Fig.2 shows
an example of a trace necking down
through a narrow gap on our Thermal
Controller PCB from March & April
2020 (siliconchip.au/Article/12584).
Single-layer PCBs
For simple designs, a single-layer
PCB (with copper on just one side) can
be an economical choice, especially for
designs on flexible substrates. Large
Australia's electronics magazine
production runs can warrant the savings in eliminating a copper layer
where that is feasible.
It’s now possible to lay out single-
layer PCBs by enabling the “PCB.
SingleLayerStack.Support” option
in Advanced Settings, then removing a copper layer from a two-layer
PCB stack.
Constraint Manager
The Constraint Manager unifies
design constraints from both the schematic and PCB layout. It works in place
of the PCB Rule and Constraints Editor
dialog (Design Rules).
A project can be set up (at creation)
to use the Constraint Manager or to
use the older Design Rules. There is
also a tool that can convert a project from using Design Rules into one
that is compatible with the Constraint
Manager.
It provides a hierarchical system
that is automatically translated into
the priority in which rules are applied.
Constraint Manager can be enabled by
setting the “System.ConstraintManager” option in Advanced Settings.
June 2025 43
Source: www.altium.com/
documentation/altium-designer/
constraint-manager
Fig.3: the Constraint Manager
provides a new interface for
managing design constraints
(design rules) across a project.
Older projects can be upgraded
to use the Constraint Manager.
Fig.3 shows some views of the Constraint Manager.
Importing
Occasionally, we have to deal with
contributed PCBs that have been
designed using a different EDA tool,
and sometimes we need to change
them. This might be as simple as making a small change to the silkscreen
markings or could involve a major
revision of the copper routing layers.
Some changes can be made by
directly editing the Gerber files, but
having access to fully editable PCB
design files is better for many reasons.
Firstly, that makes it possible to run
design rule checks to validate that any
changes do not cause a manufacturing issue like shorted traces. It then
becomes possible to make further revisions if needed in the future.
Whatever the reason, this means that
we need the ability to import designs
from other EDA tools into Altium
Designer so that they can be turned
into native Altium Designer files, such
as SchDoc schematic files or PcbDoc
PCB files.
The latest version of the importer
now works with KiCad designs from
44
Silicon Chip
KiCad version 7 or 8. This is available
as an extension known as the KiCad
Importer Extension and can be found
in Extensions and Updates.
Their website at siliconchip.au/link/
ac41 has more information on importing designs from other tools. Fig.4
shows a screenshot from our installation of the Software Extensions that
are on offer.
We have previously mentioned the
free online Altium 365 Viewer, which
is at www.altium.com/viewer
This now supports KiCad files, and
we had no trouble using it to view
some KiCad PCB files that we found
online.
Wire bonding
Altium Designer can be used for
designing much more than just traditional planar substrate PCBs. We have
previously covered Altium Designer’s
ability to work with flexible and hybrid
(rigid-flex) PCBs, printed electronics
and 3D-printed substrates using the
3D-MID (three-dimensional mechatronic integrated device) process.
Another example is the recent Harness Designer. (Also see our article on
3D-MID technology in the April 2025
Australia's electronics magazine
issue at siliconchip.au/Article/17936).
One of the technologies supported
by Altium Designer 25 is COB (chipon-board) using wire bonding. COB
involves bare silicon chip dies being
bonded directly to a PCB. Connections
are made from pads on the die (die
pads) to the bond finger pads on the
PCB by means of bond wires.
The bond wires used in COB applications are much the same as the bond
wires used to connect a silicon chip to
its leadframe in a traditionally packaged integrated circuit. These are very
fine wires of a metal such as gold, copper or aluminium that are welded to
their pads using heat, pressure or ultrasonic energy.
The process is typically performed
by an automated robotic system. You
can see some images of a COB design
at www.altium.com/documentation/
altium-designer/wire-bonding while
the photos at upper right shows two
examples of silicon dice bonded to
a PCB.
Creating a COB design involves adding a Die layer and a Bond wire layer
to a PCB document or library. A complete footprint ‘package’ including die
pads, bond finger pads, and bond wires
siliconchip.com.au
Fig.4: numerous Altium Designer extensions can be installed from the
Extensions and Updates tab. This shows just some of the extensions available on
our system.
can be created, in which case the bond
finger pads can be simply routed to on
the copper layers.
Alternatively, a die with die pads
can be placed alongside separate bond
finger pads. The bond wires are then
placed manually. With the current version, wire bonding can be enabled with
the “PCB.Wirebonding” option in the
Advanced Settings dialog. For manufacture, a wire bonding table report
can be generated.
As you can see from Fig.5, Altium
Designer’s 3D rendering allows you to
see all aspects of a wire-bonded design.
For example, you can visually check
that crossed bond wires pass at different heights to avoid collisions. We
find the 3D views invaluable for making sanity checks on our PCB layouts.
There are three different subscription levels available for Altium
Designer: Standard, Pro and Enterprise. They differ in the number of features that are included and more information is available at www.altium.
com/altium-designer/licensing
In addition to covering the important aspects of a feature (in this case,
Single-layer PCBs), it follows with a
live demonstration of how to use that
feature within Altium Designer.
The free trial offer that we have mentioned in previous years is still available. It allows you to use a fully featured trial version of Altium Designer
for 15 days; see www.altium.com/
altium-designer/free-trial
Resources
Conclusion
Altium offers numerous resources
to allow users to make the best use
of Altium Designer. You can view a
recent webinar (recorded in November) at siliconchip.au/link/ac42
Altium continues to make incremental updates to Altium Designer.
While there are some bigger features
that we would struggle to use fully,
such as wire bonding, they are no
doubt useful for larger organisations.
It is good to see that they continue to
improve usability and work on basic
features such as routing.
We hope that the switch to .NET 6
is the beginning of cross-platform support. We’re especially keen to be able
to use Altium Designer on Linux, since
so many of the other programs that we
use already allow that.
For more information on Altium
Designer, visit www.altium.com/
altium-designer
SC
Licensing
Fig.5: Altium Designer 25
now allows wire bonding
between silicon dies and
PCBs. This image shows
an example of two COB
(chip on board) dies
bonded to the PCB below.
Source: www.altium.
com/documentation/
altium-designer/wirebonding#placing-wirebonds-in-a-pcb
siliconchip.com.au
Two examples of chips bonded
directly to PCB pads. Source:
www.rocket-pcb.com/rocket-pcbwholesale-wire-bonding-technologybulk-fabrication-for-electronics
Australia's electronics magazine
June 2025 45
SSB Shortwave
Receiver
Part 1 by Charles
Kosina, VK3BAR
While there are
plenty of cheap radios these
days, including software-defined types,
I decided to build this analog shortwave radio for the
satisfaction of making it myself. I learned a lot about shortwave, SSB
and how radios work in the process, which you will not get just buying an ‘appliance’!
R
adio receiver architectures
have changed dramatically
in the last few years. Digital
techniques have largely displaced the
analog techniques from the past. Radio
receivers are now available at ridiculously low prices from various internet sources.
The simplest ones are the Software
Defined Radios (SDR) that are a small
module that plugs into a USB port.
The typical coverage is from 100kHz
to 2GHz; they rely on the processing
power of the attached computer to
recover the desired signal.
They are not ‘communications
receivers’, as their noise figure and
immunity from intermodulation are
quite poor. With no input tuneable filter, a strong signal can easily overload
46
Silicon Chip
the front-end circuitry. But for many,
the performance is quite adequate.
The screen “waterfall display” showing signals is very useful.
Still, it isn’t too hard to build
an analog shortwave receiver with
decent performance, as I shall explain
shortly.
Performance
The performance of this unit is
quite reasonable. I set my signal generator to 1µV (-107dBm) output and
the signal-to-noise ratio was about
13dB for most of the range (slightly
less at 30MHz).
Inserting a 20dB attenuator gave
me a signal of about 0.1µV (-127dBm)
and it was still audible! At that level,
communication via Morse Code (CW)
Australia's electronics magazine
would be possible, but it is too weak
for SSB voice reception. Yes, there are
the unavoidable birdies, but they do
not interfere greatly.
What about on-air tests? The only
HF antenna I have at present is an endfed half-wave dipole on the 40m band
(7MHz). This is fed with 50W coaxial
cable and uses a 49:1 ‘unun’ (unbalanced to unbalanced) transformer. The
measured SWR (standing wave ratio)
is between 1.2 and 1.3.
Unfortunately, the ambient noise
here is rather high with all the electrical equipment in the surrounding
houses, producing heaps of RF hash,
so it needs a fairly strong signal to get
through. Comparing this receiver with
my Bando Technic 5D transceiver, the
sensitivity is much the same.
siliconchip.com.au
Fig.1: a TRF receiver comprises several identical RF amplifiers tuned to the same frequency. Most very early radios
used this configuration.
Fig.2: the superhet was an early game changer. By mixing the amplified, tuned incoming signal with an oscillator
frequency that tracks above it, the signal is shifted down to a lower, fixed (intermediate) frequency. Signals at that
frequency are easier to filter out and demodulate.
Fig.3: an SSB receiver is a bit more complex as it needs to operate without the carrier wave or half the signal
spectrum. The modulated signal is recovered by mixing it with the output of the BFO in a second mixer stage.
A list of the features and specifications for this receiver includes:
∎ Covers the shortwave band from
3MHz to 30MHz in two spans
∎ Sensitivity: 1μV (-107dBm) for
a 13dB SNR (reception possible <at>
100nV/-127dBm).
∎ 2.7kHz speech bandwidth
∎ Runs from 12V DC <at> 500mA
∎ Digital tuning with frequency
display
∎ Analog controls for tuning, volume, RF gain and squelch
∎ USB/LSB decoding
∎ Fast or slow AGC
∎ RSSI display
∎ Built-in speaker and headphone
jack
Radio receiver types
I will start with a brief summary
of radio techniques over the last 100
years or so.
Back in the 1920s, a typical radio
was most likely a TRF (tuned radio frequency) set. They consisted of several
cascaded tuned amplifiers, each set to
the same frequency, as shown in Fig.1.
A detector extracted the audio signal
at the end of the chain, which was
siliconchip.com.au
then amplified to drive headphones
or a loudspeaker.
The valves used were initially triodes, and with high feedback capacitances, were subject to instability,
leading to oscillation. A neutralising
system was developed to feed back a
phase-shifted version of the signal,
minimising or preventing this instability. Later, tetrode and pentode valves
were used that had much lower feedback capacitance and obviated the
need for neutralisation.
Not only were these early radios
difficult to set up and use, but
they lacked the selectivity to reject
unwanted strong signals on different
frequencies. However, by using regeneration, where a portion of the amplified signal is fed back to the input
grid of the triode and pentode, much
higher gain and selectivity could be
achieved.
Enter the superhet
The problems of the TRF receiver
were largely overcome by the superheterodyne architecture. Edwin Armstrong is often credited with the invention of this technique, but others filed
Australia's electronics magazine
patents only months apart. Legal battles followed, and French engineer
Lucien Lévy was awarded a patent that
included seven of the nine claims in
Armstrong’s application.
Fig.2 shows the superheterodyne
architecture. The incoming signal
passes through a tuned filter, followed
by an optional RF amplifier. Then follows the mixer, where the incoming
signal is multiplied by another frequency from a local oscillator. The
multiplication results in two extra signals, being the sum and difference of
the frequencies.
For example, if the incoming signal is 1000kHz, and the local oscillator is at 1455kHz, the output from the
mixer will contain signals at 455kHz
(1455kHz – 1000kHz) and 2455kHz
(1455kHz + 1000kHz). It will also
include the original 1000kHz signal.
The following band-pass filter
selects just the 455kHz portion, which
is amplified by the IF (intermediate
frequency) stage(s) and passed to a
detector and audio amplifier as before.
However, this technique is only suitable for receiving AM (amplitude modulated) signals.
June 2025 47
To receive SSB (single sideband)
broadcasts, discussed further below,
an additional mixer stage is necessary
after the IF amplifier(s). This mixes the
IF signal with that from a BFO (beat
frequency oscillator), and its output
goes through a low-pass filter (LPF),
as shown in Fig.3.
This architecture remained the normal way that radios were built for
many decades. Most of the selectivity
(ie, rejecting unwanted station signals)
came from the IF filter.
However, consider a broadcast at
1910kHz with the common 455kHz IF.
With the set tuned to 1000kHz, when
mixed with the LO at 1455kHz, this
signal also will produce a 455kHz output from the mixer. This is termed the
image frequency, and it is why there
is an input band-pass filter, to attenuate this image.
A single tuned circuit was adequate
for the broadcast band frequency range
of 530kHz to 1,600kHz, but once shortwave broadcasting became commonplace, the single tuned circuit was
inadequate at frequencies above 3MHz
and resulted in ‘double spotting’ of the
same input signal.
This was often tolerated, but to
get around it, double- and triple-
conversion superhet sets were used
for better performance. This resulted
in a higher-frequency initial IF signal, which was then mixed again to
obtain a lower-frequency secondary
IF signal.
There are some limitations to the
superheterodyne architecture. Spurious signals are generated as a result of
the mixing process or from non-ideal
components (like harmonic distortion). Spurious signals may be produced by the oscillator, mixer, or other
components in the receiver.
The local oscillator may generate
harmonic signals that mix with the
RF signal, producing unwanted spurious signals. In nonlinear systems,
two or more signals can combine to
produce additional unwanted frequencies, known as intermodulation
distortion.
Fig.4: this Hartley SSB
receiver configuration
is difficult to implement
in hardware as a very
accurate 90° phase shift
is required across a range
of signal frequencies.
Fig.5: this alternative
configuration is similar
to the Hartley type except
the 90° phase shift is split
into two 45° phase shifts.
It’s still difficult to make
it work in the analog
domain, though.
48
Silicon Chip
Australia's electronics magazine
Some of these spurious signals are
characterised by a rapid tuning rate.
The whistle or chirp that is produced
changes in frequency much faster than
the tuning of the receiver. Hence, they
were called “birdies”.
Hartley phasing
There are alternatives to the superheterodyne receiver. A variation is
to use the Hartley phasing method,
as illustrated in Fig.4. The incoming signal (ωs) is fed into two mixers.
The local oscillator is at the same frequency, and an RF phase shift network
of 90° will mix with the incoming signal to produce two signals at baseband,
but at 90° apart.
These signals are called I (in-phase)
and Q (quadrature). The Q signal is
applied to an audio phase shift network, which in mathematical terms
is a Hilbert transform. This shifts the
entire audio spectrum by 90°.
However, this arrangement is
impractical. A better approach is using
two separate phase-shift networks of
+45° for the I signal and -45° for the
Q signal, as shown in Fig.5. These
are then summed and filtered to produce the demodulated signal. This is
a simplified explanation of the phasing system; there are plenty of online
references that give a detailed mathematical analysis.
The phasing method is elegant in
its simplicity, but there are practical
problems in its realisation. It is relatively easy to have an accurate 90°
phase shift, but the audio phase shift
network requires an extremely high
precision in components to maintain
the accurate phase shift over the whole
range of frequencies.
This is why the analog method
has been superseded by digital techniques. In current SDR receivers, the I
and Q signals are sampled by analog-
to-digital converters and the Hilbert
transform is done by software. It does
require a fast processor, as found in
modern computers.
I decided to investigate if a phasing
receiver was practical using an analog
phasing network. There are designs
available to implement the Hilbert
transform in hardware, but it requires
careful matching and selection of components, preferably to within 0.1%.
One such design is shown in Fig.6,
and I built a test module to test its
practicality.
I bought about 50 of the 10nF
siliconchip.com.au
Fig.6: an example of a phase shift network that provides a more-or-less fixed phase shift across a range of frequencies.
capacitors and, by measuring them
to four-figure resolution, I selected a
batch where all were within 0.1% of
each other. The exact value is not quite
as important as the matching.
I originally thought that 8-pin SIL
(single in-line) resistor networks with
four 10kW resistors each would be
closely matched, but found that was
not accurate enough. The alternative
was to select from lots of 10kW SMD
resistors for a matched set. The hardest
part is getting the other six resistors to
an exact value.
For example, a value of a 12,960W is
needed, which is realised by two resistors in parallel, 13kW and 3.3MW. But
this required measuring and selecting
resistors that were close to the nominal
Fig.7: the performance of the phase
shift network shown in Fig.6.
Even with hand-selected matching
components, it doesn’t quite hit 90°,
nor is it perfectly flat with frequency
across the band of interest.
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value. Some values were difficult to
get exactly.
Fig.7 shows the measured phase
shift of my prototype which, while
close to 90°, is not really close enough.
The sideband rejection would be 40dB
at best. Also, this is not the sort of
design that can many readers would
bother to build.
It is possible to eliminate the Hilbert transform; one solution is the
Weaver architecture. Following the
baseband low-pass filters, we have
another pair of mixers, as shown in
Fig.8.
The frequency injected into the second pair of mixers is at about half the
bandwidth. Again, two signals 90°
out of phase are needed, called the
pilot tone. A further LPF extracts the
wanted signal.
There are many articles and papers
describing the Weaver method, many
with quite complicated mathematics.
It is described in detail at siliconchip.
au/link/ac51
I built a receiver with this architecture, copying some of the design ideas
available on the internet. After many
hours of trying to get decent performance, I eventually gave up. Getting
the accuracy and balance between the
I and Q channels just proved too hard.
Overall, the receiver was far too
noisy; I suspect because of the multiple mixers, and I could not get rid of
the pilot tone in the output. I would
be interested to hear from readers who
Fig.8: the Weaver receiver configuration has some advantages over Hartley but
many more mixers are required, so the resulting noise performance is less than
ideal (in the analog domain, anyway).
Australia's electronics magazine
June 2025 49
may have built a Weaver receiver and
find what their results were.
Having tried all the different architectures (apart from TRF) over a period
of about six months, I decided that
the SSB superhet design was the most
practical approach for home construction. But before we get to the circuit,
here is an explanation of two modulation techniques.
Amplitude modulation (AM) is
where a ‘carrier frequency’ signal is
Fig.9: the basic principle of
amplitude modulation (AM). The
high-frequency carrier amplitude
varies with the instantaneous
baseband signal amplitude.
Fig.10: the spectra of AM and SSB
transmissions. The transmission
power of SSB is about ¼ that of AM
without significantly reducing the
received signal strength.
The ultimate design
multiplied by an audio frequency
(AF) signal, as shown in Fig.9. We
get a signal with components in three
frequency ranges: the original carrier,
plus two ‘side-bands’, being the sum
and difference (see Fig.10).
To demodulate the AM signal, all
that is needed is a diode and a lowpass filter to remove the RF component. This filter may be just a single
resistor and capacitor.
While AM is easy to implement, is
really quite wasteful. The carrier frequency carries no information at all,
and the two side-bands at 100% modulation contain half the power of the
carrier, with identical information.
This is where the single side-band
(SSB) method of communication is
far more efficient. We essentially get
rid of the carrier and one of the sidebands. Instead of a bandwidth of twice
the baseband, our filter needs only the
baseband bandwidth. The spectrum
for SSB modulation is shown at the
bottom of Fig.10.
However, with SSB, the simple
envelope detector will no longer
work. To take an example, transmitting an SSB signal modulated at two
frequencies, 1kHz and 2kHz, an envelope detector would give us a tone of
1kHz, being the difference between the
two frequencies. For a more complex
modulated signal, the output of the
detector would be quite unintelligible.
To recover the audio, we have to
multiply the output of the IF amplifier
with the signal from a beat frequency
oscillator (BFO) with a second mixer.
The BFO frequency is set to where the
carrier frequency would otherwise be.
This results in two signals in the output; one is the original baseband signal, plus another at twice the IF, which
is easily removed by a low-pass filter.
The filtered signal can then be
amplified by an audio amplifier to
drive a speaker or headphones.
Receiver design
Fig.11: the measured performance of the pre-built 9MHz crystal filter
module. It combines a flat passband with very steep roll-offs on either side.
The receiver presented here covers
the frequency range of 3MHz to 30MHz,
with an audio bandwidth limited to the
frequencies used by human speech:
300Hz to 3kHz. This means that the IF
filter bandwidth needs to be 2.7kHz
(3kHz – 300Hz). This is best achieved
by a multi-pole crystal filter at 9MHz.
This is quite a critical item in the
design. You can build your own by
buying a batch of 9MHz crystals and
carefully selecting them for series and
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siliconchip.com.au
50
Silicon Chip
The front and rear sides of the control board. The five pots, three switches, rotary encoder, LCD screen and headphone
socket form the user interface. On the rear of the control board are the Arduino Nano and clock generator modules, LCD
adjustment trimpot, two electrolytic capacitors and some connectors. Note that these photos are shown enlarged for clarity.
parallel resonant frequencies. But
unless you have the equipment and
patience to do this accurately, it is not
worthwhile.
I bought 20 9MHz crystals for about
$6, and by selection, managed a reasonable filter after much experimentation. But a complete six-pole filter
module is available from AliExpress
siliconchip.com.au
for about $25, with an excellent bandwidth, as is shown in Fig.11.
Next, let’s look at how we deal with
image frequencies. If the desired signal
fs = 7MHz and the local oscillator fo =
16MHz, producing a 9MHz IF signal,
a signal at 25MHz mixed with 16MHz
will produce the same 9MHz IF. This
is why we have an input tuned circuit.
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How sharp does this filter have
to be? Using a high-quality toroid, a
loaded Q of 100 is typical. There are
calculators on the internet that save
us the trouble of laboriously working
it out; with the above example, the
unwanted 25MHz image signal will
be attenuated by about 50dB.
That is why a relatively high IF is
June 2025 51
What is a noise figure?
Every device generates broadband noise that will reduce the circuit’s signalto-noise ratio (SNR). The NF is the ratio of actual output noise to that which
would remain if the device itself did not introduce noise, which is equivalent
to the ratio of input SNR to output SNR.
There is another way of expressing the noise performance: the noise
temperature, expressed in Kelvins as an equivalent temperature. It is not the
physical temperature of a system, but a theoretical value that defines the
temperature required to produce a specific amount of noise power.
The equivalence between noise temperature and noise figure is shown
below. The reference temperature, Tref, is generally 290K (16.85°C).
The relationship between noise figure (NF) and noise temperature (in Kelvin).
Note that it is not the actual temperature the part is operating at.
desirable for higher-frequency signals, as the image frequency is well
removed. If an IF of 455kHz were
used, the standard for broadcast-band
receivers, the image at 7.91MHz would
only be 28dB down.
Circuit details
Figs.12 & 13 show the full circuit of
the receiver, which is split across two
PCBs, and the circuits correspond to
them. One is the control board, while
the other is the RF board.
At the heart of the control board is
the Arduino Nano module, which has
the ATMega328 microcontroller. The
display is the common 16×2 alphanumeric LCD module; the version with
a blue backlight is the best choice.
Potentiometer VR6 is the contrast
adjustment for the LCD screen.
The variable frequency oscillator
(VFO) and the beat frequency oscillator (BFO) signals are generated by
an Si5351A clock-generator module
(MOD2), controlled over an I2C serial
bus (SDA/SCL). This module can
generate three different frequencies
as square waves with amplitudes of
about 3V peak-to-peak. In this design,
the outputs used are CLK0 and CLK2;
the CLK1 output is not used.
The 8.2kW pull-up resistors for the
SDA & SCL lines are shown greyed out
in Fig.12 because they do not need to
be fitted as the Si5351A module has
onboard pull-up resistors.
A rotary encoder (RE1) is used for
frequency tuning; the step size for
each click can be varied using the integrated pushbutton switch. Pressing the
switch cycles through steps of 10Hz,
100Hz, 1kHz, 10kHz, 100kHz and
1MHz. The two poles of the encoder,
plus its integral switch, have 33kW
pull-up resistors to give defined high/
low levels and 100nF capacitors to
ground for debouncing.
The I2C serial bus is used to control
the input circuit tuning by selecting
six capacitors in various combinations for approximate tracking with
frequency. Fine potentiometer VR1 is
used to change the voltage on a varicap
diode to interpolate the approximate
values and peak the input circuit to
resonance (more on this later).
There is audio circuitry on this
board as well. Op amp IC1b has a gain
of about 5.5, and can drive headphones
directly via a 3.5mm jack provided on
the front panel. It has internal switching that disconnects the power amplifier driving the speaker when headphones are plugged in.
Despite the existence of numerous
more modern power amplifier chips,
I have used the venerable LM386 (in
an SMD package) to drive the speaker.
It requires few external components,
is cheap and with a 12V supply will
deliver over 2W to an 8W speaker
Fig.12: the control board circuit.
