Silicon ChipNew SC200 Audio Amplifier - January 2017 SILICON CHIP
  1. Outer Front Cover
  2. Contents
  3. Publisher's Letter: Pumped hydro storage is no panacea for renewables & Airbags could kill your daughter
  4. Subscriptions
  5. Feature: Pumped Storage Hydroelectricity by Dr David Maddison
  6. PartShop
  7. Feature: Viewing Radio Waves In Colour by Ross Tester
  8. Project: New SC200 Audio Amplifier by Nicholas Vinen & Leo Simpson
  9. Project: High Power DC Motor Speed Control by John Clarke
  10. Serviceman's Log: When spare parts aren't around by Dave Thompson
  11. Project: Programming the ATtiny85 With An Arduino by Lawrence Billson
  12. Product Showcase
  13. Project: El Cheapo Modules From Asia - Part 3 by Jim Rowe
  14. Project: Giving the Ultrasonic Theremin A Volume Control by Bao Smith
  15. Feature: Real-Time System Modelling by Karthik Srinivasan
  16. Feature: Set-Top Boxes Make Great (Cheap!) PVRs by Jim Rowe
  17. Vintage Radio: Pye 1951 5-Valve Model APJ-Modified by Associate Professor Graham Parslow
  18. PartShop
  19. Market Centre
  20. Advertising Index
  21. Outer Back Cover

This is only a preview of the January 2017 issue of Silicon Chip.

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Items relevant to "New SC200 Audio Amplifier":
  • Ultra-LD Mk3/Mk4 Amplifier Power Supply PCB [01109111] (AUD $15.00)
  • New SC200 Audio Amplifier PCB [01108161] (AUD $10.00)
  • Hard-to-get parts for the SC200 Audio Amplifier Module (Component, AUD $50.00)
  • New SC200 Audio Amplifier PCB pattern (PDF download) [01108161] (Free)
Articles in this series:
  • New SC200 Audio Amplifier (January 2017)
  • New SC200 Audio Amplifier (January 2017)
  • New SC200 Audio Amplifier – Part 2 (February 2017)
  • New SC200 Audio Amplifier – Part 2 (February 2017)
  • New SC200 Audio Amplifier - Part 3 (March 2017)
  • New SC200 Audio Amplifier - Part 3 (March 2017)
Items relevant to "High Power DC Motor Speed Control":
  • High Power DC Motor Speed Control main PCB [11112161] (AUD $10.00)
  • High Power DC Motor Speed Control Mosfet PCB [11112162] (AUD $12.50)
  • PIC16F88-I/P programmed for the High Power DC Motor Speed Controller [1111216A.HEX] (Programmed Microcontroller, AUD $15.00)
  • Hard-to-get parts for the High Power DC Motor Speed Controller (Component, AUD $50.00)
  • Firmware (ASM and HEX) files for the High Power DC Motor Speed Control [1111216A.HEX] (Software, Free)
  • High Power DC Motor Speed Control PCB patterns (PDF download) [11112161/2] (Free)
Articles in this series:
  • High Power DC Motor Speed Control (January 2017)
  • High Power DC Motor Speed Control (January 2017)
  • High Power DC Motor Speed Control – Part 2 (February 2017)
  • High Power DC Motor Speed Control – Part 2 (February 2017)
Items relevant to "Programming the ATtiny85 With An Arduino":
  • Firmware (.ino) files for the Programming the ATtiny85 With An Arduino (Software, Free)
Items relevant to "El Cheapo Modules From Asia - Part 3":
  • CP2102-based USB/TTL serial converter with microUSB socket and 6-pin right-angle header (Component, AUD $5.00)
  • CP2102-based USB/TTL serial converter with microUSB socket and 6-pin right-angle header (clone version) (Component, AUD $3.00)
Articles in this series:
  • El Cheapo Modules From Asia - Part 1 (October 2016)
  • El Cheapo Modules From Asia - Part 1 (October 2016)
  • El Cheapo Modules From Asia - Part 2 (December 2016)
  • El Cheapo Modules From Asia - Part 2 (December 2016)
  • El Cheapo Modules From Asia - Part 3 (January 2017)
  • El Cheapo Modules From Asia - Part 3 (January 2017)
  • El Cheapo Modules from Asia - Part 4 (February 2017)
  • El Cheapo Modules from Asia - Part 4 (February 2017)
  • El Cheapo Modules, Part 5: LCD module with I²C (March 2017)
  • El Cheapo Modules, Part 5: LCD module with I²C (March 2017)
  • El Cheapo Modules, Part 6: Direct Digital Synthesiser (April 2017)
  • El Cheapo Modules, Part 6: Direct Digital Synthesiser (April 2017)
  • El Cheapo Modules, Part 7: LED Matrix displays (June 2017)
  • El Cheapo Modules, Part 7: LED Matrix displays (June 2017)
  • El Cheapo Modules: Li-ion & LiPo Chargers (August 2017)
  • El Cheapo Modules: Li-ion & LiPo Chargers (August 2017)
  • El Cheapo modules Part 9: AD9850 DDS module (September 2017)
  • El Cheapo modules Part 9: AD9850 DDS module (September 2017)
  • El Cheapo Modules Part 10: GPS receivers (October 2017)
  • El Cheapo Modules Part 10: GPS receivers (October 2017)
  • El Cheapo Modules 11: Pressure/Temperature Sensors (December 2017)
  • El Cheapo Modules 11: Pressure/Temperature Sensors (December 2017)
  • El Cheapo Modules 12: 2.4GHz Wireless Data Modules (January 2018)
  • El Cheapo Modules 12: 2.4GHz Wireless Data Modules (January 2018)
  • El Cheapo Modules 13: sensing motion and moisture (February 2018)
  • El Cheapo Modules 13: sensing motion and moisture (February 2018)
