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  • RIAA Equalizer Amplifier Design

    RIAA Equalizer Amplifier Design

    This article explores the fundamental’s of phono amplifier design,  culminating in a few practical designs. Special emphasis is placed on overload margins (critical if you want good sonics from your EQ amp), driving the EQ network adequately and noise.

    RIAA Equalization Amplifiers V2.0

    Below is the RIAA Calculator Excel spread sheet.  Please read the article above, before attempting to use the tool below.  Once you have calculated your RIAA values,  you are strongly encouraged to check your design out using a spice model – I use LTSpice,  but any  Spice simulator will work.

    Here are some guidelines to help you use the spreadsheet tool:-

    1. In his paper, Lipshitz discussed how all the time constants interact in the classic all-active RIAA (which is what I focus on in my article above and I recommend for best performance).  It is the most difficult to design, but you get superior overload and noise performance using this approach i.e. no trade off’s to make as in the case of passive, active-passive or passive-active approaches.
     
     
    2. Lipshitz  provides a methodology with which to accurately calculate the component values despite the fact that they are all interacting with each other – so the process in the spread sheet is a bit iterative to converge on the correct values.  Remember, you cannot simply calculate the RC values from T=RC – if you do, your RIAA break points will be all over the place
     
     
    4. Follow the steps below precisely to use the tool correctly
     
     
    A.  Set L18 to 1 kHz (I actually should have fixed this in the spread sheet at 1 kHz but did not – learning point for a future version )
     
     
    B. Select R0 in J6.  This is the lower arm resister in the feedback network that goes from the inverting input to ground, or to the DC blocking capacitor.  A value of between 100 and 500 Ohms works best.  If you try to go outside of these values, you can run into difficulties with getting the RIAA values to converge in the spread sheet, or you will get crazy values.
     
     
    C. Adjust T1 (cell E7) for the correct gain in L22 (magnitude) and L24 (dB).  I usually go for a gain magnitude of 50x to 60x which =~50-53 dB at 1kHz.
     
     
    D. Now comes the hard part: Adjust T6 (cell E12) for EXACTLY 1.000 in cell J14. You should find the value in J14 to lie typically between about 300k and 1.5 million.  Its important that you iterate on this step until you get 1.000 in J14.  This sets the resistor and capacitor values in the feedback network very accurately to the RIAA time constants.
     
     
    E. The next step is to calculate the secondary post filter value by inserting a capacitor value into L11.  A value of 10nF is a good starting point.  Do not have values of R31 less than 50 Ohms as you don’t want to capacitively load the opamp at HF (it might go unstable).  R31 should typically lie between 50 Ohms and 330 Ohms.
     
     
    F. I highly recommend you then put the values into an LTspice model and run  an AC analysis to check the conformity.  I typically get 0.2 dB 20 Hz to 20 kHz, and by tweaking the values slightly in the simulator,  easily get to 0.05 dB 20 Hz to 20 kHz.  However, in practical terms, anything better than 0.5 dB is very good.
     
     
     

    Here is an excellent noise calculator developed by Stuart Yanniger that allows you to calculate the real world noise of any  cartridge. This spread sheet does NOT include amplifier noise, but instead shows just how much  noise the cartridge+loading resistor combination produce. For the most part, it far exceeds that of any competently designed RIAA equalizer preamplifier  

    RIAA_Calculator.xls

  • Ground Loops

    Ground Loops

    Updated with new material 7th January 2019

    This set of c. 70 slides is the culmination of my experience over a period of about 25 years building  power amplifiers and preamplifiers. I first started out in audio around 1975 or 76 as a teenager. Some of my creations were reasonably quiet – through pure luck – and others hummed and hissed horribly. Later, my skills improved dramatically, and especially so after reading one of Henry Ott’s books back in about 1988/89 whilst developing a very high-resolution Digital Panel Indicator for industrial applications at the company I worked for. I then left DIY audio for about 15 years (career, family etc), returning to the subject again in 2005, having forgotten a lot of my practical skills. The path from electromagnetic theory expounded on numerous websites, application notes and posts on various web forums to building quiet amplifiers every time is not easy and requires a bit of practice. The underlying theory can be extremely complex (think Maxwell’s equations), however, with some effort and focus you can quickly master the basics.  This set of slides focuses on unbalanced interconnects (aka ‘single-ended’) that use the standard RCA phono connectors, since this is where problems mostly arise.

    When it comes to humming and hissing amplifiers, good practical advice is scarce and misguided opinions on the subject easy to find.

    This presentation (which will remain a work in progress and be expanded from time to time) is designed to get audio constructors up and running quickly both in the construction/planning phase, but also debugging. It will hopefully also serve as a useful reference for anyone wanting to know a bit more about EMC as applied to amplifiers.  One important thing about EMC: you will never stop learning, and finding new problems to solve.