Three main modules are used: the
Arduino Nano ‘brain’, an Si5351
digital clock generator that produces
the VFO and BFO oscillator signals
and the 16×2 alphanumeric LCD
module. The dual op amp provides
the squelch function (IC1a) and audio
gain for driving headphones (IC1b),
while IC2 is the power amplifier that
drives the speaker.
52
Silicon Chip
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siliconchip.com.au
The control board and RF board
are joined by a 16-wire flat cable
between headers CON2. This
supplies power to the RF board
and carries signals to it as well,
including the band change signal and the I2C bus (SDA &
SCL).
Signals coming into the control board on CON2 include
the recovered audio and RSSI
(received signal strength indicator) voltage.
Potentiometer VR5 is the volume control, while VR2 is an RF
gain control modifying the AGC
(automatic gain control) voltage.
Switch S3 is the SLOW/FAST
AGC selection, adding a 10µF
capacitor to the RSSI line for the SLOW
AGC mode.
The squelch control is useful in
eliminating background noise from
weak input signals. It works by comparing the RSSI voltage level at the
inverting input of IC1a (which is
used as a voltage comparator) with a
DC voltage derived from potentiometer VR4. When the RSSI level is low,
Mosfet Q1 is switched on, shorting out
the audio. The 1MW feedback resistor
provides hysteresis.
The mute function is provided by a
second transistor, Q2, in parallel with
siliconchip.com.au
The controls
are all labelled on
the front panel PCB. The rear
of the set only has the BNC antenna
terminal, DC power connector and holes so
that sound from the the internal speaker can escape.
Q1. I found that when the frequency
was being changed, there was a loud
annoying click in the audio. So during
tuning, Q2 is switched on, also shorting out the audio.
DC power is via CON1 and diode
D1 protects against the wrong supply
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polarity. The supply voltage can range
from 9-12V DC, with a maximum current drain of about 250mA. An ironcore transformer based plugpack is
preferable as it does not generate RF
noise, but you can try a switching plugpack; some do have low noise.
June 2025 53
Fig.13: this RF board circuit connects to the control board circuit (Fig.12) via CON2. Q1-Q6 and VD1 tune the incoming
signal while T1 (3-10MHz) or T2 (10-30MHz) are selected by RLY1 for band switching. Q8 is the RF gain stage; IC1 is the
superhet mixer; Q9 is the first IF gain stage; Q10 is the second IF gain stage; IC2 is the BFO mixer; and dual op amp IC3 is
the RSSI/AGC signal amplifier.
Because the voltage regulation of
iron-core plugpacks is poor, a 12V one
may put out a voltage that is too high
with a light load, so choose one rated
at 9V DC and 500mA. Depending on
the Arduino Nano, the voltage regulator may not tolerate an input voltage
much greater than 12V, so be careful
with the choice. You can easily blow
up a Nano with excessive input voltage (trust me, I have!).
The filtering on this type of plugpack may leave too much 100Hz ripple, which would be heard as hum
in the output. That’s why there is a
2200µF electrolytic capacitor after
D1. When S1 is switched on, there is a
very high inrush current to charge this
capacitor, hence a fairly high-current
schottky diode is used for D1.
The ideal supply would be a ~12V
battery; three 18650 cells in series
give just over 11V fully charged. The
background noise using a battery is
significantly lower than either type
of mains-powered supply. A suitable
battery holder can be squeezed into
the case, although taking out the cells
to charge them requires removing a
bracket. Still, you could integrate a
charging socket.
54
Silicon Chip
Most constructors will not need the
optional serial debugging interface
provided by Mosfets Q3 & Q4; they
offer a bidirectional RS-232 compatible serial stream at header CON5.
Those components can be left off if
not needed. You can also connect a
TTL USB/serial adaptor directly to the
TXD & RXD pins of MOD1.
RF module circuit
As shown in Fig.13, the signal from
the antenna goes to two tuned toroidal
transformers selected by relay RLY1. A
high Q is desirable in these transformers for maximal rejection of unwanted
frequencies. The toroids are Micrometals T37-17 types with an unloaded Q in
excess of 200 at most frequencies. With
a 50W source on the primary winding,
the loaded Q will be about 100.
Transformer T1 covers the range of
3-10MHz and has a secondary inductance of 7.4µH (42 turns). The antenna
winding is four turns at the ‘cold end’
of the toroid. This needs a capacitance
range from 34pF at 10MHz to 380pF
at 3MHz for tuning.
Back in the days when valves were
used, this capacitance would be
part of a two- or three-gang variable
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capacitor. These days, such capacitors are relatively rare, expensive
and too large. Instead, I used six fixed
capacitors selected by the PCF8574
I2C extender (IC4) driving six NPN
RF transistors.
A BB910 varicap diode (VD1) adds
to the tuning capacitance as a fine
adjustment to interpolate between the
fixed values. The capacitance range of
the varicap is from 40pF at 0.5V down
to 8pF at 9V (a varicap diode is used
in reverse bias, with the voltage across
it affecting its capacitance).
For the range from 10.1MHz to
30MHz, we switch in transformer T2,
with an inductance of 1.1μH (15 turns).
Its antenna winding is two turns.
Q8 is a low-noise amplifier based on
a BF998 dual gate Mosfet. While technically obsolete, this is easily obtainable from many sources. Rather than
another tuned circuit in the drain,
I have just used a 100μH inductor,
which has a reasonably high impedance over the entire 3-30 MHz range.
The gain is about 20dB and, while the
noise figure (NF) is not given below
30MHz, at 800MHz it is 1dB.
The first mixer (IC1) is an NE612 (or
SA612) IC. This has a gain of about
siliconchip.com.au
17dB and a noise figure of 5dB. The
NF of a multi-stage amplifier can be
calculated as:
NF = NF1 + (NF2 – 1) ÷ G1 +
(NF3 – 1) ÷ (G1 × G2) + ...
Here, NF is the total noise figure,
while NF1, NF2... are the noise figures
of subsequent stages, and G1, G2... the
gains of the stages. Thus, with a reasonably high gain in the first stage, the
overall noise figure is degraded only
slightly by the following stages.
The final noise figure of our circuit
is about 1.5dB. That is more than adequate given the amount of ambient
noise in the HF band.
Another BF998 (Q9) follows the first
mixer, providing another 20dB of gain.
The 9MHz crystal filter follows, which
has 50W input and output impedances.
This is matched to the preceding
BF998 amplifier by a pi network with
a 3000:50W ratio. The filter introduces
a loss of about 5dB. Another BF998
(Q10) is the second 9MHz IF amplifier after the crystal filter.
A second NE612 (IC2) is used for
the second mixer, with the ~9MHz
BFO. There are two outputs available
on the chip. One output is connected
to op amp IC1b, which has a voltage
gain of about 46 times. This is the AGC
amplifier. Schottky diodes D2 and D3
rectify this voltage and charge a 1μF
capacitor. This voltage is applied to
the inverting input of IC3a.
With no signal, this voltage is close
to zero. The non-inverting input has a
voltage from the RF gain control potentiometer on the front panel, and with
the resistor values used, the output
of IC3a is a maximum of about 4.5V.
This is applied to the second gate of
the three BF998 transistors for maximum gain.
As the RSSI voltage rises, the AGC
voltage drops, going down to zero for
very strong signals for minimum gain.
The assembled RF board - toroidal transformers T1 & T2 are on the left, while the crystal filter module is at lower right.
Note that this photo is shown enlarged for clarity.
siliconchip.com.au
Australia's electronics magazine
June 2025 55
The maximum supply voltage for
the NE612 mixers is 9V, so 8V is provided by a 7808 regulator. With a 9V
main supply voltage, this will drop to
about 7.5V, which is quite adequate.
The PCF8574 I2C I/O expander driving Q1–Q6 is the only chip that needs
a 5V supply, which is provided by an
SMD 78L05 regulator (REG2).
Parts List – SSB Shortwave Receiver
We’ve covered quite a lot in this article, so the construction details will be
in a follow-up article next month. It will
also cover programming the Arduino
Nano, preparing the case, plus calibrating and aligning the Receiver.
SC
1 180 × 130 × 110mm blue vented steel project box with feet
[AliExpress 1005008418042828]
1 assembled control board (see below)
1 assembled RF board (see below)
1 front-panel PCB coded CSE250204, 165.5 × 97mm, with black solder mask
1 panel-mount DC barrel socket, diameters to match plugpack
1 12V 500mA+ plugpack
1 8W all-purpose loudspeaker (SPK1) [Jaycar AS3025, eBay 7.7cm 5W 226113532195]
5 13mm diameter universal knobs [AliExpress 1005006143033779]
1 25mm diameter universal machined aluminium knob [AliExpress 1005007577048515]
1 10cm male SMA to female BNC panel-mount connector cable
[AliExpress 1005003990025513 select “BNC F WATERPROOF 2”]
2 16-way IDC connectors
2 2-way 2.54mm pitch polarised header plugs with matching pins
1 20cm length of 16-wire ribbon cable
4 M4 × 10mm panhead machine screws, nuts & washers (for mounting SPK1)
4 M3 × 15mm tapped spacers
4 M3 × 10mm tapped spacers
12 M3 × 6mm panhead machine screws
4 M3 × 6mm black panhead machine screws
Control board
1 double-sided PCB coded CSE250202, 150 × 79.5mm
1 Arduino Nano programmed with CSE25020A.HEX (MOD1)
1 Si5351A clock generator module (MOD2) [AliExpress, eBay etc]
1 16×2 alphanumeric blue backlit LCD module (LCD1)
1 pulse-type PCB-mounting rotary encoder with integral switch and 20mm shaft (RE1)
4 10kW 9mm vertical PCB-mounting linear potentiometers with 20mm shafts (VR1-VR4)
1 10kW 9mm vertical PCB-mounting log potentiometer with 20mm shafts (VR5)
1 10kW multi-turn trimpot (VR6)
3 miniature SPDT toggle switches with solder tags (S1-S3)
3 2-pin polarised headers, 2.54mm pitch (CON1, CON3, CON4)
1 8×2-pin header, 2.54mm pitch (CON2)
1 PJ-341 3.5mm vertical PCB-mounting jack socket (CON6) [AliExpress]
2 15-pin female headers, 2.54mm pitch (for MOD1)
1 7-pin header, 2.54mm pitch (for MOD2)
1 16-pin header, 2.54mm pitch (for LCD1)
4 5mm-long untapped spacers, 3mm inner diameter
4 M3 × 12mm panhead machine screws and matching nuts
2 M2 or M2.5 × 11mm tapped spacers
4 M2 or M2.5 × 6mm panhead machine screws
Semiconductors
1 LMC6482IM dual CMOS-input op amp, SOIC-8 (IC1)
1 LM386M audio amplifier, SOIC-8 (IC2)
2 2N7002 N-channel Mosfets, SOT-23 (Q1, Q2)
1 MBR540 40V 5A axial schottky diode (D1)
Capacitors (all SMD M2012/0805 size 50V X7R unless noted)
1 2200μF 16V through-hole electrolytic
1 470μF 16V through-hole electrolytic
1 100μF 6.3V M3216/1206 size
4 10μF 25V X5R/X7R
2 1μF
4 100nF
1 47nF
1 1nF NP0/C0G
1 220pF NP0/C0G
Resistors (all SMD M2012/0805 size 1% unless noted)
1 1MW
1 22kW
1 3.3kW
1 0W M3216/1206 size
3 100kW
1 10kW
1 68W M3216/1206 size
3 33kW
2 8.2kW
1 10W
56
Australia's electronics magazine
Obtaining the components
I have been careful in choosing
components that are readily available
from many suppliers. Virtually all can
be purchased from AliExpress (www.
aliexpress.com) at quite low prices.
For example, the modules on the
control board are an Arduino Nano,
16×2 alphanumeric LCD and Si5351a,
which can be bought for a grand total
of about $10 plus shipping (a few more
dollars).
Although some components are
classed as ‘obsolete’, they are all still
readily available. That includes the
BF998 dual gate Mosfets and NE612
ICs.
The LMC6482 op amp was chosen
as it has a very high input impedance,
an adequate GBW (gain bandwidth) of
1.5MHz but, most importantly, it is a
rail-to-rail input/output type and can
be used with a single supply voltage
of up to 16V.
While the BF998 is easily obtainable, be careful not to use the BF998R,
which has a mirror image pinout
(mounting it upside-down is not
easy!).
The most expensive component is
the 9MHz crystal filter module, costing about $25. As I mentioned earlier,
it’s cheaper to build your own, but it
requires the right equipment and is
quite a bit of effort.
The other expensive item is the case.
The metal case that I have specified is
available for about $37. It comes with
steel front and back panels. The front
panel is replaced by a 1.6mm-thick
black circuit board that has all the necessary holes and cutouts. Thus, you
only need to drill holes in the back
panel for the power, antenna connection, and loudspeaker (if fitted).
Next month
Silicon Chip
siliconchip.com.au
Ideal Bridge Rectifiers
Additional parts for optional debugging interface
1 3-pin polarised header, 2.54mm pitch (CON5)
2 2N7002 N-channel Mosfets, SOT-23 (Q3, Q4)
3 8.2kW SMD M2012/0805 size 1% resistors
1 4.7kW SMD M2012/0805 size 1% resistor
RF board
1 double-sided PCB coded CSE250203, 152 × 50mm
1 9MHz/600Hz crystal filter module (XF1) [AliExpress 1005007201667282]
2 100μH axial moulded inductors (L1, L4)
1 10μH axial moulded inductor (L2)
3 4.7μH axial moulded inductors (L3, L5, L6)
2 Micrometals Amidon T50-6 12.8mm toroidal cores (T1, T2) [Minikits T50-6]
1 80cm length of 0.35mm diameter enamelled copper wire (T1)
1 30cm length of 0.6mm diameter enamelled copper wire (T2)
3 red 5-30pF trimmer capacitors (VC1-VC3)
1 vertical SMA connector, female, standard polarity (CON1)
1 8×2-pin header, 2.54mm pitch (CON2)
1 HFD4/5 or G6K-2F-Y 5V DC coil DIP DPDT signal relay (RLY1)
4 5mm-long untapped spacers, 3mm inner diameter
4 M3 × 10mm tapped spacers
1 M3 × 16mm panhead machine screw and matching nut (for REG1)
8 M3 × 6mm panhead machine screws
4 M2 or M2.5 × 12mm panhead machine screws and hex nuts
Semiconductors
2 NE612 oscillator/mixers, SOIC-8 (IC1, IC2)
1 LMC6482IM dual CMOS-input op amp, SOIC-8 (IC3)
1 PCF8574 I2C I/O expander, wide SOIC-16 (IC4)
1 7808 8V 1A linear regulator, TO-220 (REG1)
1 78L05 5V 100mA regulator, SOT-89 (REG2)
6 BFR92P low-noise RF NPN transistors, SOT-23 (Q1-Q6)
1 2N7002 N-channel Mosfet, SOT-23 (Q7)
3 BF998 dual-gate Mosfets, SOT-143 (Q8-Q10)
1 BB910 VHF varicap diode (VD1)
2 1N5711 axial schottky diodes (D2, D3)
1 LL4148 75V 200mA signal diode, SOD-80 (D4)
Capacitors (all SMD M2012/0805 size 50V C0G/NP0 unless noted)
2 10μF 25V X5R/X7R
1 4.7μF 25V X7R
2 1μF X7R
12 100nF X7R
1 10nF X7R
12 1nF
1 390pF
1 330pF
1 120pF
4 47pF
2 27pF
1 10pF
1 4.7pF
Resistors (all SMD M2012/0805 size 1% unless noted)
4 1MW
1 470kW
1 330kW
3 100kW
1 47kW
8 8.2kW
3 150W
2 100W
1 51W
siliconchip.com.au
Australia's electronics magazine
Choose from six Ideal Diode Bridge
Rectifier kits to build: siliconchip.
com.au/Shop/?article=16043
28mm spade (SC6850, $30)
Compatible with KBPC3504
10A continuous (20A peak),
72V
Connectors: 6.3mm spade
lugs, 18mm tall
IC1 package: MSOP-12
(SMD)
Mosfets: TK6R9P08QM,RQ (DPAK)
21mm square pin (SC6851, $30)
Compatible with PB1004
10A continuous (20A peak),
72V
Connectors: solder pins on
a 14mm grid (can be bent
to a 13mm grid)
IC1 package: MSOP-12
Mosfets: TK6R9P08QM,RQ
5mm pitch SIL (SC6852, $30)
Compatible with KBL604
10A continuous (20A peak), 72V
Connectors: solder pins at
5mm pitch
IC1 package: MSOP-12
Mosfets: TK6R9P08QM,RQ
mini SOT-23 (SC6853, $25)
Width of W02/W04
2A continuous, 40V
Connectors: solder
pins 5mm apart
at either end
IC1 package: MSOP-12
Mosfets: SI2318DS-GE3 (SOT-23)
D2PAK standalone (SC6854, $35)
20A continuous, 72V
Connectors: 5mm screw
terminals at each end
IC1 package:
MSOP-12
Mosfets:
IPB057N06NATMA1
(D2PAK)
TO-220 standalone (SC6855, $45)
40A continuous,
72V
Connectors:
6.3mm spade lugs,
18mm tall
IC1 package: DIP-8
Mosfets:
TK5R3E08QM,S1X
(TO-220)
See our article
in the December
2023 issue for more details:
siliconchip.au/Article/16043
June 2025 57
Douk
ST-01
PRO
Hybrid Valve Amplifier
Big on the cute factor, this
miniature amplifier glows
warmly in the dark from its
valve filaments, but has plenty
of power thanks to a Class-D
output stage. It costs $170,
so how does its performance
stack up?
Review by Allan Linton-Smith
W
e have seen & tested myriad
amplifiers, modules and kits.
Many have totally fake or
exaggerated claims about their performance, but this one is different. It
is a well-engineered & well-presented
package with decent performance.
It combines modern technology like
a Class-D amplifier, digital audio and
Bluetooth with an old-fashioned triode preamplification stage.
It only requires two speakers, cables
and a signal source to be added. You
can select between the RCA, optical
(TOSLINK), coaxial (S/PDIF), USB
and Bluetooth inputs with the press
of a button.
They include a remote control,
instructions, valves, an optical lead
and 24V, 4.5A plugpack power supply.
A quick check on the internet uncovers many other products from them,
which all appear to be well designed
and presented.
Features and design
The heart of the Douk ST-01 amplifier is the Texas Instruments TPA3250
Stereo Class-D Amplifier IC, which is
run in a bridge-tied load (BTL) stereo
configuration.
The small dimensions of this amplifier are a result of the absence of
heavy, expensive power transformers and output transformers, instead
using an external switch-mode power
Fig.1: the signal from the various inputs is fed to the valve preamplifier
via the tone controls. The pentode anode and screen grid are joined
so it effectively becomes a triode, like the circuit shown here, creating
‘acceptable’ even harmonics. Pentodes have more of a tendency to create
less-acceptable odd harmonics.
58
Silicon Chip
Australia's electronics magazine
supply and an efficient Class-D chip
(see Fig.5).
This chip can deliver 70W per channel into 8W loads with a 32V DC power
supply (at TI’s specified 10% THD+N
[total harmonic distortion plus noise]).
However, the ST-01 delivers around
30W into 8W <at> 1% THD+N due to
the limitation of the 24V 4.5A plugpack supplied. They state that you can
upgrade it to 24V 6A if more power
is required.
By itself, the TPA3250 has very low
distortion, quoted at 0.005% THD+N
for 1W into 8W in the data sheet. However, this is a hybrid design with a pentode (wired as a triode) preamplifier to
give a somewhat softer ‘valve sound’
– see Fig.1. This deliberately injects
harmonics (but not much noise) into
the system.
As a result, we measured around
0.02-0.1% THD+N at 1W into 8W (see
Fig.6), which is significantly better
than most valve-only designs.
The warm glow from the valves is
complemented by a retro VU meter,
which is a handy to monitor the signal
levels to avoid objectionable clipping.
Another interesting feature is the
wide variety of valves that can be substituted for the ones supplied by Douk.
There are 15 alternates listed! We tried
a pair of 5654s in place of the 6K4s
supplied and an audible difference
siliconchip.com.au
Manufacturer’s data (Douk Audio ST-01 PRO)
» Audio inputs: Bluetooth, USB, coaxial [digital], optical [TOSLINK], RCA, U-disk
[USB]
» Audio output: Banana jacks / 3.5mm auxiliary socket
» Maximum output power: 100W+100W (4Ω)
[requires upgraded power supply]
» Supported load impedance: 3-8Ω
» Sampling rates supported:
– USB input: 96kHz/24-bit
– Bluetooth input: 48kHz/24-bit
– Coax/optical inputs: 192kHz/24-bit
» Supported USB formats: MP3, WAV, WMA, FLAC, APE
» Maximum capacity of USB disk: 64GB
» Treble/bass adjustment range: ±6dB
» USB systems supported: Windows, macOS, Linux
» Frequency response: 20Hz-20kHz (±1dB)
» Signal-to-noise ratio (SNR): ≥98dB
» Total harmonic distortion (THD): 0.07%
» Working voltage: 18-30V DC
» Dimensions & weight: 115 × 98 × 54mm, 634g
Included in the package: ST-01 PRO Amplifier and user manual; 24V DC 4.5A mains
power supply; remote control (without two AAA cells); USB cable; Bluetooth antenna
was immediately obvious.
Rather than leaving that as a subjective evaluation, we measured the
actual spectra generated and examined
the difference in the resultant harmonics, as shown in Fig.3.
Most valve amplifier owners love
to try different valves and/or different
brands to evaluate the audible results.
This is called “valve rolling”. Sometimes certain brands are considered
superior and have superior prices,
but our substituted 5654s only cost
$7.63 each.
By the way, if you look up the 6K4,
you may find that it is a miniature triode, not a 7-pin pentode. Confusingly,
there are two different “6K4”s! The
Fig.3: this spectrum analysis at 1kHz & 1W shows the
variation between different valves. The 6J1 is represented
by the pink trace, and the 5654 by the blue trace. The total
distortion is the same for both valves, but the harmonic
differences are audible (eg, the blue trace is slightly
cleaner below 5kHz).
siliconchip.com.au
triode is from Russia while the pentode is from China.
The Chinese “6K4” is actually pretty
close in performance to a 6J1 or 6J2
and comes in the same package, so you
could substitute it with a 6J1 or 6J2.
Performance
The frequency response for the
Fig.4: the amplifier’s response for various bass and
treble settings: flat (cyan), maximum treble (green),
minimum treble (blue), maximum bass (red) and
minimum bass (magenta).
Australia's electronics magazine
June 2025 59
Fig.5: the TI TPA3250 IC contains four amplifiers that are bridged into two channels for stereo, similar to this example
circuit from the device’s data sheet. The Class-D RF carrier is filtered out by sets of LC filters before the audio signal goes
to the speakers.
GPS-Synchronised Analog Clock
with long battery life
➡ Convert an ordinary wall clock into a highlyaccurate time keeping device (within
seconds).
➡ Nearly eight years of battery life with a
pair of C cells!
➡ Automatically adjusts for daylight saving
time.
➡ Track time with a VK2828U7G5LF GPS or D1
Mini WiFi module (select one as an option
with the kit; D1 Mini requires programming).
➡ Learn how to build it from the article in the
September 2022 issue of Silicon Chip (siliconchip.
au/Article/15466). Check out the article in the
November 2022 issue for how to use the D1 Mini WiFi
module with the Driver (siliconchip.au/Article/15550).
Complete kit available from $55 + postage (batteries & clock not included)
siliconchip.com.au/Shop/20/6472 – Catalog SC6472
60
Silicon Chip
Australia's electronics magazine
siliconchip.com.au
ST-01 was flat, within ±0.2dB from
20-20kHz when the controls were at
the mid-position.
The bass control added +12.5dB at
20Hz or cut it by -15dB. Bass boost
can help make up for smaller speakers having less bass output. The treble
control gave a boost and cut of +6dB
and -6dB at 20kHz. That can be quite
useful if your speakers have an overly
muted or bright sound.
Full bass or treble boost may not be
effective at high power levels, as you
could run into clipping. The frequency
response plot shown in Fig.4 was made
at 1W into 8W.
The distortion (THD+N) shown in
Fig.6 is 0.03-0.08% at 1kHz & 1W,
which is acceptable for a hybrid amplifier. It is mainly due to the addition of
harmonics (not noise) from the valve
preamplifier, as was visible in the spectrum analysis graph (Fig.3).