  • El Cheapo Modules 14: Logarithmic RF Detector (March 2018)
  • El Cheapo Modules 14: Logarithmic RF Detector (March 2018)
  • El Cheapo Modules 16: 35-4400MHz frequency generator (May 2018)
  • El Cheapo Modules 16: 35-4400MHz frequency generator (May 2018)
  • El Cheapo Modules 17: 4GHz digital attenuator (June 2018)
  • El Cheapo Modules 17: 4GHz digital attenuator (June 2018)
  • El Cheapo: 500MHz frequency counter and preamp (July 2018)
  • El Cheapo: 500MHz frequency counter and preamp (July 2018)
  • El Cheapo modules Part 19 – Arduino NFC Shield (September 2018)
  • El Cheapo modules Part 19 – Arduino NFC Shield (September 2018)
  • El cheapo modules, part 20: two tiny compass modules (November 2018)
  • El cheapo modules, part 20: two tiny compass modules (November 2018)
  • El cheapo modules, part 21: stamp-sized audio player (December 2018)
  • El cheapo modules, part 21: stamp-sized audio player (December 2018)
  • El Cheapo Modules 22: Stepper Motor Drivers (February 2019)
  • El Cheapo Modules 22: Stepper Motor Drivers (February 2019)
  • El Cheapo Modules 23: Galvanic Skin Response (March 2019)
  • El Cheapo Modules 23: Galvanic Skin Response (March 2019)
  • El Cheapo Modules: Class D amplifier modules (May 2019)
  • El Cheapo Modules: Class D amplifier modules (May 2019)
  • El Cheapo Modules: Long Range (LoRa) Transceivers (June 2019)
  • El Cheapo Modules: Long Range (LoRa) Transceivers (June 2019)
  • El Cheapo Modules: AD584 Precision Voltage References (July 2019)
  • El Cheapo Modules: AD584 Precision Voltage References (July 2019)
  • Three I-O Expanders to give you more control! (November 2019)
  • Three I-O Expanders to give you more control! (November 2019)
  • El Cheapo modules: “Intelligent” 8x8 RGB LED Matrix (January 2020)
  • El Cheapo modules: “Intelligent” 8x8 RGB LED Matrix (January 2020)
  • El Cheapo modules: 8-channel USB Logic Analyser (February 2020)
  • El Cheapo modules: 8-channel USB Logic Analyser (February 2020)
  • New w-i-d-e-b-a-n-d RTL-SDR modules (May 2020)
  • New w-i-d-e-b-a-n-d RTL-SDR modules (May 2020)
  • New w-i-d-e-b-a-n-d RTL-SDR modules, Part 2 (June 2020)
  • New w-i-d-e-b-a-n-d RTL-SDR modules, Part 2 (June 2020)
  • El Cheapo Modules: Mini Digital Volt/Amp Panel Meters (December 2020)
  • El Cheapo Modules: Mini Digital Volt/Amp Panel Meters (December 2020)
  • El Cheapo Modules: Mini Digital AC Panel Meters (January 2021)
  • El Cheapo Modules: Mini Digital AC Panel Meters (January 2021)
  • El Cheapo Modules: LCR-T4 Digital Multi-Tester (February 2021)
  • El Cheapo Modules: LCR-T4 Digital Multi-Tester (February 2021)
  • El Cheapo Modules: USB-PD chargers (July 2021)
  • El Cheapo Modules: USB-PD chargers (July 2021)
  • El Cheapo Modules: USB-PD Triggers (August 2021)
  • El Cheapo Modules: USB-PD Triggers (August 2021)
  • El Cheapo Modules: 3.8GHz Digital Attenuator (October 2021)
  • El Cheapo Modules: 3.8GHz Digital Attenuator (October 2021)
  • El Cheapo Modules: 6GHz Digital Attenuator (November 2021)
  • El Cheapo Modules: 6GHz Digital Attenuator (November 2021)
  • El Cheapo Modules: 35MHz-4.4GHz Signal Generator (December 2021)
  • El Cheapo Modules: 35MHz-4.4GHz Signal Generator (December 2021)
  • El Cheapo Modules: LTDZ Spectrum Analyser (January 2022)
  • El Cheapo Modules: LTDZ Spectrum Analyser (January 2022)
  • Low-noise HF-UHF Amplifiers (February 2022)
  • Low-noise HF-UHF Amplifiers (February 2022)
  • A Gesture Recognition Module (March 2022)
  • A Gesture Recognition Module (March 2022)
  • Air Quality Sensors (May 2022)
  • Air Quality Sensors (May 2022)
  • MOS Air Quality Sensors (June 2022)
  • MOS Air Quality Sensors (June 2022)
  • PAS CO2 Air Quality Sensor (July 2022)
  • PAS CO2 Air Quality Sensor (July 2022)
  • Particulate Matter (PM) Sensors (November 2022)
  • Particulate Matter (PM) Sensors (November 2022)
  • Heart Rate Sensor Module (February 2023)
  • Heart Rate Sensor Module (February 2023)
  • UVM-30A UV Light Sensor (May 2023)
  • UVM-30A UV Light Sensor (May 2023)
  • VL6180X Rangefinding Module (July 2023)
  • VL6180X Rangefinding Module (July 2023)
  • pH Meter Module (September 2023)
  • pH Meter Module (September 2023)
  • 1.3in Monochrome OLED Display (October 2023)
  • 1.3in Monochrome OLED Display (October 2023)
  • 16-bit precision 4-input ADC (November 2023)
  • 16-bit precision 4-input ADC (November 2023)
  • 1-24V USB Power Supply (October 2024)
  • 1-24V USB Power Supply (October 2024)
  • 14-segment, 4-digit LED Display Modules (November 2024)
  • 0.91-inch OLED Screen (November 2024)
  • 0.91-inch OLED Screen (November 2024)
  • 14-segment, 4-digit LED Display Modules (November 2024)
  • The Quason VL6180X laser rangefinder module (January 2025)
  • TCS230 Colour Sensor (January 2025)
  • The Quason VL6180X laser rangefinder module (January 2025)