For these measurements, we used
an Audio Precision AUX200/AES 17
‘brick wall’ 20kHz low-pass filter system, which prevents the class-D carrier from interfering with the accuracy
of the measurements. However, it also
cuts out the second harmonic above
10kHz, third harmonic above 6.5kHz
etc. Hence the dip above 6kHz in Fig.6.
In this amplifier, we measured the
carrier at 359kHz, and the filters attenuate that by more than 50dB.
Clipping began at 20W with 0.1%
THD+N into 8W, with the THD+N
climbing to 1% at 30W. The clipping was noticeably ‘soft’ (see Fig.7).
Around 33% more power can be delivered using a larger 24V/6A power supply than the one that comes with the
amplifier.
Conclusion
The Douk ST-01 Pro amplifier is a
very compact, lightweight and versatile device with quite decent power
output and acceptable distortion levels. Its cute factor is bound to impress,
especially for its warmth in small
rooms. The ability to accept signals
from various sources is very handy,
and its price is quite reasonable for
what you get.
It is pretty unusual for a hybrid
amplifier to accept 15 valve types.
This is a plus for valve enthusiasts,
and experimenting with it is quite
SC
fun too.
Fig.6: the THD+N is 0.03-0.08% at 1kHz & 1W, which is acceptable for a
hybrid amplifier and is mainly due to the addition of harmonics (not noise)
from the valve pre-amplifier. The variation between the channels is due to
differences in the valves, which are obviously not a matched pair.
Fig.7: the THD+N vs power into 8W shows that soft clipping begins at
around 20-30W, making it very usable in a smaller room, especially with
large speakers, which are usually quite efficient.
siliconchip.com.au
Australia's electronics magazine
The amplifier is tiny despite its
reasonably high power output. The
minuscule class-D IC has had its
heatsink removed in this photo.
June 2025 61
Tim Blythman’s
433MHz
Digital Receiver Module
We recently published our version of the ubiquitous 433MHz (LIPD band) transmitter module, which
performs better than many prebuilt versions. Having found a suitable receiver IC, we then created
our own version of a matching receiver module, and it is better too!
W
e wrote about our 433MHz
Transmitter Module in the April
issue (siliconchip.au/Article/17950).
That article discussed the LIPD (Low
Interference Potential Devices) RF
band, which covers 433.05MHz to
434.79MHz and can be used without
a paid licence.
There are some simple provisions,
including that the EIRP (equivalent
isotropically radiated power) must not
exceed 25mW. This is of concern for
a transmitter, and we explained how
our Transmitter Module was compliant. Of course, this should not be a
problem with a receiver, so we don’t
need to worry about that aspect for
this project.
These sorts of receivers and transmitters are typically used to send digital data at a low bit-rate (up to around
10kbit/s) to provide a wireless link
over distances up to 100m, such as
around a home.
Typical applications include remote
control of devices like garage doors
and gates, or for sending data from
remote sensors back to a base unit, as
might be found in a wireless weather
station.
Fig.1 shows a block diagram of such
a system. As we mentioned in the earlier article, multiple layers of encoding are often used to make the best use
of the medium and to allow systems
to coexist with others nearby by providing identity and data validation
(checksum) features.
We noted how the receivers use AGC
(automatic gain control) to receive data
at differing signal strengths. Simple
OOK (on-off keying) means that it is
quite straightforward to extract a digital signal from the ambient background
RF noise.
62
Silicon Chip
Effectively, the receiver keeps track
of the average RF signal strength (over
millisecond time scales). If the instantaneous RF signal is stronger than
the average, a logical high is sent to
the data output, while a low output
is when the RF signal is weaker than
average. (That explains why you get
noise from the output when there’s no
RF signal; atmospheric noise on that
frequency will constantly vary above
and below its average.)
We’ve used these sorts of transmitters and receivers in numerous projects. The most recent was the Battery
Powered Model Train from January
(siliconchip.au/Article/17607). John
Clarke even designed a 433MHz Wireless Data Range Extender, which was
published in May 2019 (siliconchip.
au/Article/11615).
433MHz receiver
Our earlier 433MHz Transmitter
Module is a drop-in replacement for
the likes of the Jaycar Cat ZW3100
and Altronics Cat Z6900. It has the
same pinout, general size and shape
as those modules. The Transmitter
Module article has comparative performance tests between our unit and
the Jaycar ZW3100.
This Receiver Module is intended
to be a substitute for the corresponding receivers, Jaycar’s Cat ZW3102 and
Altronics’ Cat Z6905A. If you compare
the photos above and below, you can
see that we have aimed for the same
pinout and size, but you’ll note that
our unit has an extra pin (for RSSI, a
useful extra feature).
The Transmitter Module uses a
Microchip MICRF113 IC and the
Receiver Module uses a MICRF220
IC. These are both intended for use
in these sorts of applications on LIPD
bands, which makes our design task
easier.
The MICRF220 IC
One of the quirks of these receiver
modules is that when there is no
nearby transmission, the DATA pin
will produce a stream of random data.
This is analogous to an AM radio (for
those that remember radios before they
became digital!) playing static when
tuned between stations.
This can be a source of frustration
for those using these modules for the
first time, since the decoder (typically the right-hand microcontroller
in Fig.1) must be able to separate this
background noise from valid data.
Fig.1: a matching transmitter and receiver pair form a one-way wireless link
to transmit small quantities of digital data. A previous article covered the
construction of a transmitter module.
Australia's electronics magazine
siliconchip.com.au
Features & Specifications
» Drop-in replacement for Jaycar ZW3102 and
similar 433MHz receiver modules
» Operates from 3.3-5V
» Optional RSSI output (analog voltage, 0.5-2V)
» 6mA nominal operating current
» Optional squelch feature, configurable by
resistors
» Faster rise and fall times, less latency than
some prebuilt receiver modules
» Sensitivity with onboard antenna is superior
to other modules with an external wire
antenna
» Short AGC settling time
Fig.2: our circuit is based on the
MICRF220 RF chip for receiving digital
data on the 433MHz band. It requires a
3.3V supply, provided by REG1. As well as
receiving data, it provides an RSSI signal
so the controller can determine whether
an RF transmission is occurring and how
strong the signal is.
One simple strategy is to look for
signal transitions occurring more
frequently than anticipated for the
expected data stream; the presence of
high frequency components is typical
of the white noise that occurs with no
signal. So, when frequent transitions
are seen, the data can be ignored.
The data sheet for the MICRF220
describes it as a “300MHz to 450MHz
3.3V ASK/OOK Receiver with RSSI
and Squelch”. Squelch is a handy
feature on radio receivers that can
suppress the output unless a strong
enough signal is received.
To maintain compatibility with the
older modules, our Receiver Module can be built with or without the
squelch feature. It is enabled by simply fitting a single resistor. We made
this optional, since some designs may
depend on the noise to detect a valid
signal.
RSSI stands for ‘received signal
strength indicator’, and it is exactly
what it sounds like. There is an RSSI
pin on the MICRF220 that produces an
analog voltage related to the received
signal strength. The data sheet gives
figures of 0.5V for a -110dBm RF input
level and 2.0V for -50dBm. This is the
extra pin on our design.
Note that the theoretical frequency
range of the MICRF220 extends well
beyond the 433/434MHz band. The
components we have selected are
intended to optimise the operation for
this band; different values are needed
for the likes of the 315MHz band,
which sees similar use in the USA.
The MICRF220 data sheet discusses
this in more detail.
Circuit details
Fig.2 shows the circuit diagram of
our Receiver Module. Power comes in
through the various GND and Vcc pins
on CON1 and CON2. These are chosen
to match the pinouts of other receiver
modules, so a few are duplicated.
The MICRF220 is a 3.3V device, so
we have provided a 3.3V regulator
Our Receiver Module (shown in the lead photos) is the same size as boards like
the Jaycar ZW3102 shown here, but has a couple of extra features. The extra
RSSI pin produces a voltage related to the received signal strength. It also has
an optional onboard PCB trace antenna. These photographs are shown at 125%
scale for clarity.
siliconchip.com.au
Australia's electronics magazine
to allow operation with a 5V supply.
REG1, an MCP1700, can tolerate up to
6V on its input. The two 1μF capacitors are recommended input and output bypassing capacitors.
The remainder of the circuit is centred on IC1, the MICRF220 receiver IC.
Pin 8 (SHDN) is tied low with a 100kW
resistor to enable the chip whenever
it is powered. Capacitor C10 is an
optional part noted in the data sheet.
When fitted, it will assert the shutdown state momentarily while the
chip is powered on. We didn’t find it
was necessary to fit it.
Power from the regulator comes
into pins 5 (power) and 9 (ground) of
IC1, with a 100nF capacitor providing
further bypassing. The circuit around
the two inductors at lower left is the
recommended matching network for
the RF signal going into pin 3 of IC1
from the external antenna (‘ANT’)
connection. Adjacent pins 2 and 4 are
RF ground.
We were able to comfortably fit all
the required parts in the necessary
PCB area, with room to spare, so we
added a PCB trace antenna. It can be
connected by closing jumper JP1 with
a solder blob or 0W resistor.
The antenna is about 16cm long,
suitable for use at 433/434MHz. Adding the length of the other connected
traces, it is very close to the nominal
173mm needed for a quarter-wave
antenna at 433MHz. Otherwise, an
external antenna can be connected via
the module’s ANT pin.
June 2025 63
Scope 1: the current consumption of our module, measured with a low-side
100W shunt resistor, is very close to the 6mA noted on the data sheet. It rises
slightly when the data output is high.
Scope 2: the ZW3102 that we tested only drew 3mA during operation, although
its data sheet indicates a maximum of 10mA.
Scope 3: the blue trace is a signal applied to a transmitter module, while the
green trace is the DATA output from our Receiver Module. The red trace is
the output from a prebuilt ZW3102 module. Our module is clearly quicker to
respond, with sharper edges.
64
Silicon Chip
Australia's electronics magazine
Pins 1 and 16 of IC1 connect to a
13.52313MHz crystal and its loading
capacitors. Like the Transmitter Module, this circuit uses a ×32 PLL (phaselocked loop) to generate a reference
frequency.
You might notice that the crystal
for the Receiver Module is a different
frequency to that on the Transmitter
Module (13.56MHz).
That is because the MICRF220 uses
an IF (intermediate frequency) demodulator. The PLL frequency is mixed
with the incoming RF signal to produce a signal with a frequency about
1MHz lower. This lower-frequency
signal is easier for the IC to extract
the data from.
Pins 7 and 11 (SEL0 and SEL1) select
the demodulator bandwidth. We have
chosen the 13kHz low-pass filter setting by leaving both of these pins to
be pulled high by their internal current sources. Fitting a 10kW resistor
for either or both of R1 and R2 will
change this setting.
Pin 13 of IC1 (CAGC) is connected
to a 470nF capacitor; this value is
also dictated by the data sheet and the
bandwidth setting described above.
The level on this pin sets the gain of
the internal amplifier; it is part of the
AGC control loop. This capacitor value
ensures that the AGC responds at the
correct rate to allow the data of interest to be received.
The RSSI signal from pin 14 is internally derived from the CAGC signal by
being inverted and buffered. It is fed
to the extra pin on CON1 via a 1kW
resistor. This protects the chip from
potential short circuits.
The capacitor on the pin 12 (CTH)
provides bypassing of an internal
reference voltage that is used by a
comparator to generate the output
on pin 10 (DO). Like RSSI, the DO
output is protected by a 1kW series
resistor between it and the external
DATA pin.
Pin 6 (SQ) enables the squelch feature. When left open, an internal pullup current disables squelch. Fitting
R5 will pull the pin low and enable
squelch. For any of pins 6, 7 or 11, the
pullup is around 5μA, so a resistor of
10kW or lower will be more than sufficient to overcome the pullup.
Operation
The MICRF220 uses around 6mA
when configured for 433MHz operation. At this level, the dropout voltage
siliconchip.com.au
of the regulator is less than 100mV,
so it will not have much effect on the
output voltage, even if a 3.3V supply
is used.
Most 5V microcontrollers we have
seen will happily accept 3.3V logic levels, and the MICRF220 works down to
a 3.0V supply voltage, so this Receiver
Module will be suitable for 5V and
3.3V systems.
If you are considering changing the
SEL0 and SEL1 settings by adding
resistors R1 and/or R2, you should
check the MICRF220 data sheet
closely as some other parts may need
to change values. You shouldn’t need
to do this, as the default bandwidth
settings should work fine with lower
data rates.
Comparisons
We thought it was important to
describe the operation of our Receiver
Module and the MICRF220 because
it has quite an impact on the performance of the Module compared with
other receiver modules. We compared our Receiver Module (using
its onboard antenna) to the Jaycar
ZW3102 fitted with a simple wire
antenna.
We used our previously described
433MHz Transmitter Module as the
RF source for the tests. Our first test
was to confirm the operating current
of the modules. The MICRF220 data
sheet notes a typical current of 6mA;
the MCP1700 has a quiescent current
of 1.6μA, so it does not contribute significantly to the Receiver Module’s
consumption.
We rigged up a 5V supply and a
100W resistor as a low-side current
measuring shunt on a breadboard.
The breadboard allowed us to change
between the two modules without otherwise altering the circuit.
Our Receiver came in right on 6mA,
as seen in Scope 1. You can see that
the current does come up slightly
when the output pin is high; it reaches
6.1mA. The ZW3102 measured just
under 3mA, whether its output was
high or not (Scope 2). Interestingly, its
data sheet notes a 10mA maximum, so
there may be more variability amongst
these modules.
This shows us the latency, or delay,
between the input and output. The output of our Receiver Module is not only
faster (24μs vs 28μs on rising edges
and 24μs vs 34μs on falling edges),
but more symmetrical and it also has
sharper edges.
We monitored the output of both
receivers when a 1kHz square wave
was applied to the transmitter’s DATA
input.
Scope 3 shows the falling edge of a
pulse on the DATA input, with the two
receivers responses following.
We also performed some tests to see
how the receivers would respond to
different OOK modulation frequencies. As we changed the frequency
at the DATA input of the transmitter,
we watched the receiver outputs to
see how well they followed the input.
Above 10kHz, the output is 90° or
more behind the input for both receivers, as seen in Scope 4. You’ll see that
our Receiver is still delivering a signal
that is closer in time to the original
signal than the ZW3102. Both receivers are receiving a solid signal at this
frequency.
Sensitivity
You might recall from our article on
the Transmitter Module that its output
power can be set by altering a single
resistor value. This allows us to easily
produce weak signals to compare the
sensitivity of the two receivers.
We performed some tests to compare
the relative sensitivity of the receivers.
With the two receivers side-by-side on
the same breadboard, we monitored
how they responded to a transmitter
on the other side of our laboratory; this
was an Arduino connected to one of
our Transmitters to output a typical
encoded waveform.
The first test was with the Transmitter at full power, and Scope 5 shows
an interesting result. Here, we see
how quickly the receivers ‘lock on’ to
the signal. Our Receiver Module settles its AGC at the correct level a full
Scope 4: at 10kHz, a higher frequency than used for Scope 3, you can see the
difference in latency between the two modules. This is quite a bit higher in
frequency than most 433MHz transmissions we have seen, with 1kHz being
more typical.
Latency and bandwidth
For the next few tests, we rigged up
the two receivers side-by-side on a
breadboard, allowing them to be seen
responding to the same transmissions.
siliconchip.com.au
Scope 5: the blue trace here is our Receiver’s RSSI pin, while the green trace is
its DATA output; the red trace is from a ZW3102. You can see how much more
quickly our Receiver locks on to the incoming signal and starts producing valid
data.
Australia's electronics magazine
June 2025 65
Parts List – 433MHz Reciever Module
1 double-sided PCB coded 15103252, 11.5 × 43mm
1 5-way right-angle pin header (CON1)
1 4-way right-angle pin header (CON2)
1 13.52313MHz two-pin SMD crystal, 5.0 × 3.2mm (X1)
[Abracon ABM3-13.52313MHZ-10-B4Y-T]
1 39nH inductor, M1608/0603 size (L1) [Murata LQG18HN39NJ00]
1 33nH inductor M1608/0603 size (L2) [Murata LQG18HN33NJ00]
Semiconductors
1 MICRF220AY 300-450MHz ASK receiver IC, QSOP-16 (IC1)
1 MCP1700-3302 3.3V LDO linear voltage regulator, SOT-23 (REG1)
Capacitors (all M2012/0805 size, X7R 50V ceramic unless noted)
2 1μF
1 470nF
SC7447 Kit ($20 + postage):
2 100nF
includes all the parts listed here
2 10pF NP0/C0G
2 1.5pF NP0/C0G
Resistors
(all M2012/0805 size, ⅛W 1%)
1 100kW
2 1kW
Extra resistors for option
selections
3 10kW M2012/0805 ⅛W
1 0W M1608/0603
OR bridge JP1 with solder
Scope 6: using the same trace colours as Scope 5, we see the two modules
responding to a weaker signal. The RSSI is lower, and the ZW3102 is producing
glitches that are not seen in our Receiver’s output.
15ms before the ZW3102; you can still
see glitches in the latter’s output for
this time. The blue trace that we have
used as a trigger is the RSSI output of
our Receiver.
Then we used a 1kW resistor to
set the output power to 12dB below
nominal. Scope 6 is the result of this.
The RSSI trace sits at around 1.4V or
-74dBm, and our Receiver has picked
out clean data, while the ZW3102 is
seeing some data but is delivering
glitches too. At lower levels than this,
we could not see any data on either
receiver.
This is useful information in that we
now know that a level of around 1.4V
indicates sufficient RSSI to receive a
valid signal. Remember that these tests
were done with the Receiver’s onboard
antenna; an external antenna should
give even better results.
While running these tests, we also
used a software-defined radio receiver
to monitor the relative RSSI. It indicated that these active transmissions
were only about 10dB above the background RF level.
Squelch
We also ran some tests to try out the
squelch feature. For these, we simply
shorted out the R5 pads on the PCB
to pull IC1’s pin 6 low. The data sheet
notes the chip will “monitor incoming
pulse width before allowing activity
on DO pin.”
So it doesn’t appear that RSSI is
used to control the squelch. Scope
7 shows a typical waveform with
squelch active. You can see that there
is still activity on the DATA line even
when the RSSI is low.
It appears that this is where the
13kHz filter is used, as signals at a
higher frequency are cut off and do not
appear on the output. So the squelch
is helpful, but does not completely
remove the need to filter out unwanted
activity on the DATA pin.
Construction
Scope 7: even with Squelch enabled, our Receiver still produces the occasional
spurious pulse on the DATA line when the RSSI is low. So you shouldn’t expect
the Squelch to completely eliminate the need to reject noise on the DATA line,
but it helps to reduce it quite a bit.
66
Silicon Chip
Australia's electronics magazine
The 433MHz Receiver Module
uses some small SMD parts, although
nothing that can’t be hand-soldered
with a little patience. IC1 comes in
a 16-pin QSOP (quarter-size small-
outline package) with a 0.635mm pin
pitch, and the regulator is a SOT-23
part. Most of the passives are M2012
(0805) size at 2.0 × 1.0mm, although
the two inductors are M1608 (0603)
size or 1.6 × 0.8mm.
siliconchip.com.au
We’ve used M2012-sized pads for
the passives throughout to ease construction. Where possible, we have
lengthened the pads on the PCB to
make it easier to apply solder. This
also gives a bit more room between
the components.
So you’ll need the standard surface-
mounting gear; a fine-tipped soldering iron and some flux paste are the
bare minimum. You should also have
tweezers, a magnifier, solder-wicking
braid and some good illumination.
Your flux will probably also require
a solvent for cleanup, although we
find that isopropyl alcohol is a good
generic option.
The Receiver Module is built on
a double-sided PCB that’s coded
15103252 and measures 11.5 × 43mm.
Figs.3 & 4 are the overlay diagrams that
show where the parts are placed. You
can also refer to the adjacent photos
during construction.
All the mandatory components are
on one side of the PCB, as shown in
Fig.3. Apply flux paste to the pads for
all the components on that side. Start
by placing the IC over its pads on the
PCB, noting the orientation of the pin 1
marker; our chip had a moulded divot,
which was easy to find.
Clean the iron’s tip and apply a little
fresh solder. Tack one lead and check
that the other pins are lined up on
both sides. If so, carefully solder the
remaining pins, cleaning the tip and
adding extra solder as needed. Otherwise, use the iron to melt the solder
and tweak the chip with tweezers until
it is located correctly.
If you end up with a solder bridge
joining two or more pins, add extra
flux paste and press the braid against
the bridge with the iron, then gently
draw both away once the excess solder
is drawn up into the braid.
Next, fit REG1, the SOT-23 regulator. It should only fit one way,
with its leads down flat on the PCB,
so place it, tack one lead and check
the position. If all is well, solder the
other two pins. If any joins don’t look
great, add some extra flux and touch
the iron to the pad and pin to refresh
the solder.
The two inductors at bottom left
should be fitted next as they are the
smallest remaining parts. We’ve seen
some SMD inductors that only have
pads on the underside, which makes
them a little more tricky to solder.
Don’t forget that most SMD parts are
siliconchip.com.au
Figs.3 & 4: to use
the onboard PCB
trace antenna,
close JP1 with
a blob of solder
or 0W resistor.
The rear of the
PCB shows the
functions of the
external pins.
If you wish
to enable the
squelch function,
you can fit a
10kW resistor
for R5. These
diagrams are at
200% scale.
usually designed to be soldered by
a machine!
You might be able to make out a
black mark on one end of the inductors. We’ve fitted our prototypes with
the band to the left and on the top,
which you can see in the photos. We
don’t think it will make any difference,
but we recommend you do the same.
RF can be strange and we don’t want
to tempt the fates!
Use the same technique of soldering one lead then the other once the
location has been correctly fixed. You
can check that the inductors are connected to their pads by doing a continuity test; they should read well
under 10W.
For the 33nH part, you can probe
between the ANT and GND pads of
CON2. For the 39nH inductor, probe
between ground and the right-hand
pad of the 1.5pF capacitor directly
above the inductor. If either inductor
reads high resistance, add more flux
and try soldering each lead again.
Solder the crystal (X1) next. It probably will have leads only on its underside, but the PCB pads are generously
sized, so they will be easy to press
the soldering iron against. As long as
there’s flux paste on the pads when
you place the crystal, solder should
flow between the pads and crystal.
Unfortunately, you can’t check a crystal for continuity as you can with an
inductor.
The remaining mandatory small
parts are all M2012 (0805) passives,
and they are marked on the PCB silkscreen. Check their values closely
against the overlay diagram, since the
markings are quite small. There are
nine capacitors and three resistors that
must be fitted. Be careful not to get the
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capacitors mixed up once you remove
them from their packages; they will not
be marked with values.
If you wish to enable the onboard
trace antenna, you need to close JP1.
An M1608/0603 0W resistor will work,
but the easiest way to do this is to generously apply solder with an iron to
both of JP1’s pads. The solder mask
will cause the solder to bead, but if
you add enough solder, you should be
able to bridge the pads (you can see we
did it in our photos).
You can now enable the squelch feature by adding a resistor (we suggest
10kW) to the R5 pads if you want. We
have also labelled this with Squelch
text.
At this stage, we recommend cleaning the board thoroughly with your
recommended flux cleaner or another
solvent.
Allow the board to dry and scrutinise it for bridges and pins not soldered to the pads below. If you see
any problems, touch up the board,
then clean it and allow it to dry again.
Fitting the headers
We recommended using right-
angle headers since they will match
the headers found on other common modules. However, you could
choose straight headers if you need
to mount the Receiver Module parallel to another PCB. It will depend on
your planned application.
If you are connecting the Receiver
Module to an existing design, use two
four-way headers. Older designs will
not expect a connection for the RSSI
pin, so you should leave that pad
unconnected (you could run a flying
lead from that pad if you want to monitor the RSSI output).
June 2025 67
We recommend slotting the two
groups of headers into a longer header
socket to keep them aligned to the
correct 0.1in pitch before soldering
(see the photo below). Solder the pins
in your preferred orientation, then
remove them from the header socket.
If you have jumpered the onboard
antenna, the external ANT pin does
not need to be connected. In this case,
all the connections that are usually
needed (GND, DATA and Vcc) are at
one end of the board, and can be made
using a single four-way header.
An NPN transistor with a 1kW resistor between its base & emitter could
also be used as a threshold detector, as
shown in Fig.5. The RSSI signal is fed
into the base and the 1kW resistor on
the Receiver PCB forms a divider with
the external resistor to set the threshold.
We tried this out on a breadboard
and it worked quite well. You could
also bypass the LED and use the voltage at the collector as an active-low
digital RSSI threshold signal to a
microcontroller or other circuitry.