  • TCS230 Colour Sensor (January 2025)
  • Using Electronic Modules: 1-24V Adjustable USB Power Supply (February 2025)
  • Using Electronic Modules: 1-24V Adjustable USB Power Supply (February 2025)
Items relevant to "Giving the Ultrasonic Theremin A Volume Control":
  • Firmware (.ino and .c) files for Giving the Ultrasonic Theremin a Volume Control (Software, Free)
Articles in this series:
  • Arduino-Based Digital Theremin (December 2016)
  • Arduino-Based Digital Theremin (December 2016)
  • Giving the Ultrasonic Theremin A Volume Control (January 2017)
  • Giving the Ultrasonic Theremin A Volume Control (January 2017)

Purchase a printed copy of this issue for $10.00.

We make it so easy to Build the SC200... a new, high performance amplifier module By NICHOLAS VINEN and LEO SIMPSON 28  Silicon Chip with hardly an SMD in sight! siliconchip.com.au This completely new amplifier circuit incorporates most of the features of our Ultra-LD Mk4 200W amplifier module but uses easy-to-solder through-hole components. There are no tiny surface mount components. O ver the last 15 years or so, SILICON CHIP has published a number of very popular audio amplifier modules. The first of these was the SC480, described in the January & February 2003 issues. Best described as a work-horse, this amplifier was and still is very easy to assemble and get going, and countless thousands have been have been built. Indeed, you can still purchase kits for these modules from Altronics & Jaycar. The next very popular amplifier module was the 20W Class-A module published in 2007. We billed this as “having the lowest distortion of any amplifier ever published... anywhere in the world!” Very keen audiophiles have built it in large numbers but being Class-A, it does have the normal drawback of being quite inefficient and therefore it dissipates a lot of heat for its modest power output of 20 watts. Finally, the next most notable amplifier module was the Ultra-LD Mk4 design which not only has high output power but its very low harmonic distortion levels challenge even those achieved by the 20W Class-A design. Indeed, the 110W version of the Ultra-LD effectively renders the modestly-powered 20W Class-A design irrelevant. Why would you build that Class-A design when you can build a much more powerful Class-AB design for the same money and with virtually indistinguishable performance? So why are we producing this new SC200 module? Firstly, we have felt that while the SC480 design has been very successful, its distortion and noise performance is pretty mediocre when compared to the latter two designs. In short, it is old-hat and well overdue for a major upgrade. Second, while the Ultra-LD Mk.4 amplifier module is virtually state-of-the-art, it does have the drawback that it uses mainly surface-mount components and while many have been built, it would have been far more popular if it used through-hole components – ones that are much easier to solder! So in designing the SC200 module, we have tried to make it much easier to build and at the same time, produce a module which is far ahead of the SC480 in all aspects of its performance. All the semiconductors on the PCB are con- ventional through-hole components. Also the small-signal transistors are readily available types and while the input pair of transistors won’t give quite the same extremely low noise performance of our previous Ultra-LD Mk.3 & Mk.4 designs, they are cheap and readily available. The other major difference between the new SC200 design and the Ultra-LD Mk.4 is that it does not use the exotic five-lead On Semiconductor “ThermalTrak” NJ3281D/ NJL1302D output transistors which have integral power diodes for quiescent current stabilisation. Instead, this new design uses conventional 3-lead power transistors from Fairchild, types FJA4313 and FJA4213. While the ThermalTrak transistors are largely responsible for the excellent performance of the Ultra-LD amplifiers, they are rather expensive at $8.90 each (current retail price) and that adds up if you’re building a multi-channel amplifier. And unfortunately, as our experience has shown, they never quite delivered on their promise to provide a stable quiescent current over the operating temperature range, without the need for adjustment. We’ll discuss the new output devices more later. Main features The main features of this new module, which we’ve called the SC200, indicative of its 200-watt power output into a 4-ohm load, are very similar to those of the Ultra-LD Mk.4. And while it will replace the work-horse SC480, we would like to think its performance will be very much in the thoroughbred class! It certainly delivers more power than the SC480, for a similar price to build. Those main features are listed in a separate panel but some require additional comment. Apart from exceptional performance, the SC200 has quite a few features which were not thought of when we produced the SC480. These include on-board LEDs which indicate if the power rails are present and which change colour if the DC fuses blow. And there is the clipping indicator circuit which drives a LED to show when the amplifier is being over-driven. This LED can be mounted on the amplifier front panel if desired and can be wired to multiple modules to indicate when any channel is clipping. Or you can simply have a Main features • Easy to build • Uses low cost parts • Low distortion and noise • Compact PCB • Able to produce specified power output on a continuous basis with passive cooling • Onboard DC fuses • Power indicator LEDs • Fuse OK/blown indicator LEDs siliconchip.com.au • Clipping indicator LED • Clean overload recovery with low ringing • Clean square wave response with low ringing • Tolerant of hum & EMI fields • Survives brief short circuits & overload without blowing fuses • Quiescent current adjustment with temperature compensation • Output offset voltage adjustment • Output protection diodes (for driving 100V line transformers and electrostatic speakers) January 2017  29 clipping indicator for each channel in a stereo or surround sound amplifier. The power output is very similar to that of the Ultra-LD Mk.4 which is to be expected as it uses the same DC supply rails and same output stage configuration. Circuit description The main amplifier circuit is shown in Fig.1. A 1MΩ resistor DC biases the input signal at RCA socket CON1 to 0V. The signal ground (ie, RCA socket shield) is connected to power ground via a 10Ω resistor, which improves stereo separation when modules share a power supply; it prevents a ground loop due to the grounds being joined directly both at the power supply module and at the signal source. The signal passes through an RF at30  Silicon Chip tenuating RC low-pass filter (100Ω/1nF plus ferrite bead) and is coupled to the base of PNP transistor Q1 via a pair of series connected 47µF 25V electrolytic capacitors (which are together more compact and cost less than an equivalent non-polarised capacitor). A 12kΩ resistor provides a path for Q1’s base current to flow to ground. We have used readily available BC556 low-noise PNP input transistors for the input differential pair, Q1 & Q2. The input signal goes to the base of Q1 while negative feedback from the output goes to the base of Q2. Both transistors have 47Ω emitter degeneration resistors for improved linearity and they are fed with a common 2mA current via trimpot VR2 and power indicator LED1. VR2 allows the current split to be shifted slightly between the two transistors, to trim out base-emitter voltage mismatch and thus practically eliminate any output offset, to avoid excessive DC current when driving a line transformer or electrostatic speaker. LED1 has no effect on the operation of the circuit except to indicate when it is powered. The currents from Q1 and Q2 go to a current mirror comprising two BC546 NPN transistors Q3 and Q4. The 68Ω emitter resistors help ensure that equal current flows through each transistor as the voltage across these resistors is much greater than the base-emitter voltage difference between the two. Since the currents through Q3 and Q4 are held equal, any difference between the current from Q1 and Q2 must flow to the base of NPN transiliconchip.com.au Fig.1: the complete circuit for the SC200 amplfier module minus the circuitry for the clipping detector, which is shown separately in Fig.2. Q1 and Q2 are the input transistors while Q5 and Q6 are the constant-current source. The signal from the collector of Q1 is fed to the base of Q7, which together with Q8 forms the voltage amplification stage. Q9 is the constant current load for Q8, providing very linear operation. Q10 is the VBE multiplier and provides a floating voltage source which biases the complementary Darlington output stage. sistor Q7. Thus, Q7’s base current is proportional to the difference in input and feedback voltages. It forms the first half of a compound (Darlington-like) pair along with Q8, a 160V high-gain transistor. A 2.2kΩ resistor between its base and emitter speeds up switch-off. Q7 and Q8 together form the Voltage Amplification Stage (VAS). Q8 has a constant current source for its collector load, comprising transistors Q6 and Q9. Together, these set the collector current for Q8 at around 6.5mA. As a result, the current flow to the base of Q7 is translated linearly to a voltage at Q8’s collector which controls the output stage. PNP transistor Q5 provides a constant current of around 2mA to the input pair and both it and Q9 are driven by Q6, which is set up to maintain a siliconchip.com.au constant voltage across their emitter resistors. In other words, Q6 biases the bases of Q5 and Q9 in such a way as to maintain an essentially static current