Using it
Our 433MHz Receiver Module has
some handy features that make it a better choice for new designs. It generally
responds more quickly to an incoming RF signal.
At the same time, it is backward-
compatible with older modules for
use in legacy circuits that require a
433MHz receiver. The Receiver Module works with 5V and 3.3V systems,
which we think will cover most cases.
The squelch feature does not appear
to eliminate noisy data output during
the gaps between RF transmissions,
but it does reduce it. We think that
the RSSI output will be more useful
in testing the validity of a signal on
the DATA pin.
Our Receiver consumes a bit more
current than the ZW3102, but it is still
low enough that it could, for example,
be powered from a microcontroller
GPIO pin, allowing it to be completely
powered off if necessary.
The Receiver Module is quite sensitive, even when just using the onboard
PCB trace antenna, picking up all
transmissions that the ZW3102 could
with an external antenna. Our design
still allows for an external antenna if
SC
that is preferred.
Since it is a module, the usage will
depend a lot on your intended project.
In general, you should connect a supply of 3.3-5V to one or more of the Vcc
pins and one or more of the GND pins.
If you have not enabled the onboard
antenna, an external antenna should
be connected to the ANT pin.
As we noted earlier, a 173mm-long
wire (including the length of the headers and traces back to the matching
network) works well as a quarter-wave
antenna for 433MHz. It can be curled
or corkscrewed to save space if necessary.
We have found that the Receiver
Module is capable of receiving nearby
signals without an external antenna;
you might try this for testing purposes. In general, you should have no
trouble using it to replace a receiver
anywhere we have specified the Jaycar ZW3102.
Conclusion
Fig.5: this simple circuit can be used
to generate an indication that an
RF transmission is being received
based on the RSSI. The resistors set
the threshold to about 1.2V, which
we found to be a suitable level for
distinguishing a valid signal from
none.
Our unit varied around 0.9V to 1.1V
when no intended transmission was
occurring. This level might be lower
in a less urban area than the location
of our lab.
With an active transmitter, we saw
values between 1.3V and 2.0V. This
could be measured by a microcontroller’s ADC (analog-to-digital converter)
peripheral to detect the presence of a
signal. Another option is a comparator
set to an appropriate threshold.
Some micros (including the 8-bit
PIC16F18146) include a comparator
The RSSI voltage
peripheral that could be used for this
The RSSI pin delivers an analog purpose. The micro could then be provoltage between 0.5V and 2.0V, so a grammed to ignore any transitions on
microcontroller with an analog-to- the DATA pin unless the RSSI indidigital converter will be well-suited cates that a strong enough signal is
to monitoring the RSSI.
present.
We closed JP1 by bridging it with
solder (you can also use a small
0W SMD resistor). You will need a
generous amount to bridge the gap
between the pads.
68
Silicon Chip
Using a socket strip as a guide
will ensure that the pins are soldered with the
correct separation even though they are in two groups.
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Australia's electronics magazine
June 2025 69
By Andrew Levido
Precision
Electronics
Part 8: Voltage References
Last month, we looked at sampling and aliasing in DACs (digital-to-analog converters)
and ADCs (analog-to-digital converters). Now we will describe how voltage references
work, as they are critical to the precision of both ADCs and DACs.
W
e have covered a fair bit of ground
so far in this Precision Electronics
series, but we have not looked
at the important topic of voltage references in detail. We mentioned them in
our discussion of analog-to-digital and
digital-to-analog conversion, but now
is the time for a deeper dive.
In the very first article in this series,
we discussed the difference between
precision and accuracy. We learned
that precision describes the repeatability or reliability of a measured
quantity and is all about understanding and quantifying sources of error.
On the other hand, accuracy is how
closely a measured value matches the
‘true’ value (or an accepted proxy) of
the quantity.
Most of what we have covered so
far has been concerned with precision rather than accuracy. Voltage references are one of the places where
these two come together. Put simply,
voltage references provide a fixed
voltage source at some defined value.
This sounds simple, but there is a lot
to unpack in that statement.
Initial accuracy – or not
The “defined value” part is where
accuracy comes into play. A voltage
reference is expected to provide a
known output with some specific level
of accuracy; that is, some measure of
how close its output voltage is to the
‘true’ value.
This requirement implies the source
has been calibrated somehow against
a known standard. In many cases, this
calibration is done for you at the factory, but sometimes you are expected
to do it yourself.
An example of the former is the
MAX6225ACSA reference we used in
the DAC circuit in a previous instalment of this series. This is a 2.5V reference with an initial accuracy of
±200ppm (±0.02%). This means the
voltage will be between 2.4995V and
70
Silicon Chip
2.5005V at 25°C – a figure achieved by
calibration at manufacture.
Calibration would have been performed by trimming the chip’s output voltage against a voltage standard
with even higher accuracy. This standard will have been itself calibrated
against an even better standard, and
so on, in a chain ultimately traceable
to the international standard definition of the volt.
Not all voltage references are
trimmed to a standard voltage at
manufacture. Some very expensive
ultra-precision voltage references have
woeful initial accuracy. The legendary
LTZ1000, which will cost you the best
part of $150, has an initial output voltage anywhere between 6.9V and 7.5V,
but has extraordinary precision.
The intention is that you will calibrate the device in which you use this
reference against some external standard, then take advantage of its incredible stability to ensure it stays that way.
Voltage reference errors
Whether you use a pre-calibrated
or post-calibrated voltage reference,
knowing its stability is critical. As you
would expect, changes in temperature
influence voltage references; achieving
a stable voltage over temperature has
been one of the driving forces behind
the development of voltage reference
technologies.
You will therefore see a figure for
temperature drift in the voltage reference data sheet in the familiar absolute (V/°C) or relative (ppm/°C) units.
In many cases, you will also see a
‘thermal hysteresis’ figure. This is the
maximum voltage change seen after
cycling the device over some fixed
temperature range – typically (but not
always) from 25°C to 50°C and back.
This is important because of the focus
on accuracy; if the voltage changes
slightly with temperature, we at least
want it to return to a consistent value
Australia's electronics magazine
each time it reaches a given temperature.
To add to the growing list of errors,
voltage references also drift with time,
even if the temperature is held constant. Most precision voltage reference
data sheets therefore include a figure
for ‘long-term stability’ or similar. This
can be expressed as an absolute or relative change in voltage per root thousand hours (ppm/√kh) or per thousand
hours (ppm/kh).
The odd unit of root-kilohours is
used because long-term stability typically has a logarithmic decay characteristic, with more drift in the first 1000
hours than in the second and so on.
Because of this early drift, some
manufacturers of precision equipment
using will ‘burn in’ the voltage references for a period before using them.
This improves the long-term accuracy
of the references (since the higher initial drift is done with), and allows the
manufacturer to weed out any that
show too much variation.
To put some context around these
errors, consider the MAX6225ACSA.
The initial accuracy was ±200ppm
with a tempco (temperature coefficient) of ±2ppm/°C and a thermal hysteresis of 20ppm. The worst-case longterm drift is ±20ppm/kh. These are all
pretty good figures, but the LTZ1000
is in a different class.
This latter chip includes an on-chip
heater to keep the reference at a stable temperature, resulting in temperature drift in the ±0.05ppm/°C range.
No thermal hysteresis figure is given,
since the reference is always held at a
constant temperature. Long-term stability is quoted as 0.28ppm/√kh.
I should note that building a device
using the LTZ1000 or similar ultra-
precision references is no trivial
task. To get the most out of the chip,
you must employ some ridiculously
expensive high-precision, low-tempco
resistor dividers and worry about all
siliconchip.com.au
sorts of crazy details. Take this quote
from the data sheet as an example:
The Kovar input leads of the TO-5
package form thermocouples when
connected to copper PC boards. These
thermocouples generate outputs of
35µV/°C. It is mandatory to keep the
... leads at the same temperature, otherwise 1ppm to 5ppm shifts in the
output voltage can easily be expected
from these thermocouples. Air currents blowing across the leads can also
cause small temperature variations...
There is a whole online community
dedicated to getting the best possible
performance out of these and similar
devices. Just search for “voltnuts”.
Series and shunt references
Voltage references fall into two major
categories: three-terminal (series) or
two-terminal (shunt) devices, both of
which are shown in Fig.1. Series references ‘regulate’ an input voltage to
produce the reference output.
As you might imagine, the output
is influenced by changes in the input
voltage and by the load current, so for
series regulators you will see figures
in the data sheet for line and load regulation (ie, how stable the output is
despite variations in input voltage and
output current, respectively).
In the case of the MAX6225ACSA,
the line regulation is ±7ppm/V for a
Vin above 10V and the load regulation
is ±6ppm/mA. You should therefore
ensure the input to a series voltage reference is well-regulated and keep the
load current low and stable.
Achieving the latter can be a bit of
a juggling act: you can add an op amp
buffer to minimise the load current,
but this will itself introduce errors
that might outweigh those produced
by the reference’s load regulation. You
have to crunch the numbers to work
out what is optimal.
On the other hand, shunt references
maintain a constant voltage drop while
current is flowing through them. The
voltage drop is influenced by the
device current, and you can see from
Fig.1 that this current is determined by
both the source and the load currents.
Shunt references therefore usually
include a single figure for output voltage change with current that encompasses both line and load regulation.
You should therefore aim to keep
the device current constant if you
want to achieve the best results with
shunt-type references, most likely by
siliconchip.com.au
employing an active current source
and by keeping the load current fixed.
Changes in shunt current with temperature will add to the shunt element’s inherent temperature drift, so
your current source needs to be relatively stable with temperature.
Zener references
The zener diode, with its well-
defined reverse breakdown voltage, is
the simplest form of shunt reference.
This breakdown characteristic occurs
because of two different mechanisms:
the zener effect at low voltages, and
the avalanche effect at higher voltages.
The zener effect has a negative tempco,
while the avalanche effect has a positive tempco.
As both these effects are present in
zener diodes with breakdown voltages around 5-7V, it is possible to have
these temperature effects more-or-less
cancel each other out by careful selection of the diode and its operating
conditions.
For example, a BZX55C5V1 5.1V,
400mW zener diode has a tempco
of between +0.02% and -0.02%
(±1mV/°C). By contrast, a BZX55C12
(12V) zener has a tempco of +0.11%
(+13mV/°C). The initial accuracy of
the 5.1V zener won’t be great, but fed
with a constant current, its voltage stability will be surprisingly good.
In fact, the LTZ1000 and MAX6225ACSA both use internal zener
diodes as the basis of their reference.
You can temperature-compensate
a zener diode by putting it in series
with a forward-biased standard diode,
as long as you choose a zener with
a tempco of about +2mV/°C. That’s
because the tempco of a regular diode’s
forward drop is about -2.1mV/°C.
Otherwise, you can buy temperature-
compensated zener references like the
LM329, or even the LM399, which
includes an on-chip heater.
We mentioned above that you need
to maintain a constant current through
a zener reference. For example, the
BZX55C5V1 has a dynamic resistance
of up to 35W, so a change in bias current of just 1mA will shift the output
voltage by 35mV – as much as a temperature rise of 35°C.
Fig.2 shows a clever circuit that uses
the zener itself to provide a stable bias
current and allows the output voltage
to be adjusted to boot. The zener voltage is amplified by the non-inverting
amplifier to produce an output voltage,
Australia's electronics magazine
Fig.1: voltage references are
available as either three-terminal
series pass devices or twoterminal shunt devices. In either
case, keeping the input voltage or
current (and the output current)
constant is critical to getting the
best accuracy.
Fig.2: in this circuit, the zener
bias current is derived from its
own stable output. R1 and R2
allow the output voltage to be
amplified if necessary.
Vout = Vz (1 + R1 ÷ R2). The output
voltage is then used to establish the
zener bias current via R3, Iz = (Vout
– Vz) ÷ R3.
You must use a single supply with
this circuit – with a split supply, it
could settle into a second stable state
with the zener forward-biased. If you
are worried about start-up, you can
add a 1MW or greater resistor from the
zener’s cathode to the positive supply.
You will often see the term ‘buried zener’ to describe precision zener
references. This just means that the
diode junction (where the reverse
breakdown occurs) is formed below
the surface of the semiconductor and
covered with a layer of diffusion material, resulting in a more stable device
with lower noise.
Band-gap references
Band-gap voltage references are
June 2025 71
much more common than zener references these days, especially inside
integrated circuits. Pretty much every
voltage regulator, linear or switching,
uses one.
Developing a semiconductor voltage
reference with a low tempco was no
trivial task, but it came down to adding a voltage with a positive tempco to
another voltage with a negative tempco
just like the compensated zener.
The idea was first used commercially by Bob Widlar in 1971. Bob
Widlar was an erratic genius who pioneered the first commercially successful op amps, comparators and three
terminal-voltage regulators, among
many others.
Part of his success was to recognise
and work with the strengths of the IC
production process. He understood
that it was very hard to manufacture
components of precise absolute value
in silicon, but was relatively easy
to make components with precisely
matched values.
The Ebers-Moll large-signal BJT
model (a really useful model I strongly
recommend you study) tells us that the
base-emitter voltage (Vbe) of a transistor is related to its collector current (Ic)
by the relationship Vbe = Vt loge(Ic ÷
Is). Vt is the thermal voltage (proportional to absolute temperature) and Is
is the reverse saturation current (also
highly temperature-dependant).
With a fixed collector current,
the base-emitter voltage has a negative tempco of -2.01mV/°C, since
the tempco of the Is term dominates.
However, the difference between the
base-emitter voltages of two transistors
Fig.3: the simplest band gap
reference consists of just three
transistors. The voltage across R3
(Vbe1 – Vbe2), and therefore that
across R2, has a positive tempco,
offsetting the negative tempco of
Q3’s base-emitter voltage.
72
Silicon Chip
with different collector current densities has a positive tempco.
This can be achieved by using two
identical transistors with different
collector currents. If you are mathematically inclined, it is pretty easy
to see why by simplifying the expression Vbe1 – Vbe2 = Vt(loge[Ic1 ÷ Is] –
loge[Ic2 ÷ Is]). This becomes Vbe1 – Vbe2
= Vt × loge(Ic1 ÷ Ic2). Note that Is has
disappeared, leaving Vt with its positive tempco the only temperature-
dependent term.
Fig.3 shows how this phenomenon can be used in practice. Identical
transistors Q1 and Q2 have collector
currents in a 10:1 ratio because of the
values of R1 and R2. Both transistors
have the same base voltage, so the voltage at the emitter of Q2 must be Vbe1
– Vbe2. The 10:1 Ic ratio means this
voltage will be 2.3Vt (around 60mV).
The voltage across R2 will therefore
be 23Vt or about 600mV. The output
voltage, Vout, will be this voltage plus
the Vbe drop in transistor Q3 for an
output of around 1.2V.
Importantly, the tempco of Vout will
be that of Vbe3, around -2.01mV/°C,
plus 23 times that of V t (23 ×
+86.2µV/°C = +1.98mV/°C), resulting
in an overall tempco of -27.4µV/°C,
which is around 10ppm per °C. Not
bad for three transistors.
This type of reference is called a
bandgap reference because its output
voltage for zero tempco corresponds
with the theoretical bandgap voltage
of the semiconductor material (~1.14V
for silicon).
Paul Brokaw developed an improved
circuit in 1974, overcoming some of
the limitations of the Widlar circuit,
which could only produce a 1.2V output and required a fairly constant supply current. Brokaw’s circuit is shown
in Fig.4.
Brokaw’s circuit uses transistors
with identical collector currents (due
to identical R3s), but with differing
physical on-chip areas to achieve
different current densities. The voltage across R1 is the difference in
base-emitter voltages, Vt × loge(N)
where N is the ratio of transistor areas.
The voltage across R2 is therefore Vt
× loge(N) × 2(R2 ÷ R1), which has a
positive tempco due to Vt.
The reference output voltage will be
this voltage plus the base-emitter voltage of Q1 with its negative tempco. By
choosing the right values for R1, R2
and N, you can cancel the temperature
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dependencies as we did before. Fig.5
shows the same circuit configured to
provide output voltages higher than
the nominal 1.2V bandgap voltage.
You can buy off-the-shelf bandgap
references for around 60¢ each. The
Microchip LM404x series, for example, are packaged as shunt references
and available with output voltages
from 1.225V to 5.000V. The 2.5V version in C grade has an absolute accuracy of ±0.5%.
The versatile and very popular
TL431 is even cheaper. This is also
a 2.5V reference with a ±0.5% initial accuracy (C grade) with a typical
tempco of ±10ppm/°C. You frequently
see these devices in the voltage regulation circuits of low-cost flyback
switch-mode power supplies.
Many Silicon Chip projects have
used them too. For example, the DC
Supply Protectors project (June 2024;
siliconchip.au/Article/16292) used
one to set the over-voltage threshold.
The 500W Power Amplifier (AprilJune 2022; siliconchip.au/Series/380)
also used two, as part of the load-line
protection circuitry.
Exotic references
Another more exotic voltage reference technology is the ‘JFET pinchoff’ reference. These work on a similar
principle to the bandgap reference in
that the difference in pinch-off voltage
of two JFETs has a negative tempco
that offsets the positive tempco of a
current source.
The ADR420 reference uses this
technique to achieve an initial accuracy of ±400ppm (B grade) with a
tempco of ±3ppm/°C. Its long-term stability is 50ppm/kh. The big advantage
of this type of reference over bandgap
references is their very low noise.
Another interesting reference technology is the floating gate reference.
These rely on a Mosfet (actually an
array of Mosfets) with a well-insulated
‘floating’ gate. At manufacture, charge
is applied to the gate which, like a
capacitor, charges to a particular voltage.
The Mosfet then acts as a high-
impedance voltage follower to read out
this voltage. The voltage will remain
stable as long as the gate charge does
not change.
The only commercial examples I
am aware of are in the ISL2090 series.
The 2.50V B-grade version has an initial accuracy of ±0.02%, a tempco
siliconchip.com.au
of ±7ppm/°C and long-term stability of 20ppm/kh. By my calculations
(assuming a gate capacitance of 100pF
charged to 1V), the gate leakage must
be something less than 12 electrons
per hour! Amazing.
Voltage reference noise
Depending on your application, you
may have to take voltage reference
noise into account. Unlike op amps,
there is little consistency in how manufacturers specify the noise in their
voltage references, especially at very
low frequencies (say, below 10Hz).
This is the area we usually operate in, and it is the territory where 1∕f
noise tends to dominate, meaning we
can’t just extrapolate from a wideband
noise voltage to a noise density figure.
Because we are dealing with DC
signals, we can almost always add
some filtering to reduce the voltage
noise. Many references come with a
‘noise reduction’ pin that you bypass
to ground with a small capacitor to
improve the noise performance.
For example, the MAX6225ACSA
has such a pin which, if bypassed with
a 1µF capacitor, will reduce the noise
density above 100Hz from around
40nV/√Hz to under 15nV/√Hz.
If we add an external filter, we have
to make sure it does not adversely
influence the reference voltage. Fig.6
shows one example of how we could
do this. R1 and C1 form a low-pass filter with a -3dB frequency of 0.016Hz.
The bottom end of C1 is bootstrapped
by R2/C2 so that the voltage across C1
is zero in the steady state.
If we did not do this, the leakage
current through the capacitors would
cause a voltage error as it is dropped
across R1. You should also use a lownoise precision op amp buffer so that
you don’t add new errors.
Miscellany
Precision voltage references can be
expensive, so it is worth treating them
with respect. Below are a few considerations you may need to be aware of,
depending on your application.
Solder shift: the worst thermal
shock a voltage reference is likely to
experience is during the assembly process, particularly if it is reflowed onto
the printed circuit board (PCB). Like
thermal hysteresis, this can cause a
permanent change in the output voltage, known as ‘solder shift’.
You generally won’t find information
siliconchip.com.au
on this in the data sheets, but there are
a few app notes out there that discuss
it. It is only going to be of concern for
very high precision applications but is
worth knowing about. You might want
to hand-solder the reference if your
application falls into this category.
Start-up time: many references use
their own output to provide stabilised bias conditions (like the circuit
in Fig.2), so they include start-up circuitry to ensure everything comes up
in an orderly fashion. This means that
the output voltage might not reach its
final stable value for some time.
It is not unusual for this time to be
tens or even hundreds of milliseconds.
Your application should be aware of
this and not use the reference until it
is stable.
Board flex: flexing a PCB that contains a precision reference can produce a measurable change in the output. One manufacturer suggests this
can be as much as a 60ppm peak-topeak change for a reference mounted
on a standard 1.6mm FR4 board that
is 100mm wide board and flexed up
and down by 1.8mm.
You can minimise such mechanical
stress by fixing boards down firmly
and/or by using slots in the board to
mechanically isolate the reference.
Leakage: leakage currents across the
surface of a printed circuit board can
cause errors in precision references.
References with noise-filtering pins
(eg, the MAX6225ACSA) can be especially vulnerable, since these usually
expose a high-impedance summing
node to the outside world.
A few tens of nano amps flowing
into or out of one of these nodes can
shift the output voltage by hundreds
of ppm. Flux contamination or skin
oils are more than enough to allow
this level of current leakage, so it pays
to clean your precision boards thoroughly and to keep your fingers off
them once you have.
Fig.4: the Brokaw band gap
reference uses two transistors with
the same collector currents, but of
differing areas to produce a voltage
across R2 with a positive tempco to
offset the negative tempco of Q1’s
base-emitter voltage.
Fig.5: the Brokaw band gap
reference can easily be adapted to
produce higher output voltages.
Conclusion
Precision voltage references are
unique in that they are one component that combines both precision and
accuracy, allowing the device they are
used in to deal in absolute quantities.
In the next and final article of this
series, we will zoom out and look at
the big picture – how one might go
about the high-level design of a precision electronics device from a wholesystem perspective.
SC
Australia's electronics magazine
Fig.6: this RC filter reduces the
noise voltage produced by a voltage
reference by limiting the bandwidth
to 0.016Hz. R1 and C1 are the filter,
while R2 and C2 bootstrap the
bottom of C1 to eliminate its leakage
current, which would be otherwise
be dropped across R1, causing the
reference voltage to drop.
June 2025 73
M
easy-to-build
Outdoor Subwoofer
By Julian Edgar
any people have outside speakers
in a deck or patio area, but they
are often small, wall-mounted designs
that lack adequate bass response. This
subwoofer project can add a lot of that
missing bass. Because it’s built around
a fibre cement stool available from
Bunnings, very little woodworking is
needed, and the enclosure is weather
resistant.
This design includes a simple and
cheap protection mechanism that
makes the subwoofer very hard to blow
up (that’s always a danger with small
subwoofers). Depending on your interior décor, it can also be used inside.
The enclosure
The subwoofer enclosure is based
on an elegant white cement stool available from Bunnings, called the “Marquee 350 × 350 × 450mm Stool Side
Sorrento” (I/N 0596376). It costs $69
and, while completely hollow, still
weighs a little under 14kg. You don’t
need to modify it; you simply glue
an internal panel into it and add feet.
Fibre cement is a good material for
speaker enclosures, as it is acoustically
dead (it doesn’t ‘ring’ when tapped)
and is quite stiff. This stool is even
stiffer than most because it uses a
ribbed wall design. The fibre cement
can be painted any colour you want.
If you wish to make the subwoofer
using another design of stool, or even
(gasp!) from MDF or similar, the key
dimension is that a volume behind the
drivers of about 18L is required.
The drivers
This passive subwoofer is designed to be used on an outside deck
or patio. It is quick and easy to build, and will add substantial
bottom-end to your small exterior wall speakers. It’s also largely
weatherproof.
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74
Excellent frequency response for its size
Inbuilt protection against being over-driven
Medium-power design suitable for amplifiers up to 100W
Uses low-cost drivers
Easy and quick construction
Largely weatherproof, suitable for undercover outdoor use
Can also be used indoors
Can be painted any colour to match décor
Frequency response: 35-200Hz
Impedance: 4Ω
Silicon Chip
Australia's electronics magazine
Two drivers are used, mounted in
an isobaric (face-to-face) configuration. Both are 170mm (6.5-inch) WS
17 E units made by Visaton. Note that
you need the 8W versions.
These speakers are available worldwide – a web search will find your
nearest stockist. We bought ours from
RS Components (Stock No 431-8563),
but they ended up coming from the
UK. A major criterion in their selection is that they are cheap – about $47
each, including GST.
The speakers come with full ThieleSmall specifications, allowing computer modelling of the enclosure. Still,
when bench tested with the Smith and
Larsen Woofer Tester hardware/software package, the tested specs of the
two drivers differed somewhat from
the official specifications, even after
being ‘run in’.
siliconchip.com.au
Table 1 shows the advertised specifications, the test results and the final
values used in the modelling. Note
that the stated maximum cone displacement is 13mm – something we’ll
come back to later.
Enclosure modelling
Three different designs were modelled using the freely available WinISD speaker enclosure design software.
These designs were sealed, ported and
a 4th-order band-pass configuration.
Fig.1 shows the modelled response
curves of each design approach.
The aim was to achieve a response
from about 150Hz down to 40Hz.
Good efficiency was also important –
that is, the greatest output for a given
power. Given that the bare driver
has a fairly low efficiency (85dB at
1W/1m), achieving maximum efficiency becomes an important part of
the enclosure design.
Of the three designs, the sealed
approach was the worst in efficiency
and had a lower -3dB point of about
43Hz.
The band-pass design had a much
higher efficiency, about 4.5dB louder
in the critical area, so the equivalent of having 2.8 times the amplifier
power! It had a modelled -3dB point
of about 42Hz, but as is the characteristic of such band-pass designs, fell
away quickly at the top end, being 3dB
down at 110Hz. This concerned me,
as many small outdoor speakers will
struggle to get down to 110Hz.
The ported enclosure had a -3dB
point of 36Hz (substantially better
than the other designs), and was nearly
3dB up at 110Hz. It peaked at about
65Hz (over 6dB up) and had a greater
‘area under the curve’ than the other
two designs. It was modelled using
a 100mm-long, 50mm inner diameter port.
Note that I was not aiming for a flat
response – since the sub can be used
outside, it needs as much gain as possible without becoming crazily peaky.
This modelling was just a starting
point – it’s easy to look at lines on a
PC screen and think that they represent reality, not just a model of reality. However, software modelling is a
good way of getting into the region of
what is wanted.
What counts as a subwoofer?
A traditional subwoofer works only at very low frequencies – for example,
below 40Hz. That is, the subwoofer provides output below the frequencies of
a conventional woofer. However, over time, this definition has become blurred.
Computer sound systems, for example, typically use two small satellite
speakers that might work down to only 200Hz, with the separate ‘subwoofer’
providing the frequencies below this. Many high-level and custom car sound
systems use a subwoofer, but again, it typically provides the bass component
below 100-200Hz.
So rather than developing only very low frequencies, a subwoofer has come
to be known as any separate speaker that provides the bass.
If you’re listening to music, how low a frequency response is actually
required? The response of human hearing is stated as being 20-20,000Hz.
However, age reduces this range, and 20Hz can arguably be more clearly felt
as vibrations than heard.
A pipe organ can produce notes at just 16Hz, but few pipe organ recordings
have this low frequency content. There’s not much point in including sounds that
no speakers will reproduce! A bass guitar and a double bass go down to 41Hz,
which is clearly audible. A bass drum can produce frequencies of 20-120Hz,
usually centred around 40Hz. The lowest note on a standard piano is 27.5Hz.
So, while having as low a frequency response as possible is desirable, in
the real world, a speaker system that can reproduce down to 40Hz will give
the vast majority of what is needed. Whether you then call that speaker a subwoofer is up to you!
This subwoofer is not designed to fill large outside areas with booming bass.
To do so, it would need to be about ten times as big, ten times as expensive
and ten times as powerful! Instead, it’s designed to add bottom-end and body to
normal background music played at quiet-to-moderate levels in outdoor areas.
Fig.1: the model outputs (predicted frequency responses) for three different
enclosure designs: sealed (blue), band-pass (red) and ported (green). The
ported design was chosen.
Table 1 – WS 17 E 8Ω specifications
Specification Listed
Speaker A
Speaker B
Used in modelling
DC resistance 6.3W
6.1W
6.2W
–
Sensitivity <at> 1W/1m 88dB
85dB
85db
–
Resonant frequency 41Hz
45Hz
43Hz
44Hz
Qms 2.83
3.45
3.22
3.4
Isobaric configuration
Qes 0.81
1.10
1.01
1.1
The two drivers are mounted in
an isobaric configuration – that is,
Qts 0.63
0.83
0.77
0.8
Vas 31L
25L
27L
26L
siliconchip.com.au
Australia's electronics magazine
June 2025 75
Photo 1: the Bunnings fibre
cement stool. Making it into a
subwoofer doesn’t change its
appearance much – it will
just have a slightly larger
gap at its base.
Source: Bunnings
Photo 2:
this halogen
incandescent
light bulb
is used as
the speaker
protector. Its
resistance
rapidly
rises
as the
current
flow through
it increases,
limiting the
maximum
speaker power.
Source: Narva
face-to-face with a small, trapped air
volume between them. The drivers
are wired out of phase so that as one
pushes, the other pulls.
The advantage of an isobaric configuration is that the drivers act as if
they are working in a larger enclosure
volume, and most importantly from
our perspective, the power handling
of the drivers doubles from a nominal 60W (90W peak) to 120W (180W
peak).
The use of paralleled drivers
explains the need for selecting 8W
designs – the two drivers then form
a nominally 4W amplifier load. The
WinISD software can model isobaric
configurations.
Test and development
To initially test the design, a disc
of 22mm-thick weatherproof particleboard was cut so that it would
sit within the upturned stool, about
130mm down from the end. This
placement gives room for the drivers
and the port to project from both sides
of the baffle.
Two holes were cut in the particleboard disc – one for the drivers and the
other for the port. The hole for the port
was made a tight fit so that different
lengths of 50mm ID PVC plastic pipe
could be trialled. The gap between the
edge of the particleboard disc and the
inner wall of the stool was temporarily sealed.
A layer of polyester quilt wadding
76
Silicon Chip
was placed inside the enclosure, with
care taken that it did not block the port.
The wadding prevents sound reflections off the hard interior surfaces.
The subwoofer stool could then be
tested upside-down. A frequency generator app (Signal Gen from Media
Punk Studios) on an iPhone was used
in conjunction with an audio amplifier to test the subwoofer on sine wave
sweeps from 150Hz down to 25Hz.
Always test at low volumes – you
can easily blow up drivers with sinewave testing!
Different port lengths were trialled,
with a 190mm-long port giving better
results to my ears than the modelled
100mm port. Yes, that’s a big difference, implying the enclosure tuning
point has moved from about 47Hz
down to about 35Hz. Testing of the
completed enclosure showed an actual
enclosure tuned frequency of 38Hz.
Using shorter ports than 100mm
gave a much peakier response – something the software modelling had
shown would be the case. For example,
using a 50mm ID port that was only
40mm long gave a modelled +10.5dB
peak at about 75Hz. Therefore, if
you’re not unduly concerned about
one-note bass and just want it louder,
use a shorter port like this.
Extensive testing with music followed, and this showed something
else. Because these are not expensive
drivers with huge cone travel, driving the sub hard could bottom-out the
drivers’ suspensions. This is important
to understand, because many people
Speaker resonance and one-note bass
Many people confuse a good bass response with a pronounced bass resonance. I remember when I was young and trying to make my car sound system
perform well. I’d fitted a new amplifier, new speakers and a new head unit (a
cassette player in those days!). In one particular song, a note from the bass
guitar caused the whole car to vibrate… something I thought was really cool.
What was happening was that a major speaker resonance was being triggered, and that excited the car. Nowadays, I’d see that as a shortcoming!
A speaker resonance is where, for a given power input, the audio output
of the speaker sharply peaks. That is, at a particular frequency, the speaker
is much more efficient at turning electrical input power into an audio output.
The problem with a subwoofer having a pronounced resonance is that the
output at that frequency will dominate the rest of the content. This is often
termed ‘one-note bass’. One-note bass is the thump, thump you often hear in
poor sound systems – all the bass, no matter its actual frequency, is reproduced as much the same-sounding thump.
Australia's electronics magazine
siliconchip.com.au
Photo 3: the underside view
of the baffle with the
speakers, port, protection
light bulb and terminal
strip temporarily
mounted. In the
final design, some
of the parts were
orientated slightly
differently.
Photo 4: a closeup showing the
8mm flanged
nuts used as
spacers between
the speaker
mounting lugs,
the protection
light bulb
mounted on its
bracket and the
terminal strip.
over-drive subs without realising that
they are doing so.
When developing a subwoofer,
always test it with a crossover and
without the other speakers running.
That is, listen to just the sub working
at only low frequencies. This way,
you can hear what is really happening, without the sound being masked
by the other speakers.
the speaker system, they will dominate the sound.
For example, without a sub crossover, the lower midrange can be
over-emphasised. Crossovers can be
achieved by using a series inductor
in the subwoofer speaker feed (not so
good), or much better, using an electronic low-pass or band-pass filter.
Subwoofer crossovers
Two solutions were developed
to prevent the sub from being overdriven. The first was to temporarily place a heavy lid on top of the
upturned sub, raised from the stool
body by 10mm spacers. This replicates how the sub will actually be used
– inverted and placed on the ground
on short feet.
The use of this lid (or in use, the
presence of the ground) better acoustically loads the drivers, reducing
their displacement peaks. Technically,
we’re also adding another chamber
and port (the gap around the periphery), but that made little difference
to the sound except that upper frequencies were better suppressed. You
don’t want these coming out of a sub
anyway.
The other solution was electronic –
or at least, electric. Many professional
speakers used in commercial settings
have a very simple approach to protecting (especially) the tweeters. They
place a normal incandescent light bulb
in series with the drive to the speaker.
A subwoofer – especially a small
one like this – must be ‘crossed over’.
It must not be fed frequencies outside the range of those you’re trying to
reproduce. The reason for this is that a
small sub can easily reproduce higher
frequencies, and if you have the sub
producing them as well as the rest of
Photo 5: two of these Visaton 170mm
(6.5in) drivers are used in the
subwoofer, mounted in an isobaric
configuration. Source: Visaton
siliconchip.com.au
Speaker protection
Australia's electronics magazine
Low-voltage incandescent light
bulbs have low resistance (eg, 0.7W)
when they are cold but about 15 times
as much resistance when they are hot
– that is, when the filament is glowing brightly.
Therefore, as the current flowing
through the bulb increases, so does its
resistance, limiting the power getting
to the protected speaker. We decided
to take a similar approach to protect
the subwoofer drivers.
Many different light bulbs were
tested, including those with different
voltages and wattages, and multiple
bulbs wired in series, parallel and
series/parallel configurations. The aim
was to limit power to the subwoofer
such that the speakers could not be
overdriven on a variety of music. However, a lot depends on the amplifier you
are using, the type of music you play
– and how loudly you play it!
While the light bulb approach has
audio downsides (it is a non-linear
compressor), and so is frowned on
by purists, it works very effectively.
Depending on the music type and
power level, the bulb may not glow at
all, glow just a little, or light brightly.
Furthermore, it has a short-term
memory in that if the power is repeatedly high (eg, you are loudly playing
a song with lots of bass), the filament
stays warm and so limits the power
earlier. To put this another way, if the
subwoofer is constantly being overdriven, the sub output drops a lot – it
June 2025 77
Light bulb based speaker power limiters
The question that is always asked by people wanting to use light bulbs as
speaker power limiters is how to choose the correct bulb for the application.
The bottom line is that it is nearly impossible to do it theoretically – testing is
the only practical way.
The difficulty with trying to specify the required light bulb theoretically is
that the resistance posed by the bulb constantly varies with filament temperature. In turn, this is governed by the light bulb’s characteristics, amplifier
power, the type of music being played and the impedance curve of the speaker
being protected.
If we were using a sinewave as the signal, it would all become much simpler – but we aren’t.
Even the bulb’s maximum continuous power dissipation (ie, the wattage
rating) isn’t as useful as it might first appear. In our application, the bulb is
required to dissipate large amounts of power only on very short transients.
Therefore, the power limiting that occurs depends in part on the response
speed of the filament.
Furthermore, the filament has a thermal memory. If it is dissipating large
amounts of power in successive bursts (eg, there is a rhythmic bass beat),
the filament stays hot between the bass notes. It therefore has a higher constant resistance and so the expected high pulses of amplifier power are not
fully developed!
Based on the voltage swings of the audio signal, it would appear obvious
that a bulb with a higher voltage rating (eg, 60V) should be used – however,
such a bulb has a higher cold resistance, so it will reduce amplifier output
power all the time. That is not what we want.
In the case of the project described here, the 24V 55W halogen bulb worked
well. A similar result could also be achieved using multiple 24V 18W tail-light
bulbs. However, they were more expensive to buy than the single 55W bulb.
It’s a fascinating area, and we’d love to hear about any successful results
readers have gained using light bulbs for speaker protection.
Two light
bulbs
used to
limit the
power in
a Bose
Lifestyle
speaker
system.
is actually louder when the amplifier
is turned back down.
By watching the filament lamp
during testing, you can also get a very
good idea of when the speaker is being
driven too hard and so reduce the maximum power the sub will ever see.
(More on setting up the amplifier later.)
If, in ‘normal’ use, some crazy dude
gets hold of the amplifier knob and
cranks it right up (eg, when you’re
away on holiday and the kids decide
to host a party!), the light bulb will
protect the speaker. If the worst comes
to the worst, the bulb will likely blow
before the drivers do, cutting off the
subwoofer output.
We have nominated using a single
Narva 24V 55W bulb (part number
48701). This bulb costs about $10 from
automotive parts shops. It is difficult
to over-drive the sub on normal music
with this bulb wired in series, using
any amplifier up to about 100W.
However, if you want to be less conservative, using two of these bulbs in
parallel gives more subwoofer power
but still some protection. Of course,
you can choose to delete the protection bulbs entirely and use only a lowpower amplifier. However, we suggest
using the single light bulb.
Despite the combined drivers being
rated at 180W peak, this does not mean
that if the sub is used with an amplifier
having less power than 180W, the sub
requires no protection. Remember, the
protection is primarily to protect the
drivers from being over-driven rather
than their voice coils being burned out.
Warning: if the subwoofer is continuously overdriven, the protection
lamp will become very hot. The subwoofer should always be placed on a
firm, level and non-combustible surface like tiles, concrete or similar. It
should not be placed on dry grass.
Construction
Construction is easy, and should
take you only about an hour, spread
over two days. The steps are:
1. Make the baffle and trial-fit the
speakers, port, protection lamp and
terminal strip to it.
2. Disassemble the baffle, removing
all the parts.
3. Glue the baffle, port and feet in
place and let the glue harden for 24
hours.
4. Fit and wire the speakers, protection lamp and terminal strip.
5. Test it.
78
Silicon Chip
Australia's electronics magazine
siliconchip.com.au
Photos 6 & 7: the baffle and port glued into place with Liquid Nails. The port
protrudes from both sides of the baffle, while the two drivers are positioned
face-to-face in the opening. The towel under the stool protects this surface when
working on the subwoofer. Once the glue has hardened, you can paint the inside
of the enclosure, the baffle and the port tube.
Photo 8: a close-up of the protection
lamp and terminal strip wiring. Note
the cable going through the baffle to
the other speaker.
The first step is to use a jigsaw to cut
a disc of particleboard about 285mm
in diameter. Measure the maximum
diameter of the opening in the stool’s
base – the disc should be just smaller
than this. The stools are handmade
and so vary a bit in size.
We used 22mm-thick, moisture-
resistant particleboard (a flooring
offcut), but if you seal it on all sides
with paint before gluing it into place,
slightly thinner MDF should be fine.
Don’t use material less than about
18mm thick – the peripheral glue
needs plenty of ‘meat’ to adhere to.
Cut a 165mm hole in the baffle for
the drivers to sit in, and mark and
drill small diameter pilot holes for
the particleboard screws that will
hold the drivers in place. Next, use
a hole saw to make the opening in
the baffle for the 50mm ID PVC pipe.
The required hole diameter is 56mm
– if you don’t have a hole saw of this
diameter, make a smaller hole and
then file it to size.
The exact location of these holes is
not critical – just ensure the speakers
and port clear the inner walls of the
stool. We recommend proper safety
precautions when cutting MDF, such
as using a respirator and cutting in a
well-ventilated location.
Drill a small hole for the inside
speaker’s cable to come through from
the other side of the baffle.
Cut a suitable speaker gasket from
a thin foam rubber sheet before dropping the first speaker into place. In the
final assembly, you can use silicone if
on the baseplate and enlarge this hole
to 3mm. Be very careful when drilling
these holes – it is easy to damage the
lamp (eg, by dropping it).
The lamp mounts on a small
right-angle bracket that is attached to
the baffle with a wood screw. Wiring
connections to the lamp are by two
solder lugs that are attached with the
3mm screws.
Ensure the baffle assembly will
fit inside the stool without the port
fouling the inside wall. When you
are happy that everything will fit correctly, remove the baffle and disassemble it. If using non-weatherproof MDF,
paint the baffle on both sides and on
all cut edges.
Spread ‘water clean-up’ Liquid
Nails (or equivalent) building adhesive at an appropriate height around
the inside of the stool where the baffle
will sit. Be generous with this glue –
you want no leaks and for the baffle
siliconchip.com.au
you don’t want to make a gasket. The
other speaker fits on top, so they mount
face-to-face (see Fig.2).
These speakers have an external
gasket, so they seal to each other very
well – no further gasket or sealant is
needed between them.
Use 6mm spacers between the two
sets of speaker mounting holes so
that the speakers are clamped firmly
together, but the mounting tags are
not overly bent. I used 8mm flanged
nuts that had the required 6mm depth.
The particleboard screws go through
both sets of speaker mounting tags and
the spacers, holding the two speakers
firmly to the baffle.
Push the 190mm PVC pipe through
the hole in the baffle; the pipe projects
about equally from each side.
Next, mount the protective light
bulb. To do this, enlarge the existing
hole in the bulb’s bottom tang to 3mm.
Nip off one of the nipple protrusions
Fig.2: the two drivers are
mounted face-to-face, being
inserted into the baffle from
the underside of the enclosure.
Australia's electronics magazine
June 2025 79
to be held in place very firmly. Ensure
the glue is the water clean-up type or it
will be difficult to remove the excess!
(We suggest “Liquid Nails Fast Grab”,
Bunnings I/N 1230096).
Carefully drop the bare baffle into
place and push it down onto the glue,
ensuring the baffle stays level. Apply
more glue around the gap between the
baffle and the inside of the stool and
smooth the glue with a wet finger, wiping up any excess with a wet cloth that
you repeatedly rinse in water. Insert
the vent, also sealing it into place with
the glue.
Let the glue harden for at least 24
hours. You may choose to paint the
interior of the stool at this stage –
ie, the baffle, glue and visible inside
wall of the stool. I did so using black
spray paint.
A single layer of quilt wadding,
about 500 × 500mm can now be glued
in the bottom of the enclosure (the
top when it is orientated normally).
This step is optional – I am not sure
it makes a great deal of difference, but
it will possibly reduce ‘hollow sounding’ reflections.
Place the gasket on the underside of
the first speaker or, if not using a gasket, apply silicone around the upper
edge of the hole.
Solder the speaker’s connecting
cable to its terminals, then feed this
wire through the baffle hole, pushing
it from the inside by placing your hand
through the speaker hole.
Ensure you know the polarity of your
connections, eg, by using coloured
wires or a cable with a trace on one
conductor.
Put the first speaker into place and
then mount the second speaker on top,
remembering to include the spacers.
Insert the four screws and tighten in a
series of steps using a diagonal tightening pattern.
Wire the two speakers out of phase
– the inside speaker’s positive connection goes to the outside speaker’s negative and vice versa (see Fig.3). Seal
the wiring hole in the baffle.
Next, install the protective light
bulb. It mounts on a small bracket that
is attached to the baffle with a particleboard screw (drill small diameter pilot
holes for the screw). Do not place the
lamp against the PVC vent.
If you have touched the bulb’s glass
at any point in the installation process,
wipe it with a cloth moistened in methylated spirits. This removes any oils
that may have been deposited on the
glass from your fingers, which could
potentially weaken the glass.
The terminal strip mounts next,
again with a particleboard screw into
a pilot hole. Wire the drivers to the
terminal strip with the light bulb in
series (it doesn’t matter which lead
it goes in).
Because the outside driver pushes
air outwards when the cone moves
backwards (rather than the normal
forwards), the negative terminal of the
outer driver connects to the positive
speaker connection terminal. Mark
this with a (+).
Should the vent be flared?
The vent uses straight rather than
flared ends. Flared ends reduce port
noise (sometimes called ‘chuffing’).
However, considering the size of the
drivers and their isobaric configuration, a large diameter vent has been
used, so air velocities in the port are
relatively low. No port noise could be
heard even without flares.
Photo 9: testing the subwoofer with Niles wall-mounted speakers on a deck under construction. The ceiling is 2.7m high,
and the deck area is about 10 × 5m. On a deck this large, two subwoofers spaced about 5m apart will give the best results.
80
Silicon Chip
Australia's electronics magazine
siliconchip.com.au
Testing
The next step is to test the subwoofer. Place it upright on its feet on
a firm, flat surface. Feed the subwoofer
through an amplifier and crossover,
and ensure other speakers cannot
be heard. Use a frequency generator
app to perform a sweep from 200Hz
down to 20Hz. The speaker should
be audible down to about 35Hz, and
there should be no buzzes, whistles
or rattles.
If there are, isolate where the sound
is coming from (eg, a loose port or leak
around the frames of the drivers) and
then fix the problem. If you hear a
buzz, ensure it’s not something in the
room becoming excited, rather than
the subwoofer itself.
If the bass output is poor, check the
speaker phasing, ensuring the speakers are wired out of phase.
Now switch to the type of music
you normally play. Do not run any
high-power tests with the frequency
generator. Ensure you can see if the
light bulb is glowing brightly – eg, in
dim conditions, it will cast a visible
ring of light around the open base of
the enclosure. Increase the amplifier
gain until the filament is just glowing
on bassy passages.
Now, while not changing the amplifier gain, select music of the type that
has as much bass as you will ever listen to. The light bulb(s) should light
quite brightly on these greater bass
passages, showing the protection is
working, and the drivers should not
bottom out.
If the bulb is glowing brightly a lot
of the time, the amplifier gain is too
Fig.3: wire the two speakers out of
phase so that as one pushes, the other
pulls (and vice versa). The protection
light bulb is inserted in one conductor
of the main feed (either is OK).
siliconchip.com.au
Parts List – Outdoor Subwoofer
2 Visaton WS 17 E 8W speakers [RS Components 431-8563;
there are many other suppliers]
1 Marquee Sorrento 350 × 350 × 450mm Side Stool [Bunnings I/N 0596376]
1 300 × 300mm 22mm-thick weatherproof particleboard sheet
1 190mm length of 50mm internal diameter PVC DWV pipe
4 25mm diameter, 10mm thick white rubber feet
1 cartridge of water clean-up Liquid Nails [Bunnings I/N 1230096]
1 Narva 48701 24V 55W automotive light bulb [Car parts supplier]
1 500 × 500mm section of dressmaker’s quilt wadding [Spotlight]
1 small terminal strip (eg, 2-way)
1 packet of self-tapping particleboard screws
various lengths of wire & cable
assorted small hardware items (screws, washers, nuts etc)
4 6mm spacers (particleboard screws must fit through)
1 thin foam rubber sheet
1 small steel right-angle bracket
high. Of course, depending on the
amplifier power, you may not see the
bulb light at all.
Results
The prototype speaker had good
output from 35Hz to 200Hz. Furthermore, the response was pleasingly
smooth across this range. The measured impedance did not drop below
4W at any point in the frequency range.
Using the specified protection lamp,
amplifier powers up to 100W should
be fine when playing normal program
material.
Setup
Remember that the subwoofer needs
its own amplifier, and that amplifier needs either a built-in subwoofer
crossover or to be fed only low frequencies via an electronic crossover. Lowcost Class-D subwoofer amplifiers with
built-in crossovers are readily available, but it can be much cheaper to use
a surplus, bridgeable stereo amplifier
with an adjustable subwoofer crossover on its input.
The location of the subwoofer is
important. Placing the subwoofer at
the intersection of a wall and the floor
causes greater loading of the speaker’s
drivers. As a result, the energy of the
speaker is better communicated to the
air, so the bass output will increase.
Placing the sub at the intersection of
two walls and the floor increases this
effect even more.
Conversely, placing the sub on a
pedestal in the middle of the room or
outdoor area will reduce the output.
Large changes in output are achievable
by these various placements.
Australia's electronics magazine
The other aspect of placement is that
when used outside, the closer the sub
is to you, the more its presence will be
felt. Unlike in a small room, where the
loudness of the sub doesn’t vary much
wherever you are in the room, outside
the low frequencies are clearly louder
when you are closer to the sub. Therefore, place it near where you will most
often be sitting.