through their collector/emitter junctions. Output stage The output stage consists of two pairs of Fairchild power transistors arranged as complementary emitter-followers. NPN transistors Q13 and Q14 are connected in parallel and source current for the speaker while Q15 and Q16 are PNP types and sink current from the speaker. Surface-mount 3-watt 0.1Ω 1% emitter resistors ensure equal current sharing, linearise the output stage and produce a small amount of local feedback. They also serve as handy shunts for measuring the quiescent current. Large power transistors require a substantial base current due to limited gain and this is supplied by driver transistors Q11 and Q12. These effectively make the output stage a complementary Darlington. The parallel 220Ω resistor and 220nF capacitor between the driver emitters speed up their switch-off when drive is being handed off from one to the other. Quiescent current stabilisation The four base-emitter junctions in the output stage, plus the voltage across the emitter resistors adds up to around 2.2V (as shown just to the left of Q10 in the circuit diagram) and thus a similar DC bias must be maintained between the bases of Q11 and January 2017  31 +57V K CON4 (TO A OFF-BOARD CLIPPING K INDICATOR LED) A ZD1 4.7V  LED6 CLIP 100k K A 1k 100k A D5 1N4148 K 100k C Q17 BC546 B E 33k A K D6 1N4148 100k E C E 68k Q18 BC556 100k B C K C LED6 2N5551 B A B TP7 BC546, BC556 D7 1N4148 B K E A 100k K C E Q19 2N5551 D5-D7, ZD1-ZD2 A SC 20 1 7 ZD2 4.7V A –56V K CLIP PING DETECTOR FOR SC 200 AMPLIFIER Fig.2: the clipping detector monitors the output waveform and lights LED6 whenever the output voltage comes within about 4V of either supply rail. This indicates the onset of clipping. NPN transistor Q17 detects positive signal excursions while PNP transistor Q18 detects when the output signal approaches the negative rail. Q12 to keep the output transistors in partial conduction most of the time; otherwise, there will be substantial crossover distortion each time the signal passes through 0V. The reason is that when the signal polarity changes (ie, from positive to negative or vice versa), the output current drive is handed off from one set of output transistors to the other; ie, from Q13 and Q14 to Q15 and Q16 or the other way around. This transition has to be smooth or else there will be a step in the output voltage and the way to smooth it is to ensure that there is overlap between the conduction of both pairs. In other words, with the output at zero volts, all four transistors are passing some current. This is known as the quiescent current. This partial conduction requirement is a defining characteristic of a ClassAB amplifier (otherwise, they would be Class-B). To maintain a more-or-less constant quiescent current we need a “floating” voltage source of 2.2V between the bases of Q11 and Q12 and this is provided by the VBE multiplier Q10 and its associated components. But since the base-emitter voltages of the six transistors in the output stage all vary with temperature, a fixed floating voltage source is not suitable. The base-emitter voltages drop with increasing temperature at around 2mV/°C so a fixed voltage source of 2.2V would lead to increased current as the output transistors heated up and ultimately, to thermal runaway and destruction. VBE multiplier So our floating voltage source must not only be adjustable, to compensate for manufacturing variations in the output transistors and emitter resistors, it must also automatically reduce the bias as the amplifier heats up, so that the quiescent current remains reasonably constant. But first, let’s explain the basic concept of a “VBE multiplier” before we consider how it tracks and adjusts for changes in operating temperature. The VBE multiplier is sometimes referred to as an “amplified diode” and this gives some insight into its operation. Consider that the base-emitter voltage of a conducting transistor is around 0.6V. The bias network to our VBE multiplier comprises the 680Ω resistor between collector and base and the 1kΩ trimpot and 150Ω resistor between base and emitter. This forms a divider between its collector and emitter, with a tap at the base. We already know that the voltage between base and emitter is 0.6V and Specifications Output power (230VAC mains):.................. 200W RMS into 4Ω, 135W RMS into 8Ω Frequency response (10Hz-20kHz):........... +0,-0.05dB (8Ω); +0,-0.12dB (4Ω); Input sensitivity:.......................................... 1.26V RMS for 135W into 8Ω; 1.08V RMS for 200W into 4Ω Input impedance:......................................... 11.85kΩ shunted with 1nF Rated Harmonic Distortion (4Ω, 8Ω):......... <0.01%, 20Hz-20kHz, 20Hz-30kHz bandwidth Signal-to-Noise Ratio:................................. -116dB unweighted with respect to 135W into 8Ω(20Hz-20kHz) Damping factor:........................................... ~250 Stability:....................................................... unconditionally stable with any nominal speaker load 4Ω Music power:................................................ 170W (8Ω), 270W (4Ω) Dynamic headroom: ................................... 1dB (8Ω), 1.3dB (4Ω) Power supply: ............................................. ±57V DC from a 40-0-40 transformer Quiescent current:....................................... 88mA nominal Quiescent power:........................................ 10W nominal Output offset: .............................................. typically <10mV untrimmed; <1mV trimmed 32  Silicon Chip siliconchip.com.au Parts list – SC200 Amplifier Module 1 double-sided PCB, coded 01108161, 117 x 84mm 1 diecast heatsink, 200 x 75 x 28mm (Altronics H-0536) 4 M205 fuse clips (F1,F2) 2 6.5A fast-blow M205 fuses (F1,F2) 1 small ferrite bead (FB1) 1 2.2µH air-cored inductor (L2) (or 1 20mm OD x 10mm ID x 8mm bobbin and 1m of 1.25mm diameter enamelled copper wire, plug 10mm length of 20mm diameter heatshrink tubing) 1 1kΩ 25-turn vertical trimpot (VR1) 1 100Ω mini horizontal trimpot (VR2) 1 switched horizontal RCA socket (CON1) OR 1 2-pin polarised header (CON5) OR 1 vertical RCA socket (CON6) 1 4-way pluggable terminal block with socket, Dinkle 4EHDV or equivalent (CON2) 1 4-way pluggable terminal block with socket, Dinkle 3EHDV or equivalent (CON3) 4 TO-3P insulating washers 3 TO-126 or TO-220 insulating washers 7 15mm M3 machine screws with nuts 6 6mm M3 machine screws with nuts 4 9mm M3 tapped nylon spacers 8 PCB pins (optional; TP1-TP7) Semiconductors 2 FJA4313 250V 17A NPN transistors, TO-3P (Q13,Q14) 2 FJA4213 250V 17A PNP transistors, TO-3P (Q15,Q16) 3 KSC2690A medium power NPN transistor (Q8,Q10,Q11) 2 KSA1220A medium power PNP transistors (Q9,Q12) 3 BC546 NPN transistors (Q3,Q4,Q7)* 4 BC556 PNP transistors (Q1,Q2,Q5,Q6)* 1 blue 3mm or SMD 3216/1206 LED (LED1) 2 red 3mm or SMD 3216/1206 LEDs (LED2,LED4) 2 green 3mm or SMD 3216/1206 LEDs (LED3,LED5) 1 1N4148 small signal diode (D1)* 1 BAV21 high-speed signal diode (D2)* 2 FR307 3A fast-recovery diodes (D3,D4) Capacitors 1 1000µF 6.3V electrolytic 1 100µF 63V electrolytic 1 47µF 35V electrolytic 3 47µF 25V electrolytic 2 220nF 50V multi-layer ceramic or MKT 1 100nF 250VAC MKP 4 100nF 63V/100V MKT 2 1nF 63V/100V MKT 1 150pF 250V C0G/NP0 ceramic or MKT/MKP Resistors (all 0.25W, 1% unless otherwise specified) 1 1MΩ 4 47kΩ 1 22kΩ 2 12kΩ 2 6.8kΩ 3 2.2kΩ 1 680Ω 1 470Ω 1W 5% through-hole or SMD 6332/2512 1 470Ω 1 330Ω 3 220Ω 1 120Ω 1 100Ω 1W 5% through-hole or SMD 6332/2512 * SMD versions 2 100Ω 2 68Ω 2 47Ω 1 10Ω can be substituted; 1 6.8Ω 1% 3W SMD 6332/2512 see text next month 4 0.1Ω 1% 3W SMD 6332/2512 siliconchip.com.au since the beta (DC current gain) of the transistor is quite high (>100), it will draw negligible base current, so the current through the two resistors and trimpot VR1 will essentially be identical. Furthermore, since we will have 0.6V between base and emitter, it follows that we need 1.6V between collector and base, if we are to obtain 2.2V between collector and emitter. So, to adjust the resistance of VR1 to obtain 1.6V between collector and emitter, we need a resistance ratio between collector/base and base/emitter of 1.6V÷0.6V or 2.6666:1. This means the total resistance of VR1 and its series 150Ω resistor will be 680Ω x 0.6÷1.6 = 255Ω. And that means that trimpot VR1 must be set to a value of 255Ω -150Ω = 105Ω. We can therefore calculate the total resistance of the divider between collector and emitter at around 255Ω + 680Ω = 935Ω and therefore 2.2V / 935Ω = 2.35mA will flow through it. The remainder of the 6.5mA, ie, 4.15mA must flow through the collector/emitter junction of Q10. But what if the external operating conditions around the VBE multiplier act to increase the voltage between its collector and emitter above 2.2V? If that did happen, the resistive divider would cause its base-emitter voltage to increase but that would force the transistor to turn on harder and that would have the effect of reducing the collector-emitter voltage. So the VBE multiplier transistor is instead forced to operate with a constant collector-emitter voltage! In other words, it operates as a shunt voltage regulator, maintaining a constant voltage across the collector/emitter Additional parts for clipping detector circuit 1 2-pin header and matching plug (optional; CON4) Semiconductors 1 BC546 NPN transistor (Q17)* 1 BC556 PNP transistor (Q18)* 1 2N5551 high-voltage NPN transistor (Q19) 1 yellow, amber or red LED (LED6) 2 4.7V 0.4W/1W zener diodes (ZD1,ZD2)* 3 1N4148 small signal diode (D5-D7)* Resistors (all 0.25%, 1%) 6 100kΩ 1 68kΩ 1 33kΩ 1 1kΩ January 2017  33 SC200 Load Lines (Two Pairs Output Transistors, ±57V Supply, 1% resistors) 10 8 Resistive Load 8 Reactive Load, 