When placed on the floor against a
wall, the sub was effective over about
a 25m2 area – it works fine in an open
area about 5 × 5m. If your deck or patio
area is larger than this, you could use
two of these subs.
To limit cone movement, the open
end of the sub should always be
placed on the ground (spaced upwards
by its feet). If the sub is to be used
upside-down with the opening facing upwards, a heavy panel should be
placed over the opening, again spaced
upwards by about 10mm.
The sub is weatherproof in that
the concrete stool can cope with rain
or being sprayed with a hose. However, the sub is open underneath, so it
should not be placed on grass or any
other surface where there is moisture
present all the time. If washing a deck
or other outside area where the sub is
placed, move it first.
You may occasionally wish to spray
some insecticide into the interior of
the enclosure (including through the
port) to prevent bugs and spiders making colonies.
Finally, if you can obviously hear
that the sub is working, it’s probably too loud – it should be just part
of the music, not a separate, identifiable entity.
SC
June 2025 81
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Power LCR Meter (Mar25)
PIC16F15214-I/P Digital Volume Control Pot (TH; Mar23), Filament Dryer (Oct24)
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PIC16F15224-I/SL Multi-Channel Volume Control (OLED Module; Dec23)
PIC32MX170F256B-50I/SO + PIC16F1455-I/SL
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NFC IR Keyfob Transmitter (Feb25), Rotating Light (Apr25)
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PIC32MZ2048EFH064-I/PT DSP Crossover/Equaliser (May19), Low-Distortion DDS (Feb20)
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W27C020
Noughts & Crosses Computer (Jan23)
KITS, SPECIALISED COMPONENTS ETC
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(JUN 25)
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(MAY 25)
RGB LED ‘ANALOG’ CLOCK KIT (SC7416)
(MAY 25)
USB POWER ADAPTOR COMPLETE KIT (SC7433)
(MAY 25)
Includes the PCB and all onboard parts (see p66, Jun25)
Includes everything in the parts list (including the case), except the optional
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PICO COMPUTER
(DEC 24)
FLEXIDICE COMPLETE KIT (SC7361)
(NOV 24)
MICROMITE EXPLORE-40 KIT (SC6991)
(OCT 24)
DUAL MINI LED DICE
(AUG 24)
AUTOMATIC LQ METER KIT (SC6939)
(JUL 24)
For full functionality both the Pico Computer Board and Digital Video Terminal kits are
required. Items shown unbolded are optional (see p71, Dec24)
- Pico Computer Board kit (SC7374)
$40.00
- Pico Digital Video Terminal kit (SC6917)
$65.00
- PWM Audio Module kit (SC7376)
$10.00
- ESP-PSRAM64H 64Mb SPI PSRAM chip (SC7377)
$5.00
- DS3231 real-time clock SOIC-16 IC (SC5103)
$7.50
- DS3231MZ real-time clock SOIC-8 IC (SC5779)
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Includes all required parts except the coin cell (see p71, Nov24)
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$35.00
(APR 25)
Includes an assembled PCB, separate Raspberry Pi Pico 2 and front/rear panels $120.00 DUAL-RAIL LOAD PROTECTOR (SC7366)
(OCT 24)
Hard-to-get parts: includes the PCB and all semiconductors except the
ROTATING LIGHT FOR MODELS KIT
(APR 25)
optional/variable diodes (see p73, Oct24)
$35.00
Complete kit which includes the PCB and all onboard components (see p60, Apr25):
- SMD LEDs (SC7462)
$20.00 PicoMSA PARTS (SC7323)
(SEP 24)
- Through-hole LEDs (SC7463)
$20.00 Hard-to-get parts: includes the PCB, Raspberry Pi Pico (unprogrammed),
plus all semiconductors, capacitors and resistors (see p63, Sep24)
$50.00
433MHz TRANSMITTER KIT (SC7430)
(APR 25)
Includes the PCB and all onboard parts (see p75, Apr25)
$20.00 COMPACT OLED CLOCK & TIMER KIT (SC6979)
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Includes everything except the case & Li-ion cell (see p34, Sep24)
$45.00
PICO 2 AUDIO ANALYSER SHORT-FORM KIT (SC6772)
(MAR 25)
The Pico Audio Analyser kit from Nov23, but with an unprogrammed Pico 2
$50.00 DISCRETE IDEAL BRIDGE RECTIFIER
(SEP 24)
Both kits include the PCB and everything that mounts to it (see page 83, Sep24)
USB PROGRAMMABLE FREQUENCY DIVIDER (SC6959)
(FEB 25)
- All through-hole (TH) kit (SC6987)
$30.00
Complete kit: includes all components (see p85, Feb25)
$60.00
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$27.50
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NFC PROGRAMMABLE IR KEYFOB (SC7421)
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Complete kit: includes all required items, except the cell (see p67, Feb25)
COMPACT HIFI HEADPHONE AMP (SC6885)
(DEC 24)
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(DEC 24)
Complete kit: includes everything except the power supply (see p47, Dec24)
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- Through-hole LEDs kit (SC6849)
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82
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hip sockets (see p36, Dec24)
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Australia's electronics magazine
June 2025 83
PRINTED CIRCUIT BOARDS & CASE PIECES
PRINTED CIRCUIT BOARD TO SUIT PROJECT
TINY LED ICICLE (WHITE)
DUAL-CHANNEL BREADBOARD PSU
↳ DISPLAY BOARD
DIGITAL BOOST REGULATOR
ACTIVE MONITOR SPEAKERS POWER SUPPLY
PICO W BACKPACK
Q METER MAIN PCB
↳ FRONT PANEL (BLACK)
NOUGHTS & CROSSES COMPUTER GAME BOARD
↳ COMPUTE BOARD
ACTIVE MAINS SOFT STARTER
ADVANCED SMD TEST TWEEZERS SET
DIGITAL VOLUME CONTROL POT (SMD VERSION)
↳ THROUGH-HOLE VERSION
MODEL RAILWAY TURNTABLE CONTROL PCB
↳ CONTACT PCB (GOLD-PLATED)
WIDEBAND FUEL MIXTURE DISPLAY (BLUE)
TEST BENCH SWISS ARMY KNIFE (BLUE)
SILICON CHIRP CRICKET
GPS DISCIPLINED OSCILLATOR
SONGBIRD (RED, GREEN, PURPLE or YELLOW)
DUAL RF AMPLIFIER (GREEN or BLUE)
LOUDSPEAKER TESTING JIG
BASIC RF SIGNAL GENERATOR (AD9834)
↳ FRONT PANEL
V6295 VIBRATOR REPLACEMENT PCB SET
DYNAMIC RFID / NFC TAG (SMALL, PURPLE)
↳ NFC TAG (LARGE, BLACK)
RECIPROCAL FREQUENCY COUNTER MAIN PCB
↳ FRONT PANEL (BLACK)
PI PICO-BASED THERMAL CAMERA
MODEL RAILWAY UNCOUPLER
MOSFET VIBRATOR REPLACEMENT
ARDUINO ESR METER (STANDALONE VERSION)
↳ COMBINED VERSION WITH LC METER
WATERING SYSTEM CONTROLLER
CALIBRATED MEASUREMENT MICROPHONE (SMD)
↳ THROUGH-HOLE VERSION
SALAD BOWL SPEAKER CROSSOVER
PIC PROGRAMMING ADAPTOR
REVISED 30V 2A BENCH SUPPLY MAIN PCB
↳ FRONT PANEL CONTROL PCB
↳ VOLTAGE INVERTER / DOUBLER
2M VHF CW/FM TEST GENERATOR
TQFP-32 PROGRAMMING ADAPTOR
↳ TQFP-44
↳ TQFP-48
↳ TQFP-64
K-TYPE THERMOMETER / THERMOSTAT (SET; RED)
MODEM / ROUTER WATCHDOG (BLUE)
DISCRETE MICROAMP LED FLASHER
MAGNETIC LEVITATION DEMONSTRATION
MULTI-CHANNEL VOLUME CONTROL: VOLUME PCB
↳ CONTROL PCB
↳ OLED PCB
SECURE REMOTE SWITCH RECEIVER
↳ TRANSMITTER (MODULE VERSION)
↳ TRANSMITTER (DISCRETE VERSION
COIN CELL EMULATOR (BLACK)
IDEAL BRIDGE RECTIFIER, 28mm SQUARE SPADE
↳ 21mm SQUARE PIN
↳ 5mm PITCH SIL
↳ MINI SOT-23
↳ STANDALONE D2PAK SMD
↳ STANDALONE TO-220 (70μm COPPER)
RASPBERRY PI CLOCK RADIO MAIN PCB
↳ DISPLAY PCB
KEYBOARD ADAPTOR (VGA PICOMITE)
↳ PS2X2PICO VERSION
MICROPHONE PREAMPLIFIER
↳ EMBEDDED VERSION
RAILWAY POINTS CONTROLLER TRANSMITTER
↳ RECEIVER
84
Silicon Chip
DATE
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JAN24
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FEB24
PCB CODE
16111192
04112221
04112222
24110224
01112221
07101221
CSE220701
CSE220704
08111221
08111222
10110221
SC6658
01101231
01101232
09103231
09103232
05104231
04110221
08101231
04103231
08103231
CSE220602A
04106231
CSE221001
CSE220902B
18105231/2
06101231
06101232
CSE230101C
CSE230102
04105231
09105231
18106231
04106181
04106182
15110231
01108231
01108232
01109231
24105231
04105223
04105222
04107222
06107231
24108231
24108232
24108233
24108234
04108231/2
10111231
SC6868
SC6866
01111221
01111222
01111223
10109231
10109232
10109233
18101231
18101241
18101242
18101243
18101244
18101245
18101246
19101241
19101242
07111231
07111232
01110231
01110232
09101241
09101242
Price
$2.50
$5.00
$5.00
$5.00
$10.00
$5.00
$5.00
$5.00
$12.50
$12.50
$10.00
$10.00
$2.50
$5.00
$5.00
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$10.00
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$5.00
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$12.50
$5.00
$5.00
$5.00
$1.50
$4.00
$5.00
$5.00
$5.00
$2.50
$2.50
$5.00
$7.50
$12.50
$2.50
$2.50
$10.00
$5.00
$10.00
$2.50
$2.50
$5.00
$5.00
$5.00
$5.00
$5.00
$10.00
$2.50
$2.50
$5.00
$5.00
$5.00
$3.00
$5.00
$2.50
$2.50
$5.00
$2.00
$2.00
$2.00
$1.00
$3.00
$5.00
$12.50
$7.50
$2.50
$2.50
$7.50
$7.50
$5.00
$2.50
For a complete list, go to siliconchip.com.au/Shop/8
PRINTED CIRCUIT BOARD TO SUIT PROJECT
LASER COMMUNICATOR TRANSMITTER
↳ RECEIVER
PICO DIGITAL VIDEO TERMINAL
↳ FRONT PANEL FOR ALTRONICS H0190 (BLACK)
↳ FRONT PANEL FOR ALTRONICS H0191 (BLACK)
WII NUNCHUK RGB LIGHT DRIVER (BLACK)
ARDUINO FOR ARDUINIANS (PACK OF SIX PCBS)
↳ PROJECT 27 PCB
SKILL TESTER 9000
PICO GAMER
ESP32-CAM BACKPACK
WIFI DDS FUNCTION GENERATOR
10MHz to 1MHz / 1Hz FREQUENCY DIVIDER (BLUE)
FAN SPEED CONTROLLER MK2
ESR TEST TWEEZERS (SET OF FOUR, WHITE)
DC SUPPLY PROTECTOR (ADJUSTABLE SMD)
↳ ADJUSTABLE THROUGH-HOLE
↳ FIXED THROUGH-HOLE
USB-C SERIAL ADAPTOR (BLACK)
AUTOMATIC LQ METER MAIN
AUTOMATIC LQ METER FRONT PANEL (BLACK)
180-230V DC MOTOR SPEED CONTROLLER
STYLOCLONE (CASE VERSION)
↳ STANDALONE VERSION
DUAL MINI LED DICE (THROUGH-HOLE LEDs)
↳ SMD LEDs
GUITAR PICKGUARD (FENDER JAZZ BASS)
↳ J&D T-STYLE BASS
↳ MUSIC MAN STINGRAY BASS
↳ FENDER TELECASTER
COMPACT OLED CLOCK & TIMER
USB MIXED-SIGNAL LOGIC ANALYSER (PicoMSA)
DISCRETE IDEAL BRIDGE RECTIFIER (TH)
↳ SMD VERSION
MICROMITE EXPLORE-40 (BLUE)
PICO BACKPACK AUDIO BREAKOUT (with conns.)
8-CHANNEL LEARNING IR REMOTE (BLUE)
3D PRINTER FILAMENT DRYER
DUAL-RAIL LOAD PROTECTOR
VARIABLE SPEED DRIVE Mk2 (BLACK)
FLEXIDICE (RED, PAIR OF PCBs)
SURF SOUND SIMULATOR (BLUE)
COMPACT HIFI HEADPHONE AMP (BLUE)
CAPACITOR DISCHARGER
PICO COMPUTER
↳ FRONT PANEL (BLACK)
↳ PWM AUDIO MODULE
DIGITAL CAPACITANCE METER
BATTERY MODEL RAILWAY TRANSMITTER
↳ THROUGH-HOLE (TH) RECEIVER
↳ SMD RECEIVER
↳ CHARGER
5MHZ 40A CURRENT PROBE (BLACK)
USB PROGRAMMABLE FREQUENCY DIVIDER
HIGH-BANDWIDTH DIFFERENTIAL PROBE
NFC IR KEYFOB TRANSMITTER
POWER LCR METER
WAVEFORM GENERATOR
PICO 2 AUDIO ANALYSER (BLACK)
PICO/2/COMPUTER
↳ FRONT & REAR PANELS (BLACK)
ROTATING LIGHT (BLACK)
433MHZ TRANSMITTER
VERSATILE BATTERY CHECKER
↳ FRONT PANEL (BLACK, 0.8mm)
TOOL SAFETY TIMER
RGB LED ANALOG CLOCK (BLACK)
USB POWER ADAPTOR (BLACK, 1mm)
DATE
MAR24
MAR24
MAR24
MAR24
MAR24
MAR24
MAR24
MAR24
APR24
APR24
APR24
MAY24
MAY24
MAY24
JUN24
JUN24
JUN24
JUN24
JUN24
JUL24
JUL24
JUL24
AUG24
AUG24
AUG24
AUG24
SEP24
SEP24
SEP24
SEP24
SEP24
SEP24
SEP24
SEP24
OCT24
OCT24
OCT24
OCT24
OCT24
NOV24
NOV24
NOV24
DEC24
DEC24
DEC24
DEC24
DEC24
JAN25
JAN25
JAN25
JAN25
JAN25
JAN25
FEB25
FEB25
FEB25
MAR25
MAR25
MAR25
APR25
APR25
APR25
APR25
MAY25
MAY25
MAY25
MAY25
MAY25
PCB CODE
16102241
16102242
07112231
07112232
07112233
16103241
SC6903
SC6904
08101241
08104241
07102241
04104241
04112231
10104241
SC6963
08106241
08106242
08106243
24106241
CSE240203A
CSE240204A
11104241
23106241
23106242
08103241
08103242
23109241
23109242
23109243
23109244
19101231
04109241
18108241
18108242
07106241
07101222
15108241
28110241
18109241
11111241
08107241/2
01111241
01103241
9047-01
07112234
07112235
07112238
04111241
09110241
09110242
09110243
09110244
9049-01
04108241
9015-D
15109231
04103251
04104251
04107231
07104251
07104252/3
09101251
15103251
11104251
11104252
10104251
19101251
18101251
HWS SOLAR DIVERTER PCB & INSULATING PANELS
SSB SHORTWAVE RECEIVER PCB SET
↳ FRONT PANEL (BLACK)
433MHz RECEIVER
JUN25
JUN25
JUN25
JUN25
18110241
$20.00
CSE250202-3 $15.00
CSE250204 $7.50
15103252
$2.50
NEW PCBs
Australia's electronics magazine
Price
$5.00
$2.50
$5.00
$2.50
$2.50
$20.00
$20.00
$7.50
$15.00
$10.00
$5.00
$10.00
$2.50
$5.00
$10.00
$2.50
$2.50
$2.50
$2.50
$5.00
$5.00
$15.00
$10.00
$12.50
$2.50
$2.50
$10.00
$10.00
$10.00
$5.00
$5.00
$7.50
$5.00
$2.50
$2.50
$2.50
$7.50
$7.50
$5.00
$15.00
$5.00
$10.00
$7.50
$5.00
$5.00
$2.50
$2.50
$5.00
$2.50
$2.50
$2.50
$2.50
$5.00
$5.00
$5.00
$2.50
$10.00
$5.00
$5.00
$5.00
$10.00
$2.50
$2.50
$5.00
$7.50
$5.00
$15.00
$2.50
siliconchip.com.au
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Australia's electronics magazine
June 2025 85
CIRCUIT NOTEBOOK
Interesting circuit ideas which we have checked but not built and tested. Contributions will be paid for at
standard rates. All submissions should include full name, address & phone number.
Detecting smokers using a MaixCam board
Smoking is prohibited in many
places but that doesn’t stop some people. This project uses AI and a camera
to catch people smoking where they
shouldn’t. It can sound an alarm or
even record a photo of the offender.
The MaixCam’s camera captures a
320×240 pixel image in 24-bit RGB format. This image is processed using a
Python script, which runs the YOLOv5
model to analyse the frame and look
for a burning cigarette. The pre-trained
model will not detect just smoke; a
cigarette must be visible for a positive detection.
On detection of a smoker, the
GPIO15 pin is brought high, switching
on an LED indicator and/or sounding a
buzzer. A 120×120 pixel snapshot will
be saved on as /snapshot/snapshot.jpg
When no smoker is detected,
GPIO16 is high, lighting a green LED.
AI processing requires computing
power. The Sipeed microcontroller
on the MaixCam board has a dual-core
CPU with two RISC-V C906/ARM A53
cores running at 1GHz & 700MHz, plus
a 1TOPS<at>INT8 NPU, 256MB of RAM,
a TFT touchscreen, SD card interface,
microphone, 5MP camera and WiFi. It
is just good enough to run the smoker-
detection model and costs around
US$50 (~$80).
The MaixCam runs a lightweight
Linux-based operating system that
supports YOLOv5 to YOLOv8, with
Python 3.11 for scripting and automation. It is a great choice for entrylevel AI projects or lightweight edge
AI systems. MaixCam has a Pro version
86
Silicon Chip
which has a ~3 TOPs NPU and is capable of more demanding tasks.
Running the same computing load
on a Raspberry Pi 5 (8GB) requires
additional components like a TFT
display, keyboard, and a power supply capable of delivering at least 3A <at>
5V, significantly increasing the overall cost.
As evidence, the device will take a
snapshot of the smoker and will save
it to the SD card along with its metadata: the date & time, detection confidence level and bounding box. The
date & time is printed on the image
itself (the code can be modified to add
the others as well).
To get started, download the latest MaixCam operating system from
https://github.com/sipeed/MaixPy/
releases
In most cases, the board you purchased will already have an operating
system installed. If so, you only need
to connect it to your computer. There
are three main ways to connect the
board to your computer: USB direct
connection, though SSH or using the
Maixvision IDE (https://wiki.sipeed.
com/maixvision).
You can SSH directly to the MaixCam’s command prompt using a program like PuTTY. The user name is
“root” and you will need to get the
device’s IP address from your router.
The password will also be “root”.
Once you’ve confirmed you can
access it, use scp (eg, PuTTY’s pscp
command) to copy the required files
to the board: smoking.mud, smoking.
cvimodel and smoke_detection_snapshot_metadata.py. You can get them
from our website at siliconchip.au/
Shop/6/1847
The files smoking.mud & smoking.
cvimodel need to be copied into the
/root/models/ directory on the MaixCam (that’s where the Python code
expects them to be).
Alternatively, you can install the
MaixVision IDE onto your computer
and then upload the files using that. On
the right side of MaixVision IDE, you
Australia's electronics magazine
will find the “Device file manager”.
Select the drive where you want to
upload and then simply press the button. Never try to upload anything into
the “/boot” directory of the device; it
may brick the operating system.
Running the code from MaixVision
IDE is pretty simple. Just get the MaixCam connected to your WiFi. Connect
the MaixCam by pressing the ‘connect’
icon on the bottom left and then press
the ‘play’ button on the bottom left
side. The code will then start running.
To get the code to run at boot time,
find the ‘Package’ button at the bottom
left of the MaixVision IDE and make
a package of your code. Provide all
the data like ID, name, version, developer, description etc. Then submit and
finally install it.
This will create a link in the /maixapp/apps/app.info file with your name
and a folder named “smoker_detection” inside /maixapp/apps/ which
will have three files, one of them being
main.py (which is your Python code).
Now in the /maixapp/auto_start.txt
file, just enter your program name and
save the file. This file should not have
any other entry. You can also do this in
the MaixCam’s touchscreen interface
after installing your code, via Settings
→ Start-menu → smoker_detection.
Now restart the board and smoker_
detection will be auto start.
Once you have it up and running,
you might consider coming up with a
way to send an email or SMS when a
smoker is detected.
Bera Somnath,
Kolkata, India ($100).
siliconchip.com.au
Non-contact diagnostic tool detects electromagnetic fields (EMFs)
This circuit picks up magnetic/
electric fields in the frequency range
of 1Hz to 1MHz and converts them to
an audible signal.
I have been using this circuit (and
its variations) for the last 20 years
for diagnosing and repairing switchmode power supplies and basically
any electronic device that graces my
workbench.
It usually allows one to pinpoint the
fault in the device, sometimes even
without opening the housing! It also
is quite educational, and is a must for
teaching institutions to obtain an intuitive understanding of electronics. It
has certainly saved me hours of troubleshooting.
Inductor L1 picks up the EMI field.
It is a type that is frequently found
in switch-mode power supplies, so
you should be able to obtain it from
a dud one.
The signal is then amplified by op
amp IC1, with its gain set by trimpot
or potentiometer VR1.
For signals in the audible range
(eg, 50Hz to 10kHz), the output of
IC1 is fed to a set of earphones via a
22kW resistor. Higher-frequency signals pass to the CD4518 divider chip,
which reduces the frequency by factors of 10 and 100. Both of its outputs
are mixed back into the signal sent to
the earphones.
The result is you can hear impulses
from 50Hz to 10kHz (÷1), 10kHz to
100kHz (÷10) and 100kHz to 1MHz
(÷100). 50Hz fields sound like a slow
clicking, while 15kHz sounds like a
distorted 150Hz tone.
I have used it on many appliances
and have shown schoolkids what
electromagnetic radiation sounds
like. You can even use a stereo version (eg, with an LF353 op amp) to
help home in on the signals (or lack
thereof).
My enhanced version has 10kW
volume controls and a three-way
switch for ×1, ×10, and ×100 gain
ranges. Knowledgeable readers could
no doubt create their own variations.
Other op amps could be used for IC1,
like the ua741, CA3140 or TL071.
Dr George A Davidson,
Larnook, NSW. ($80)
3D-printed case for Advanced SMD Test Tweezers
I have recently built Advanced
SMD Test Tweezers (February/March
2023; siliconchip.au/Series/396)
from the kit you sell and made a 3D
printable enclosure for it. I’m new to
3D printing and modelling; I got my
first BambuLab A1 mini and started
learning Fusion 360 about a month
ago. Still, it has worked out nicely.
I have included photos of my
printed enclosure and lid for it. I
printed it with PLA Metal filament.
The lid slides in/out into the top
part, which makes it easy to access
the battery for replacement. The
enclosure top has two pins to hold
the screen in place and accommodates 3D-printed buttons, making it
much easier to control the device.
The STL files can be downloaded
from siliconchip.au/Shop/11/584
I printed the enclosure parts
together but the buttons separately
to have a nice concentric finish.
Vitali Bobrov,
Wysoka, Poland. ($70)
siliconchip.com.au
This 3D-printed case for the
Advanced SMD Test Tweezers is
made from a top, lid and three
button extensions.
Australia's electronics magazine
June 2025 87
SERVICEMAN’S LOG
Another mixed bag of bits and bobs
Dave Thompson recently surprised us by visiting Australia. It was such
a surprise, we didn’t know he was here! Having recharged his batteries,
he’ll be back in July. So, for now, here are some stories from our readers.
Mystery amplifier toroidal transformer replacement
The mains light-bulb limiter is not a new idea, but not
everyone is aware of it. My version is the simplest, comprising a 100W 230V incandescent lamp (these are getting
scarce) mounted in a batten holder screwed to the wall
above my bench. This is wired with a piece of two-core
mains flex to a PDL40A Interrupted Phase Tapon Plug.
This means that any appliance plugged into the Tapon
has the lamp in series with its live connection. I leave the
Tapon plugged into one outlet of a power board, and I can
choose to plug the appliance under test either directly to
the mains or via the Tapon. I use an inexpensive power
meter to measure the mains voltage and the current
drawn by the test load.
Turning to the repair in question, a PA speaker had
blown its mains fuse, so after fitting a replacement, I
plugged it in via the lamp limiter. I expected to see the
lamp briefly lighting brightly, then fading to a dim glow.
This is because the amplifier main capacitors charge
when power is first applied, drawing a large initial current, which then subsides.
However, the lamp lit up at full brightness and stayed
that way. If I had plugged it straight into the mains, it
would have likely blown another fuse. There must have
been a heavy short circuit somewhere in the amplifier.
I dismantled the amplifier module from the cabinet and
noted a large toroidal power transformer at one end. The
secondary wires were easily identified and fitted with
Faston connectors, allowing me to quickly disconnect
them. When I plugged it back into the Tapon, the lamp
immediately lit at full brightness again.
That indicated the transformer was the likely culprit,
but to be sure, I disconnected the transformer primary
and tried again.
This time, the lamp didn’t light at all. So a new transformer was required, but it had no markings on it to tell
me what the secondary voltages should be. A label on
the back panel told me the total power consumption was
160VA, so I needed a 160VA transformer with a 230V
The original transformer
(above) and replacement
(below).
88
Silicon Chip
Australia's electronics magazine
siliconchip.com.au
primary and a centre-tapped secondary of unknown
voltage.
I had a schematic of this unit, but there was no mention of the transformer voltage. However, someone had
written 35V next to the DC rails. That seemed a little
high to me, so I looked at the main capacitors on those
rails and found they were only rated at 35V. The actual
rail voltage would be less than that.
The amplifier uses LM3886 power amplifier ICs, so I
consulted the datasheet. This gives different rail voltages for 8W or 4W loads. The woofer was a 4W unit, and
the datasheet said the rail voltages should be ±28V. That
would suggest the transformer secondaries should be
roughly 20V AC.
A look at the selection of 160VA toroidal power transformers available from my regular suppliers showed two
contenders: 18-0-18V or 22-0-22V AC.
From experience, I know that a transformer rated at 18V
will deliver closer to 20V with a light load because it is
designed to deliver 18V at its full rated load. I selected
the 18V unit and, when it arrived, I was surprised to find
it was somewhat larger than the original. I fitted it to the
chassis with a bit of fettling and wired it up.
When I applied power again, all was well and the DC
rail voltages measured a touch over 28V DC.
I should mention that the light-bulb limiter can give
tricky results with appliances with switch-mode power
supplies. Most are OK, but some can draw a lot of current at startup, lighting the lamp and lowering the voltage
to the power supply, which may subsequently not start.
Not long after that repair came another, this time a
wedge floor monitor made by the same manufacturer
and using similar technology. Only this time, the woofer
amplifier was a discrete design with a higher power output. The customer said there was a crack sound, and the
HF horn stopped working.
I initially powered the box through my light-bulb limiter; again, the lamp came on at almost full brightness
Items Covered This Month
• Mystery amplifier transformer replacement
• A curious remote control problem
• HP 8660D signal generator repair
• Arlec NL0009 LED Night Light repair
Dave Thompson runs PC Anytime in Christchurch, NZ.
Website: www.pcanytime.co.nz
Email: dave<at>pcanytime.co.nz
Cartoonist – Louis Decrevel
Website: loueee.com
and stayed that way. The customer said it was still working, so I held my breath and plugged it directly into the
mains. It came on and, as described, the woofer was
working but not the horn.
A quick resistance check of the horn driver revealed
it was open-circuit. Connecting my ‘scope to the output
of the horn amplifier explained why. There was a solid
-30V across the horn, meaning the IC amplifier driving
it had failed and had taken the horn with it. If I had just
replaced the horn driver, the new one would have burnt
out at switch on.
After replacing the IC (LM3886), I tried again with the
light-bulb limiter, and this time the bulb came on bright
and then faded to a dim glow as expected. This suggests
that the faulty IC was also drawing a lot of current; I
think if it was powered up for any length of time, there
would have been smoke.
Paul Mallon, Christchurch, New Zealand.
A curious remote control problem
I had noticed that our air conditioner remote control was working poorly. It would control the AC, but it
seemed less sensitive, and the AC unit did not display
the set temperature. I have a separate control for each
room, so tried another one with no better result.
That evening, I also found that the LG TV was responding strangely. I changed the batteries in the remote and
even tried a second one with no change.
The next morning, I tried using the sound system with
a new (replacement) remote control. This was also acting strangely; since the batteries were low, I replaced
them. I then had the bright idea of checking the sound
system remote itself and found that it was continuously
transmitting.
Opening it and carefully reseating all the buttons
stopped that, and now everything else worked properly.
So, although the controller was transmitting codes not
recognised by the AC and TV, it was enough to interfere
with both systems.
Graham P. Jackman, Melbourne, Vic.
HP 8660D signal generator repair
I went out to the radio shack intending to check some
VHF receivers using my Hewlett-Packard 8660D signal
generator. However, my effort was short-lived – the sig
gen didn’t want to produce any useful output.
Of course, the HP that built this sig gen is very different from the HP we know today as an IT company. The
test and measurement arm of HP that created the 8660D
siliconchip.com.au
Australia's electronics magazine
June 2025 89
was spun off from the IT company many years ago and
became Agilent, later renamed to Keysight.
When it was released in 1971, the 8660 was truly
‘bleeding edge’; it was the first fully synthesised sig gen
built by HP. Although HP built frequency synthesisers
before the 8660, they lacked the modulation capability
and a wide range of calibrated output levels.
The 8660’s specifications were impressive. In its early
form, it offered 0.01MHz to 110MHz in 1Hz steps, AM or
FM modulation, and an output from +10dBm to below
-140dBm. Its output was also clean, with all in-band
unwanted (spurious) outputs at least 80dB below the
level of the wanted frequency; a real achievement. Truly
impressive for the time!
Add two front-panel plugin bays for a modulation section (with various options available) and the output section (again, different modules available) and it was a very
flexible design. It also had an internal plug-in bay for a
“Frequency Extension Module”, which was required for
the later 1300MHz and 2600MHz versions.
The one specification that was a bit below par was
phase noise; the analog HP 8640B signal generator stayed
king of the phase noise heap for many years after the
8660 was released. Phase noise is the wideband noise
created by all oscillators, with some designs much better than others. Still, the 8660 was still very usable for
most purposes.
All of this did not come cheap or small. Despite being
designed in the early 1970s, the 8660D was still on sale
in 1990. The list price in 1990, for the 2.6GHz version
with plugins, would not leave you with much change
from US$40,000. But you got a lot of hardware for your
money – a 4U (about 175mm) high 19 inch rack-mount
box over 500mm deep and weighing about 30 kg.
So, when I switched it on and no signal appeared, what
to do next? My first check was with a spectrum analyser
and frequency counter, which confirmed that with the
8660 set to a nominal frequency in the VHF range, it had
an unstable (frequency varying) output at a few MHz.
Fortunately, HP instruments came with excellent documentation, usually including an operations and service
manual with full schematics, part layouts, fault-finding
guides and parts lists down to individual components.
Scanned versions are often available online.
One useful source of info on the higher-end HP equipment is the Hewlett Packard Journal. Although essentially a sales strategy, the HPJ often had articles written
by the project development teams about the high-end
new equipment they had developed. For the 8660, the
March 1971 and December 1971 HPJ issues both had very
useful information, one about the 8660 mainframe, the
other about the plugins.
There are two basic fault-finding options in a complex
system such as this, where no functional block stands out
as the most likely to create the problem. One is to start
near the signal source and work through the instrument
to locate where the correct signal disappears, or work
backwards from the output and find where the fault stops.
Starting at the source was not attractive. It is a 100MHz
master oscillator which is phase-locked to a reference
oscillator at 5MHz or 10MHz, which can be either internal
or external.
Many different signals are derived from the master
90
Silicon Chip
oscillator by frequency division or multiplication, to
provide the reference signals for the phase-lock loops –
7 PLLs in the mainframe, plus several more in the Frequency Extension Module and in the output plugin. That
means a lot of signal paths to check, including several
complex programmable frequency dividers.
Starting at the output and working back looked a lot
easier. The output plugin module receives only two signals from the Frequency Extension Module: one tuning
from 2.750GHz to 3.950GHz in 100MHz steps, the other
tuning from 3.950GHz to 4.050GHz in 1Hz steps. The
desired output frequency is the difference between these.
A fault found here on one signal would immediately
provide a path to further investigation ‘upstream’.
Although a service manual is available for the output
plugin, there is none online for the Frequency Extension
Module, and in any case, the Frequency Extension Module is basically impossible to test without special (and
unavailable – of course!) ‘extender’ cables. If the fault
was in one of these modules, the instrument was probably
a write off. So, trace backwards from the output it was.
I just needed to locate the relevant connections and
check with a spectrum analyser to see if the expected
signals were there. The instrument is a maze of cable
looms carrying various signals; most of the cables are
terminated with special-purpose plugin connectors that
have both coaxial and standard connections – which are
inaccessible with modules installed in the chassis. Sigh!
As it happened, the two required signals were actually
on SMB connectors, so it was only a few minutes to make
a suitable adaptor cable and have a look with the spectrum analyser. Lo and behold – one signal was absent.
So, the fault was probably not in the output plugin module – so that was one critical module cleared.
The Frequency Extension Module has four RF signals feeding into it, all via a multi-way connector. After
a bit of fiddling, I was able to make a cable that kind-of
mated with the coax connectors in the multi-way plug,
with the Frequency Extension Module unplugged (and
hence inoperable). Another test with the speccy showed
the reference signals to the Frequency Extension Module were not present.
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So the Frequency Extension Module was probably
OK, too. Big sigh of relief! Now I had a new place to
look – the circuits that generate the reference frequency
signals used by all the phase-locked loops.
The 100MHz master oscillator is used to generate
500MHz, 100MHz, two 20MHz, two 10MHz, 2MHz,
400kHz, and 100kHz reference signals. These are easy
to check in what’s called the A4 assembly, which has all
the circuitry to generate the reference signals.
Most, but not all, reference frequencies were MIA, so at
least the master oscillator was operating, but the circuits
to generate most of the reference frequencies weren’t.
Then I spotted some greenish corrosion on a small area
of the “A4A4 reference loop and dividers” circuit board.
Closer inspection showed that an electrolytic capacitor
used as a bypass on the -10V power rail had leaked onto
the board and the electrolyte had eaten a couple of power
supply tracks. Bingo!
After that, it was easy. Clean up the board, replace the
missing tracks with copper wire bridges, a new capacitor, and we were in business. Or so it seemed.
As a final check, I hooked up the sig gen output to my
frequency counter, which is locked to a GPS reference.
That showed the sig gen was putting out a signal significantly low in frequency, which drifted in frequency as
I watched. Bother! Was there another fault with one of
the phase-lock loops?
Then the penny dropped – the sig gen was using its
internal reference, an ovenised crystal oscillator, very
likely the venerable HP 10544A or something similar.
This was drifting low in frequency as it came up to temperature during its warm-up phase before settling to
something very close to the correct frequency.
Previously, I had always used the sig gen with an
external reference from a GPS-derived 10MHz frequency
source, so I never saw this behaviour. So, with relief, I
decided it was all good!
John Morrissey, Traralgon South, Vic.
Arlec NL0009 LED Night Light repair
We have two separate car garages and, a few years ago,
we decided that a motion sensing night light in each
garage would be ideal to help find our way to the light
switch or door when we come home at night. So we purchased plug-in Arlec NL0009 PIR motion sensing LED
night lights from the local hardware store and installed
one in each garage.
These are low-cost plug-in devices and worked very
well until a year or so ago, when the first one became
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Australia's electronics magazine
June 2025 91
faulty. It was still functioning, but the light output had
become very dim, so I accepted the challenge to see if it
was easily repairable at minimal cost. These units come
apart easily with the removal of four small Phillips-head
self-tapping screws to reveal the PCB.
My first thought was it could be a problem on the supply side from the incoming 230V AC to the electronics.
I could not find a circuit diagram for these units, but
inspection of the PCB showed the power supply to be
fairly conventional.
This consisted of a 330nF 275V AC rated X2 capacitor paralleled by a 390kW resistor and connected in
series with a 47W resistor (on the underside of the PCB)
between the incoming 230V AC supply and a bridge rectifier, BD1. Across the DC output side of this rectifier is
SMD capacitor C14, plus C15, a 220uF 35V electrolytic
(on the underside) and a SOD-80 type zener diode, ZD1.
This provides a voltage-limited, filtered and regulated
DC supply to power the night light electronics and the
white high brightness LED lights.
I first checked the 330nF X2 capacitor as I recalled one
failure mode of these metallised film ‘safety’ capacitors
is to lose capacitance over time due to internal partial
discharges, which progressively degrade the metallised
film.
I measured the capacitance of the X2 capacitor with
my DMM and found this to be about 230nF. This was
significantly below its labelled value, and would certainly explain the diminished light output from the
unit. I replaced this faulty component with a new
330nF X2 275V AC capacitor and its full light output
was restored.
About six months later, the second night light failed,
but this time with no light output at all. I opened up the
unit and firstly checked the 330nF X2 capacitor, finding
its capacitance to be about 320nF, which was acceptable.
I next used my current-limited DC bench supply to
apply voltage on the AC (input) side of BD1, checking
both polarities. Voltage measurements indicated about
1.6V across the bridge input, for either polarity, before
a significant current draw started. This seemed to be
indicating a short circuit somewhere on the output side
of the bridge rectifier; 1.6V is approximately equivalent
to the sum of two forward-biased diode voltage drops
in the bridge.
Zener diode ZD1 seemed to be the most likely culprit, followed by the two DC filter capacitors. I removed
ZD1 from the PCB and, on testing, I found it to be pretty
much a dead short circuit. Assuming the zener diode to
be the only faulty component, the next challenge was
determining what voltage it should be.
The zener had what appeared to be one green band
with no other markings. A quick online search was of
little help, so with no zener in the circuit and the light
sensing photodiode (photo 1) shaded with a small piece
of black tape, I decided to apply a current-limited DC
voltage to the output side of the bridge rectifier.
I slowly increased the voltage while moving my hand
over the PIR sensor, and at about 22V, the LEDs started
to glow. Further increasing the voltage to about 28-30V
resulted in a LED brightness level of about what I thought
it should be.
As a further check, I decided to test, in a similar way,
the previously repaired Arlec unit from the other garage.
This unit still had the original zener diode installed and
showed the voltage developed across the zener to be
about 30V, so that was good confirmation.
As I didn’t have a SOD-80 type 30V zener diode on
hand, I decided to try two series-connected DO-41 zeners of 13-15V, hoping this would be good enough. These
diodes were easily installed sitting just above rectifier
BD1, and the repair proved to be very successful.
While I was at it, I decided to also replace the original
X2 capacitor just in case it was heading the same way as
the original X2 capacitor in the other unit.
So, with a little effort and replacement of a few lowcost components, both night lights are continuing to provide their helping glow when we come home at night.
SC
Stephen Denholm, Tranmere, Tas.
One of the
repaired night
lights.
92
Silicon Chip
Australia's electronics magazine
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The replacement
grey 330nF X2
capacitor is much
larger than the
original but it
still fits.
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Australia's electronics magazine
June 2025 93
Vintage Radio
Building a 1970s Little General
By Fred Lever
The Little General is
a classic superhet
AM radio design
published in the
April 1940 issue
of Radio & Hobbies
magazine. Some
time ago, I built one
using parts that were
available in 1946, but
I decided to see what
improvements could be
made using parts from
the 1970s.
M
y classic post-war styled (1946)
Little General, shown in Photo
1, used octal valves and contemporary parts. The set was quite heavy
and bulky by today’s standards at
280 × 200 × 200mm and 5kg, but for
1946, that was typical of what a radio
enthusiast could achieve. By 1976,
30 years later, electronics and components had greatly advanced due to
the advent of TV.
So I decided to build a new Little
General using valves and parts that
were available in 1976.
For inspiration, I went through
my valve box and, out of dozens of
TV types, found a 6CS6 pentagrid,
a 6EH7 frame grid pentode and a
6DX8 triode/pentode output valve.
All were new old stock (NOS), still
in their original boxes. With a twogang mini condenser, a suitable aerial
coil and an oscillator coil, the 6CS6
could be the tuner/converter and the
6EH7 could be used as an IF amplification stage.
That IF signal would then be applied
to a diode and filter to demodulate the
94
Silicon Chip
AM and eliminate the remaining RF
signal. As the 6DX8 is a triode/pentode, I could use the triode section as
a diode and the pentode as the audio
amplifier.
To keep things compact, four of the
new (in 1976) silicon diodes can work
as a bridge rectifier in the power supply in place of a 6V4 valve rectifier.
That eases the heater draw and allows
a simpler transformer with just two
secondary windings.
The resulting set (see the lead
photo) measures 230 × 150 × 140mm
and weighs approximately 2kg, so it
is much more compact than my 1946
style model, at 4.8L versus 11.2L. The
more modern miniature valves draw
much less power, reducing the size of
the required power supply. Parts like
IF transformers and valves are about
¼ of the size of the 1946 version. The
performance is similar.
had several types of mini intermediate-
frequency transformers (IFTs) to
choose from. However, I was short
aerial and oscillator coils. Still, I had
a box full of assorted unknown coils
to go through at a later stage.
I wanted to settle the size of the
transformers first as they are the biggest parts on the chassis and affect
the layout more than the small pieces.
Using three valves, I needed 1.3A at
Design process
I will now go through the design
process. Having selected the valves, a
look through the junk boxes showed I
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Photo 1: this 1940s-style Little General
radio I built earlier works well, but it’s
hardly compact and fairly hefty at 5kg.
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Photo 3: I placed the components on the chassis to get a
rough layout, marked the locations, drilled and cut the
holes and then painted it. Here it is ready to start having
parts mounted to it.
6.3V for the heaters and about 30mA
at 250V for the plates. That works out
to about 16W, so a 20W transformer
would be suitable. I had a discarded
soldering iron transformer specified
as “22 watts” on the sticker.
I dismantled the transformer, leaving the mains primary winding on the
bobbin. I replaced the soldering iron’s
30V secondary with a 6.3V winding
for the heaters and a 240V winding
for the HT. I then restacked the transformer, tested it with dummy loads
and finally, varnished it.
I had a Jaycar AS3025 90 × 50mm 8W
general-purpose rectangular speaker
on hand, so I decided to use that for
the radio.
The speaker transformer needed
to reflect the 8W impedance of the
loudspeaker to a higher value for
the plate of the 6DX8. I had a Jaycar
MM2006 2W 12V mains transformer
Photo 2: the aerial coil (left) and
oscillator coil (right) look a bit messy,
but they tune over the required ranges.
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Photo 4: I riveted the valve sockets and mains transformer
to the chassis. Most other components were mounted less
permanently later, via bolts or on tag strips.
that I wired to a 6DX8 in a bench test
circuit configured as a class-A audio
amplifier to see how it performed. The
transformer did an OK job of passing
a couple of watts from the valve to
the speaker.
The impedance of the primary circuit, at maximum power transfer,
was around 12kW. I dismantled the
transformer, stripped off the original
tapped secondary and wound back
on a single secondary with a turns
ratio that matched the 8W speaker to
12kW. I reassembled the transformer
with a slight air gap in the lamination
stack, tested it again, then dunked it
in varnish.
Tuning coils
The mixer stage needed tuning and
oscillator coils that would give a continuous frequency differential matching the intermediate frequency (IF)
while adjusting the tuning gang. For
example, if the tuning coil tuned from
500kHz to 1700kHz over the full rotation of the tuning gang, the oscillator
coil would need to tune from 955kHz
to 2155kHz, ie, 455kHz above the tuning coil (assuming a 455kHz IF).
Both coils needed to be adjustable,
with ferrite cores, and inductances to
suit the broadcast tuning range. Note
that the required ratio on the tuning
coil is about 3:1, while it’s closer to
2:1 for the oscillator coil.
The mini gang I intended to use had
equal aerial and oscillator capacitance
sections. That means series ‘padding’
of the oscillator gang capacitance is
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needed to compress the oscillator
range from 3:1 to 2:1.
I scratched about in my coil junk
box and found nothing that looked
like an oscillator coil, but I did locate
a rough-looking complete ferrite core
coil on a ½” (12.7mm) tube with a
tuning winding and a small primary.
I measured the inductances as 0.1mH
for the big coil and 0.01mH for the
other.
When I hooked it to the gang and
tested for resonance, I found it tuned
from 600kHz to 1800kHz, and screwing the core in and out made a big difference to the range. That was good
enough for the aerial coil.
For the oscillator coil, I had a spare
blank portion of a ¼” (6.35mm) IFT
former left over from previous projects,
so I wound on about 250 turns of scrap
Litz wire and measured its inductance
as 0.08mH. I added a 30-turn tickler
coil of 0.01mH. I tested its resonance
and, with 150pF in series with the
coil, I had a tuning range of 950kHz
to 2300kHz that also varied a fair bit
by moving the slug in and out.
Those two coils were good enough
to start testing.
I found a pair of mini IF cans marked
“L128” and checked their resonance.
Both coils resonated at around 440kHz
with measurements of 1.43mH and
23W. The four adjusting cores worked
on both, so they looked good to go.
Building the set
I dropped the parts gathered so far
onto a sheet of paper and outlined a
June 2025 95
Photos 5 & 6: these photos show the underside of the chassis (left) and top (right) partway through construction. Most of
the larger parts are in place, with the smaller components and wiring to do.
likely layout. That layout provided
a template for the chassis. The chassis is so small that some light gauge
sheet (from a computer case) sufficed. I centre-punched the holes and
used drills and hole saws to make
the cutouts.
I made a few adjustments, like slotting the control spindle holes so I
could drop those parts in and out easily. I sprayed a light undercoat on the
inside and a light coat of white paint
on the outside, giving the result shown
in Photo 3.
I then started mounting parts on the
chassis, pop riveting some parts permanently into place, like the valve
sockets and tag strips, as shown in
Photo 4.
Next, I mounted the heavy parts,
followed by lighter parts like the coils
and gang. I mounted the tuning gang
using some spacers to lift the shaft to
the centre height of the speaker. I left
the actual dial drum for later and used
a large knob to move the gang spindle
temporarily.
I also bolted a pot shaft to the chassis for a string drive. That shaft bush
and nut were later secured to a strip
of Bakelite on which the tuning coils
were mounted. I made access holes in
the chassis front panel for the slugs of
the tuning coils.
I fitted some tag strips underneath
and squeezed another tag strip on the
top of the chassis behind the speaker.
On that, I mounted the filter capacitors and three 4.7kW PW5 ceramic
resistors in parallel for ~1.5kW total
to use in the HT filter. I pushed the
resistors hard up against the transformer as a heat sink.
Underneath, I mounted a small MB4
bridge rectifier on a tag strip and wired
the HT through the filters to the 6DX8.
I then completed the mains and the
heater wiring to the sockets. It was time
to power it up and road test the 6DX8
with the new power supply.
The audio stage
Having completed the power supply
and 6DX8 wiring, I increased the AC
input voltage in small steps using a
variac to reform the electrolytic capacitors. Nothing smoked, and I measured 313V DC at the rectifier output
and 6.6V AC on the heaters. The three
4.7kW 5W HT dropper resistors lowered the 313V DC to 284V DC.
I had wired the 6DX8 with a 330W
bias resistor, keeping in mind the
plate rating of 18mA, and measured a
24V drop across the HT resistor and
6V bias, both indicating about 20mA
being drawn. The audio stage tested
OK with an input sensitivity of 0.5V
for clipping and no audible hum.
The IF stage
I wired in the 6EH7 and 6CS6 and
fluked the oscillator tickler coil phasing, allowing the oscillator to run
immediately. I aimed to prove the IF
part of the circuit first but encountered
Photos 9 & 10: shown adjacent is the set with a temporary
tuning knob, while above is the tuning knob string
arrangment I came up with.
96
Silicon Chip
Australia's electronics magazine
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Photos 7 & 8: the photo on the left shows the initial stage of under-chassis wiring, while on the right I have added and
wired up the smaller components too.
problems feeding a 440kHz IF signal
through the control grid of the 6CS6.