135W (5.6+5.6j) 8  Resistive Load Collector Current (Amps)  Reactive Load, 200W (2.83+2.83j) 6 4 2 0 0 20 40 60 80 Collector-Emitter Potential (Volts) junction even if the current passing through it varies (but as long as it’s higher than the 2.35mA required for the divider to operate properly). Thermal tracking So how does VBE multiplier transistor Q10 adjust for temperature changes in the output transistors? We make it do that by mounting Q10 on the heatsink immediately between driver transistors Q11 and Q12. Furthermore, Q10 is the same transistor type as Q12, so the thermal tracking of the driver transistors and by extension, that of the four output power transistors, is quite good; not perfect but quite good. So if the temperature of the heatsink rises by 50°C, that would mean that the required base-emitter voltages of all seven transistors (for a given collector current) on the heatsink will reduce by 50 x 2mV = 100mV. If the base-emitter voltage of Q10 has reduced by 100mV, given that it operates with a gain of (1.6 + 0.6)÷0.6 = ~3.7 times, the voltage of our floating source will be reduced to 2.2V – 100mV x 3.7 = 1.83V and this voltage will be applied across the four baseemitter junctions of the complementary Darlington output stage transistors. That means that even though the transistor junction temperatures may have increased by 50°C, their quiescent current should remain much as it was at much lower temperatures. In practice, the process is not quite that good so we also have local feedback provided by the 0.1Ω 3W emitter resistors for the output transistors. If 34  Silicon Chip 100 120 Fig.3: this diagram shows resistive (straight) and reactive (curved) load lines for operation into loudspeaker loads. Note that all the load lines are comfortably inside the safe operating area (SOA – red line) of the paralleled output transistors. the voltage across these emitter resistors increases, due to increasing quiescent current, that will tend to reduce the base-emitter voltage (by subtraction) and therefore the current will reduce (or at least, not increase by as much as it would without them). By the way, the 220Ω resistors between either end of the Vbe multiplier Q10 and Q11/Q12 act as RF stoppers and also limit current flow under fault conditions (eg, a short circuit). Feedback & compensation Negative feedback goes from the junction of the output emitter resistors to the base of Q2 via a 12kΩ/470Ω resistive divider, setting the closed loop gain to 25.5 times (+28.5dB). The bottom end of the feedback network is connected to ground via a 1000μF electrolytic capacitor. This has a negligible effect on lowfrequency response but sets the DC gain to unity, so that the input offset is not magnified at the output by the gain factor of 25.5. The 150pF compensation capacitor is connected between the collector of Q8 and the base of Q7, ie, it is effectively a Miller capacitor for the VAS “Darlington” (in a real Darlington, the collectors would be common). This is a single-pole compensation arrangement which rolls off the open-loop gain at a high frequency to give unconditional stability with highly reactive loads across the amplifier’s output. The 22kΩ resistor in series with the collector of Q7 limits its current under fault conditions. Should the amplifier outputs be shorted, it will try to pull the output either up or down as hard as possible, depending on the offset voltage polarity. If it tries to pull it up, the output current is inherently limited by the approximate 6.5mA current source driving Q11 from Q9. However, if it tries to pull down, Q8 is capable of sinking much more than 6.5mA. The 22kΩ resistor limits Q8’s base current to around 2mA and since Q8 has a beta of around 120, Q8’s collector will not sink much more than 240mA. This is still enough to burn out Q12’s 220Ω base resistor but that may be the only damage from an extended short circuit; very brief short circuits will should not cause any lasting damage. Note that the 22kΩ resistor will cause Q7’s collector voltage to drop as it is called on to supply more current and the Early effect means its gain will drop when this happens. This can cause local negative feedback and oscillation. A low-value capacitor in parallel with the 22kΩ resistor prevents this while still allowing the current to Q8’s base to quickly drop to 2mA during a short circuit. Output filter The 0.1Ω 3W emitter resistors of output transistors Q13-Q16 are connected to the output at CON3 via an RLC filter comprising a 2.2μH series inductor in parallel with a 6.8Ω 3W surface-mount resistor, with a 100nF capacitor across the output terminals. The inductor isolates any added capacitance at the output (eg, from the cables or the speaker’s crossover network) from the amplifier at high frequencies, which could otherwise cause oscillation. The resistor reduces the