Usually, I just kill the local oscillator and treat the converter as a straight
RF valve to pass the IF signal into the
control grid and through the IF transformer set. In this case, if I shut down
the local oscillator, the 6CS6 valve
would not pass a signal from its control grid to the plate! As soon as I
unblocked the oscillator grid circuit,
the valve would self-bias and work as
an RF amplifier.
However, if I blasted several volts
of 440kHz into the 6CS6 grid, enough
passed through the plate that I could
at least peak the cores. There were
many other problems with making
the IF section work, but suffice it
to say that after a hard struggle, it
worked well.
One important lesson I learned was
that the 6EH7 needs a separate, stable
screen supply, not one shared with
the converter. Also, the 6EH7 is a very
high-gain valve and needs an AGC bias
feedback control on top of a pedestal
of self-bias to work stably at all signal
strengths.
With the IF system working, I had
to adjust the tuning and oscillator
coils so that, with the tuning gang set
anywhere in its range, the oscillator
frequency was 440kHz higher than
the tuned station frequency. The initial oscillator range of 1000kHz to
2700kHz was too high. I left the coil
turns the same but changed the padder capacitor value, added a trimmer
on the gang and varied the coil core
position.
By juggling those three factors, I
achieved the desired range.
The next job was to make the tuning
coil resonate from 500kHz to 1800kHz.
With the core set so that good coupling was achieved from primary to
secondary, I could not get the bottom
frequency under about 650kHz, and
then the top was around 2300kHz,
both too high, indicating insufficient
turns on the coil.
I pulled one lead end off the big
winding, joined some Litz wire and
wound on another 40 turns. I then got
a range of 549kHz to 1890kHz, close
enough to work.
Next, I carefully measured the actual
difference in frequency between the
two coils at multiple points over the
tuning range. My first tests concluded
that the variation was about ±20kHz
around 450kHz over the tuning range.
With a bit more careful adjustment of
the coils, I reduced that error to ±5kHz
– see Fig.1.
As a product of that process, the
mean IF value increased to about
455kHz. I deemed that acceptable, as
the IFTs have a passband broad enough
to encompass the deviation without a
significant loss of coupling.
With those changes, the set started
to act like a real receiver. The volume could be adjusted from zero to
Fig.1: this plot shows the difference in the tuning
and oscillator coil resonances (vertical axis)
as the dial is rotated (horizontal axis). The red
plot is what I found initially, with a variation of
more than ±20kHz from an average of 450kHz.
Some tweaking gave me the blue curve, within
about ±5kHz from 455kHz over most of the range,
resulting in more consistent performance.
siliconchip.com.au
Australia's electronics magazine
June 2025 97
Fig.2 (above): this is my revised version of the Little
General circuit. There are other changes besides the
different valve lineup, such as the volume control
method (attenuation of the audio signal rather
than varying the valve bias) and the oscillator coil
arrangement (tapped rather than two coupled windings).
Fig.3 (below): the original Little General circuit diagram
from Radio & Hobbies, April 1940. You can find all the
changes I made in my circuit by comparing the two.
Still, the overall configuration (number of valves and
purpose) is very similar.
98
Silicon Chip
Australia's electronics magazine
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maximum, and the audio output was
level no matter what station it was
tuned into. At this stage, the circuit,
shown in Fig.2, was pretty much final.
You can compare it to the original Little General circuit, Fig.3.
The AGC voltage was low on a
weak station, around -1V with 4.2V
across the IF valve bias resistor. On
a strong station, the AGC signal measured -12V and the cathode measured
1.5V, indicating that the valve was
throttled, trying to keep a consistent
IF signal level.
However, the set was full of heterodyne whistles! They led me on
another merry chase, trying this and
that with little effect. Having run out
of ideas, I realised that the set, while
very selective, was not that sensitive,
needing a fair length of antenna to
work. I decided to look at that problem first.
Harking back to the 6CS6 not wanting to work as a plain RF amplifier, I
tried another 6CS6 valve. For this test,
I tuned the receiver with the original
valve and settled the RF level so the
AGC was –12V.
I then swapped the valve for a
grubby, well-used XTV chassis 6CS6
(from a different manufacturer), and
as it warmed up, without moving anything else, I was amazed to see the AGC
climb past -12V and settle at -24V!
That was not just double the gain, as
the AGC works up a slope throttling
the 6EH7, but many times the gain.
The AGC system was now working
even better, with the 6EH7 operating
over a huge bias range, drawing 4mA
with no signal and throttling back to
around 0.2mA on 2RPH, with a mean
level of around 2mA on average stations.
The net result was that the audio
level was consistent, irrespective of
the station signal level. Off-station,
the background frying and fizzling
from all the suburb rooftop inverters
comes up, while on-station, the background noise disappears and stations
tune in loudly.
I then realised that the whistle problem was also gone! Thinking about
this later, I suspect the 6CS6 might not
have been the best choice. While it is
a pentagrid, the valve was designed to
be used as a sync pulse separator. A
minor manufacture variation that had
no effect on separator use may have a
large impact when used for another
application like this one.
siliconchip.com.au
Scope 1: testing the
IF response with
a swept sinewave
fed into the radio
reveals that it is
pretty symmetrical
about the ~450kHz
intermediate
frequency.
Scope 2: the signal
from the volume
control pot’s wiper
with a station
tuned in. You can
see the lowerfrequency audio
signal is overlaid
with higherfrequency noise, the
remnant of the IF
(and possibly RF)
signals.
Scope 3: the audio
signal delivered
to the speaker is
cleaner than that
shown in Scope
2, mainly due to
filtering by the 1nF
capacitor across the
speaker coil.
I also tried a second old 6CS6,
which worked just as well as its stablemate. Still, no real conclusion can
be drawn with a sample of just three
valves. I suspect a radio type 6BE6
would be a better choice. Another
possibility is that my NOS 6CS6 was
simply faulty!
Returning to the IF stage
I went back to the IF, swept it, and
Australia's electronics magazine
took some shots of the response. The
sweep response was quite symmetrical on either side of 450kHz, as shown
in Scope 1. Note that this is an ‘active’
response curve as the AGC is working
and limiting the gain. However, the
general response is evident.
When tuned to a station, after the
volume control, I found a signal of
over 120mV peak-to-peak with a fair
amount of RF still present (Scope 2).
June 2025 99
Photos 11 & 12: I turned five-ply
timber on a lathe and routed a
channel around to hold the string.
Note the tension spring on the back of
the dial.
By the time we get through the 6DX8,
and with the help of the top-cut capacitor on the plate, we wind up with a
clean audio signal of around 140V
peak-to-peak at the plate (Scope 3).
Finishing it off
The final chassis is not one of my
neatest jobs and would benefit from
being stripped out and rebuilt, with
some parts moved. Placing an electrolytic capacitor next to a hot output
valve is not the most sensible move.
However, it was good enough to function, and I wanted to press on, finalise
the cabinet and dial and get to the end.
With a tuning knob spindle already
mounted on the chassis, I needed a
drum on the tuning capacitor to couple to the spindle. I had nothing in
the junk box, so I grabbed a flat scrap
of five-ply timber and made a drum
about 80mm in diameter. I machined
a string groove in the centre of the
outer rim.
I had a Jaycar ¼in (6.35mm) bore
hub (Cat YG2784) that matched the
gang shaft and fitted that to the centre of the timber wheel. Next, I drilled
holes to thread the string ends through
the drum from the rim groove. These
short holes emerge at an angle at the
back of the drum. One hole allowed
one end of a string to be anchored to
a wood screw.
The string then goes around the
drum, down to the spindle, two-and-ahalf times around the spindle and back
up to the drum, then down through a
second hole, terminated to a spring to
maintain some tension on the string.
I sketched out a cabinet design
made of plywood with a circular dial
opening and then looked for something to make a dial bezel. What I
needed was something round and
shiny. My eye fell on some tin cans
in the kitchen recycling bin. I put a
can in the lathe and bored the end
out of it. Then I swung the tool post
around and cut the end off, giving me
a ‘chrome’ bezel.
The idea for the cabinet was to have
the front panel recessed from the front
to protect the knobs. Otherwise, it’s a
simple box made from five-ply timber with glue fillet joints and a back
plate with slots to let air in and form
a handle. The dial bezel and a bunch
of ¼in (6.35mm) holes for the speaker
completed the front panel.
The back is then held in with four
screws that go into the chassis blocks
and two top blocks. One of those also
limits the power transformer’s upward
movement.
With the basic box made, I sanded
it down a bit and flowed on a coat of
red stain. I repeated that a couple of
times, with sanding in between, until
I had a reasonably smooth finish. Ultimately, I decided that sticking one’s
fingers into the live works to carry
it was not a good idea, so I carefully
added a flat strap to the top as a proper
carry handle.
Conclusion
It has some flaws, such as parts not
quite lined up straight, rat’s nest wiring
and values that need optimising. These
are properties of prototype radios that
would be ironed out in a production
run. Still, I am not a manufacturer, so
it will do.
As with any other scratch-built project, there was far more work involved
in getting it to work than this article reveals. Much more detail can be
found at the following links (parts 1-3):
• siliconchip.au/link/abtk
• siliconchip.au/link/abtl
SC
• siliconchip.au/link/abtm
Photos 13-15: the last few steps required before assembly involved making the timber cabinet, which I then stained red.
The complete Little General radio was more compact, weighing ~2kg; about half the weight of the radio shown in Photo 1.
100
Silicon Chip
Australia's electronics magazine
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Ceramic capacitor
values measure low
I recently ordered the short-form
Automatic LQ Meter kit (SC6939).
A set of three SMD capacitors was
included, which I assume are the 10μF
parts. However, upon measuring them
with my SMD Test Tweezers (now one
of my most-used tools), I got a reading
of 5μF each. This made me think they
were actually 4.7μF capacitors.
I just used my Peak Atlas LCR, and
it showed 10μF, so I guess they are the
correct types. The SC Test Tweezers
are normally reasonably accurate, so I
didn’t double check. Why are the readings so far off? (M. H., Mordialloc, Vic)
● We were initially puzzled by the
low capacitor readings you describe,
but soon realised that they are mostly
due to a design aspect of the Improved
Test Tweezers and an often overlooked
shortcoming of MLCCs (multi-layer
ceramic capacitors).
Most of the error is because of the
capacitor’s behaviour under DC bias.
The Tweezers work by applying 3V
DC to the device under test (via a
10kW resistor) and probing the junction point. For capacitors, the Tweezers discharge the capacitor, but most
of the time it has close to 3V across it.
Like many MLCCs, the Samsung
CL21A106KOQNNNE 10μF 16V
capacitors we supply in the kit suffer
from a loss of capacitance as the DC
bias voltage rises. At 3V, their capacitance is down by 30%, according to
the chart from Samsung below.
Given that the capacitors have a
+20
0
ΔC(%)
-20
-40
-60
-80
-100
0
5
10
DC bias (V)
siliconchip.com.au
15
±10% initial tolerance, they could
have as little as 6μF capacitance once
charged to 3V (-40%). They will be
down to about 10% of their nominal
capacitance at the rated voltage, 16V!
This is a good reason to use MLCCs
with a higher than necessary voltage rating; they retain more of their capacitance
when charged up. Of course, such capacitors may be larger or more expensive.
We didn’t specify an accuracy for
the Tweezers, but we’d say they have
about ±10% accuracy for capacitance
readings. This is heavily affected by
oscillator accuracy (due to the timing needed for capacitance measurements), which is specified as ±8%.
With the capacitor already possibly
being down to 6μF, and another 10%+
error from the Tweezers, a reading of
5μF (or even lower) is possible.
D1 Mini doesn’t work
with 5GHz WiFi
I constructed the GPS-Synchronised
Analog Clock (September & November 2022; siliconchip.au/Series/391)
with the D1 Mini WiFi module from a
kit supplied by Silicon Chip. It works
well, but I found it was rapidly flattening the two AA cells.
The high drain was happening
because the PIC continually powers
the D1 Mini module until it can connect, and it was failing to connect to
my home’s WiFi, either for long periods each day or at all.
After experimenting and finding
that it would readily connect to several other different WiFi routers, I
noticed that my home’s WiFi router
has both 2.4GHz and 5GHz band networks, with the same SSID and password. I disabled the 5GHz network
and the D1 Mini connected easily to
the 2.4GHz network.
An alternative solution might be to
rename the 5GHz network.
Either way, the ability to have
devices roaming freely between the two
networks is lost. This does not matter to
me, but I wonder if a firmware update
to the D1 Mini is available to fix this
Australia's electronics magazine
problem properly. I can imagine, in a
year or two, switching the 5GHz network back on and forgetting that this
will cause the kitchen clock’s batteries
to quickly go flat! (A. P., Norwood, Tas)
● It’s odd that this affects the D1
Mini, since it has no 5GHz capability. But in my home network, I have
renamed the 5GHz network to use a different SSID because there were one or
two devices that simply did not work
otherwise. I am using a TP-Link router.
Apparently, some dual-band routers try to kick devices off the 2.4GHz
network (using WPA deauthenticate
packets) to see if they reappear on the
5GHz network. If the D1 Mini does not
handle this elegantly, then that could
explain the problem. A note on GitHub
suggests that the ESP8266 WiFi chip
in the D1 Mini may have this problem (see https://github.com/esp8266/
Arduino/issues/8956).
There is mention of forcing the
802.11g protocol, but no indication of
how it can be done; it is not something
we’ve ever seen as being configurable.
Your fix is a good workaround; however, we now have a newer WiFi Time
Source based on the Pico W (June 2023
issue; siliconchip.au/Article/15823).
Programming Adaptor
needs programmer
Is your SC6774 kit all I need to program a PIC16F1459 chip? (P. C., Denistone, NSW)
● The PIC Programming Adaptor is
just an adaptor. You still need a PICkit
or similar programmer to use with
it (see our September 2023 issue for
details; siliconchip.au/Article/15943).
Due to the large number of PICs
available and different programming
protocols, it is not practical for us to
produce an all-in-one programmer.
The PICkits, SNAPs and their clones
are the best way to get that interface.
The PICkit 5 is currently quite
expensive, at around $150. The Microchip Snap (PG164100) is much more
cost effective at around $25. Unfortunately, at the time of writing they are
June 2025 101
out of stock at the likes of DigiKey
and Mouser, but due back in stock by
the time you read this. They are effectively a cut-down version of a PICkit 4
and don’t support powering the target
device or high-voltage programming.
The lack of high-voltage programming may mean they might not be
suitable for some projects, but we
have used a Snap to program the
PIC16F1459. For a $125 saving, we
think we can figure out a way to supply power to the target device!
Dual Hybrid Supply
CPU board problem
I have nearly finished building the
Dual Hybrid Power Supply project (February & March 2022; siliconchip.au/
Series/377). After some initial testing, I
needed to fix up a few incorrectly orientated diodes on the regulator boards.
However, those boards are now functioning as per the testing instructions.
I am now stuck with the control
board. The LD1117 regulator gets
very hot after seconds and the LCD
has no output (other than just the
blue screen). I have checked the orientation of the SMD diodes on the
board and they are OK. I have also
double-checked for solder bridges etc.
I checked that my ribbon cables have
the correct orientation too.
Do you have any suggestions on how
I can continue to trouble shoot? (B. L.,
Maidstone, Vic)
● Phil Prosser responds: the first
step is to unplug everything but power
from the CPU board and check the
current draw. Perhaps an IC has been
installed with the incorrect orientation
or there is a solder bridge you haven’t
found yet. If the power draw is reasonable in that condition, plug in the display and see what happens.
A hot LM1117 is almost certainly a
sign of something being soldered in the
wrong way around. If one of the reverse
diodes was the protection diode for the
regulator, the full input voltage would
have been applied to everything on the
3.3V rail, which could be scary.
Note: B. L. later confirmed there was
a short circuit on the microcontroller
pins causing the excessive current draw.
BIG LED Clock
power supply
The BIG LED Clock (January 2025
issue; siliconchip.au/Article/17603)
102
Silicon Chip
looks great. I have cleared a spot on
my workshop wall and ordered the
major parts, but I can’t see what the
power requirements are. I would have
expected a plugpack or something similar in the materials list.
I also didn’t see if the clock was 12- or
24-hour, or configurable. I presume that
the first digit would need at least six segments for a 24-hour clock. Keep up the
mighty work. (R. W., King Creek, NSW)
● We noted on page 58 of the article
that our BIG Clock peaked at around
700mA with the default brightness setting, and we simply used the USB-C
connector to power it, since USB is
so common. Unlike the older USB
specifications, USB-C supports a minimum of 900mA, so any compliant
USB-C to USB-C cable should provide enough power, no matter what it
is connected to.
We simply ran our prototype from a
computer. You could use a phone charger or other USB-C power adaptor. We
figured that most readers would have
something appropriate in their spare
parts collection. 700mA should be
comfortably within the limits of just
about any USB mains adaptor, since
most support 1A or more.
If you have a supply that can only
provide 500mA, then you could set the
BRIGHTNESS #define to 40.
And yes, the number of segments
available limits the hardware to displaying a 12-hour clock.
Adding a Fetron to a
vintage radio
I have a couple of queries regarding
the Fetrons that Dr Hugo Holden used
to make a communications receiver,
described in March 2021 (siliconchip.
au/Article/14777).
I am restoring a 1935 Atwater Kent
radio (it’s now my own set) and its performance is rather woeful. It was built
as an economy set and performs like
one. I am seriously considering modifying the set to have a proper IF stage
& diode detector, and I wondered if I
could ‘hide’ at least one Fetron somewhere in the set along with fitting a
second IF transformer.
Currently, the radio has one IF
transformer with an extra winding for
regeneration. The ‘2nd detector’ valve
doubles as the detector (using grid
leak detection) and the audio amplifier. While it works, there is significant
distortion. I have recapped the entire
Australia's electronics magazine
radio and replaced most of its resistors.
I have also considered adding a transistor IF stage to the set, but I am unsure
how well it would work. Do you have
any thoughts on this? In a ‘normal’
AM transistor circuit, the IF transformers are tapped to provide impedance
matching as well as IF coupling.
I considered having two transistors
connected as a Darlington pair to provide a high input impedance, with the
collectors of the transistors connected
to a valve radio IF transformer to provide coupling to the detector diode. (P.
W., Pukekohe, New Zealand)
● Dr Hugo Holden responds: you
could eliminate the regeneration of
the existing IF stage and add another
IF stage to get the overall IF gain up,
then use a standard detector. If I were
doing that, I probably wouldn’t use a
Fetron, because they are hard to get.
Still, it would work and would avoid
the need for a heater supply.
A small, easy-to-get seven-pin Pentode tube such as the 6AG5 or similar
and an extra IF transformer would also
work. Suitable heater voltages should
be available in the set. If they were the
wrong voltage, there are some possible solutions.
It could also be done with two
high-voltage transistors. Ideally, it
should probably not be a Darlington
but a cascode design. Otherwise, there
will not be enough input/output isolation and the IF stage could oscillate
(Fetrons are inherently cascoded).
I have used a single JFET in an IF
stage, and it was stable due to the low
feedback capacitance of the MPF102,
but it was a low-voltage circuit. Higher-
voltage JFETs likely would have to be
in cascode, much like the Fetron, to
work with equivalent input/output
isolation to the screen-grid pentode.
To increase the input impedance
of a transistor cascode arrangement,
a third transistor can be used as an
emitter-follower to drive the cascode
circuit. Generally, though, a small
Pentode like a 6AG5 would be easier
if a suitable heater voltage is available. Another option is to use a low
heater voltage valve with heater ballast resistors.
Question on expanding
Multi-Spark CDI
Greetings from New Zealand. I have
been an avid reader since Electronics
continued on page 104
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When working on these projects use extreme care to ensure that you do not accidentally come into contact with mains AC
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Australia's electronics magazine
June 2025 103
Advertising Index
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Blackmagic Design....................... 9
Control Devices........................... 85
Dave Thompson........................ 103
DigiKey Electronics....................... 3
Emona Instruments.................. IBC
Hare & Forbes............................ 6-7
Icom Australia............................. 14
Jaycar........................IFC, 11, 15-17
Keith Rippon Kit Assembly....... 103
Lazer Security........................... 103
LD Electronics........................... 103
LEDsales................................... 103
Microchip Technology.............OBC
Mouser Electronics....................... 4
OurPCB Australia........................ 10
PCBWay....................................... 13
PMD Way................................... 103
Rohde & Schwarz........................ 83
SC Ideal Bridge Rectifiers kits.... 57
SC GPS Clock kit......................... 60
SC Advanced Tweezers kit......... 93
Silicon Chip Shop.......... 69, 82, 84
Silicon Chip Subscriptions........ 30
The Loudspeaker Kit.com.......... 12
Wagner Electronics..................... 91
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104
Silicon Chip
Australia’s demise. I have been involved
in the electronics industry, servicing,
building and importing components
since the days of Mullard’s transistors
(half of which did not function).
I have built a number of circuits
published in Silicon Chip and would
like to congratulate you on your persistence in encouraging young minds
to delve into both analog and digital
electronics. The shrinking size of components will not help, especially for
old guys like me.
I have a question about John’s
Multi-Spark CDI design (December
2014 & January 2015; siliconchip.au/
Series/279). I want to be able to trigger
up to six spark plugs simultaneously
while revving to high RPMs. Rather
than building six complete units,
would the output from the inverter
be sufficient for one inverter to supply
six individual trigger systems? (K. S.,
Dunedin, New Zealand)
● Thank you for your words of
appreciation for Silicon Chip magazine.
Regarding the Multi-Spark ignition,
the coil driver section comprising IC2,
Q3, Q4 and the 1μF capacitor and associated components would need to be
duplicated six times for six separate
ignition coils. The 300V DC generator
comprising IC1, Q1, Q2, T1, the D2-D5
full-wave rectifier and associated components should be able to drive all six
output circuits with the 300V DC.
If the 300V is not maintained with
the six outputs connected and running
at high RPM, you may need to build
another 300V DC section so that each
will only drive three output circuits.
RIAA preamp wanted
for record player
I have been asked to restore an old
1950s chest-type valve radiogram that
has great sentimental significance to its
owner. Unfortunately, the existing Collaro record changer looks to be beyond
help, with perished rubber parts. The
only solution I have is to retrofit a
newer turntable/record changer unit.
I envisage using something like
a later model Garrard obtained second-hand, fitted with a magnetic cartridge. The radiogram won’t have sufficient audio gain to be driven directly
from a magnetic cartridge, but I can
easily add a solid state preamp, hidden inside the cabinet.
Have you published a design for a
mono (or stereo) RIAA magnetic phono
Australia's electronics magazine
preamp that can provide an output of
up to 300-400mV? If so, do you have
PCBs available for it? (P. W., Pukekohe,
New Zealand)
● We have published a Magnetic
Cartridge Preamplifier (August 2006;
siliconchip.au/Article/2740). It is
a stereo preamplifier with a gain
that should be suitable for your
application. Its output level depends
on the cartridge signal output with
record groove modulation. The PCB is
still available from our Online Shop
(siliconchip.au/Shop/?article=2740).
Bouncing Kelvin causes
the eyes to light up
My son and I enjoyed building the
Kelvin the Cricket project (October
2017; siliconchip.au/Article/10828)
and would love to learn more about
two aspects of his design and function.
1. If I bounce Kelvin, his eyes light
up, even with the batteries out and the
jumper removed. I’ve only tried this
on dark rooms because the LED is too
dim to see in well-lit rooms. I’ve tried
leaving Kelvin alone for an hour in case
there was a charged capacitor. I’ve tried
different locations in case there was a
strong magnetic field. Sometimes both
LEDs glow, sometimes one does.
2. Do you have the PIC code in C# or
pretty much any other language other
than assembly, so I can learn how the
functions were implemented? (B. B.,
via email)
● The interesting effect where the
LEDs light when Kelvin is dropped is
due to the piezo transducer producing a voltage when flexed. Since the
transducer is in parallel with the LEDs
and their current limiting resistors,
they light up when this happens, but
for extremely brief periods and very
low currents.
Piezo materials flex when a voltage
is applied (producing a sound) but
they also do the reverse, ie, if flexed
they will produce a voltage. The dropping of Kelvin the Cricket causes piezo
movement when it hits the ground, as
it experiences inertial forces.
The piezo element will probably
ring (oscillate) with the initial abrupt
stop when hitting the ground and
drive the LEDs alternately as the AC
waveform from the transducer changes
polarity on each ringing cycle.
Sorry, we don’t have C source for the
software as it was written in assembly
language.
SC
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