inductor’s Q, to damp ringing and also forms a Zobel network in combination with the 100nF capacitor, which also aids stability. Driving a line transformer While a very low output offset voltage gives slight benefits when driving normal speakers, it’s absolutely critical when driving a 100V line transformer (for professional PA applications) or electrostatic speaker (which will typically have an internal transformer). That’s because the DC resistance of the primary winding will be much lower than that of a loudspeaker’s voice coil, so a lot of DC current can flow with an output offset voltage of siliconchip.com.au WARNING! High DC voltages (ie, ±57V) are present on this amplifier module. In particular, note that there is 114V DC between the two supply rails. Do not touch any wiring (including the fuseholders) when the amplifier is operating, otherwise you could get a lethal shock. just a few millivolts. The other requirement for driving a transformer is to have protection diodes on the amplifier output to clamp inductive voltage spikes which occur when the amplifier is driven into clipping (overload). These would otherwise reverse-bias the output transistor collector-emitter junctions, possibly causing damage. D3 and D4 are 3A relatively fast recovery diodes with low junction capacitance for their size and we have checked that they do not have any impact on performance. So there should be no changes necessary to use this module in a PA amplifier or to drive electrostatic speakers, as long as the output offset voltage is trimmed out during set-up. Indicator LEDs We have already mentioned a blue LED1 connected in series with the input pair current source and which is lit while ever the board has power applied. Since there is an ~50V drop required from Q5’s collector to VR2’s wiper, the power to operate this LED is effectively free. We’ve also included red/green LEDs LED2-LED5 to indicate the status of the output stage power rails. It isn’t always obvious that a fuse has blown without careful inspection. In the case of LED2, assuming F1 has not blown, the voltage at either end of the fuse-holder is the same so no current will flow through the red junction. However, LED3is connected between the collectors of Q11, Q13 and Q14 and ground via a 47kΩ currentlimiting resistor, so it will light up. If fuse F1 blows, the collector voltages will drop to near 0V, so green LED3 will turn off but the full rail voltage will be across the fuse-holder and so the red LED2 will switch on. Similarly, LED5/LED4 indicates green/red when F2 is OK/blown. These LEDs will also indicate if one of the two supply rails is missing (eg, due to a wiring fault); in this case, siliconchip.com.au Spot the five surface-mount 3W resistors. Four are the emitter resistors for the output transistors and the fifth is inside the output inductor. LED1 will probably still light up so it might not otherwise be obvious. Clipping indicators Now we can talk about the on-board clipping detector/indicator circuit. This involves just a few components and will indicates whenever the amplifier is driven into clipping, which may not be obviously audible. It can drive an external LED mounted on the front panel of the amplifier. These components may be omitted if they are not required. The clipping detector circuit is shown in Fig.2. Zener diode ZD1 derives a reference voltage 4.7V below the nominally 57V positive rail, ie, at about +52V. This is connected to the emitter of NPN transistor Q17. Its base is connected to the amplifier’s output via a 100kΩ current-limiting resistor, with diode D6 preventing its base-emitter junction from being reverse-biased. At the onset of clipping, the speaker voltage will rise above the +52V reference plus Q17’s base-emitter voltage, ie, to about +53V. Q17 will switch on and sink current via LED4, a 1kΩ current-limiting resistor and isolating diode D5, lighting up clipping indicator LED6. As the reference voltage is relative to the positive rail, any variations in supply voltage will be accounted for. ZD2, PNP transistor Q18 and diode D7 work in an identical manner for negative excursions. However, Q18 drives LED6 via highvoltage NPN transistor Q19 which acts as a level shifter. The 100kΩ resistor in series with its collector limits the LED current to a similar level (1mA) despite the much higher rail voltage differential. This is not the simplest clipping detector circuit but it presents an almost completely linear load to the amplifier output, to minimise the possibility of any distortion due to its input load current. It’s connected to the driven end of L2, to give the amplifier the best chance to cancel out any non-linearities in the load it introduces. Next month Have we whetted your collective appetites? Next month we will present the full details of performance and construction details. SC January 2017  35