    Ground Loops

    Here is DIYaudio member Ilimzn’s excellent posts on the subject that I gathered into a single document:

    ilimzn’s Excellent Posts on Ground Loops

    Here is some additional material:

    Amplifier PCB Design Guidlines for Minimizing Hum

    Some practical guidance offered to a builder on diyAudio:

    More Notes On Amplifier Hum Problems

    For some practical examples of low noise amplifiers using these techniques,  see the nx-Amplifier and sx-Amplifier on www.hifisonix.com

    Here are some commercial products that use the techniques described in the presentation: www.ovationhifidelity.com

    The picture below shows the internal wiring of one of the two nx-Amplifiers I built a few years ago with zero noise or hum problems. The power wiring is tightly bundled, and small signal wiring is kept well away from the transformer and other power wiring. On the PSU PCB, strict attention to the capacitor ‘T’ connection and ‘star’ ground return result in an exceptionally quiet amplifier.


    IMGP8749

    Finally here is a YouTube video of HOW NOT TO DEAL WITH GROUND LOOPS. What is really disconcerting about this is that if you type ‘Ground Loops’ into Google, this will probably be the first reference that comes up on the list.

    All the basic safety rules about earthing [grounding] by using a ‘ground lifter’ are completely broken and the noise problem has actually not been solved – they have gone around the problem and made the product completely unsafe in the process – and especially so since this is on a tube amplifier.

    The question to ask when dealing with a potential safety fault is ‘What would happen if the live wire  came loose and touched on the input jack, or any other metalwork on the product without the safety earth[ground] connected?’ If the answer is ‘it would be at the live potential’ don’t do it!

    Never, ever, use a ground lifter in the manner shown in the YouTube video to get rid of hum – its plain dangerous and illegal. Period.

  • MC Head Amp Circuit Compendium

    MC Head Amp Circuit Compendium

    Here is the new updated moving coil head amp designs compendium – updated 31 July 2019. The first file is a PDF compendium of about 28 different circuits with noise, distortion and current consumption details. All the LTspice sim files are zipped in the second file.

    What is immediately apparent from this is that having an amplifier that is much quieter than the source resistance gives little benefit.

    The table below shows how the amplifier noise and the source resistance noise add. Select your amplifier equivalent noise resistance on the y axis, your source resistance on the x axis and the intersection is the total equivalent input noise. Note, as is the table does not account for input noise current – but this should not be an issue with head amps that use 1 or 2 bipolar transistors for the amplifier stage.

    For example, if the source resistance is 40 Ohms, a very quiet amplifier with an equivalent input noise voltage of 2 Ohms (something like the Hawking designed by Richard Lee in the presentation above) offers only about 1/3rd lower total system noise (0.83nV/rt Hz) noise than an amplifier with an equivalent input noise of 40 Ohms i.e. 1.15 nV/rt Hz.

    On the other hand, if the source resistance is just 2 Ohms, but the amplifier equivalent noise resistance is 40 Ohms (akin to a JFET input stage), the difference is far more marked and the total system noise will be about 3.2x worse than the source resistance noise.

    So, as a general rule we can say:- If the amplifier equivalent noise resistance is not more than 1.414x the source resistance noise, it will be just audible since the human ear can just about detect 1.5 dB change in power level.

  • Hifisonix Ripple Eater PSU for the sx and kx-Amplifiers

    Hifisonix Ripple Eater PSU for the sx and kx-Amplifiers


    The PCB’s are  through hole plated and silk screened and are available from Jim’s Audio here:

    Ripple Eater PSU for kx and sx Amplifiers

    (please note these PCB’s are not available from the Hifisonix Shop)

    Here is an Excel file with the BOM:  Ripple Eater PSU BOM

    The BOM is provided for assistance – always carefully check the part numbers and quantities before ordering.

    Here is the BOM if the link above does not work

    Introduction

    Here is a very simple capacitor multiplier PSU aka ‘ripple eater’ for the sx or kx-Amplifiers.  The LTspice simulated ripple rejection at 100 Hz is about 65dB and at 10 kHz it is 85 dB.  These figures assume you have a 2.5A load and also include the on-board filter capacitors on the amplifier modules themselves (220uF per rail on the sx-Amp and 1000uF per rail on the kx-Amp per amplifier module).

    Class A amplifiers draw heavy quiescent current from their power supplies, and this gives rise to significant amounts of mains related ripple that will affect the amplifiers noise performance.  VFA amplifiers generally have better LF PSU noise rejection than CFA’s, but it can still be a problem with a class A VFA.

    A further benefit of this supply is that the radiated mains noise from the PSU to amplifier module wiring is greatly reduced because you will be supplying close to DC into the amplifier module local reservoir capacitors, so the associated mains ripple charging currents are very low. Low frequency (because the HF currents will be provided by the local on board reservoir capacitors – 220 uF for the sx-Amp and 1000 uF for the kx-Amp) signal related currents will still be flowing in the wiring of course, so you have to pay careful attention to layout, how you dress the wiring, loop area minimization and common impedance coupling issues – you can read more about this in ‘How to Wire -up a Power Amplifier’. Nevertheless, this PSU goes a long way to making sure your finished amplifier can be as quiet as theoretically possible. When combined with the 50~60dB mains noise rejection of the actual amplifiers themselves, the noise levels on the amplifier output will be down as much as 100 dB which is an outstanding result by any measure. At HF, the performance will be even better, and that is important for the amplifier sound in the mid and high range.

    The series pass transistors (8A MJE15032/33 devices) are designed to be mounted underneath the PCB with their tabs screwed to the amplifier chassis base using the appropriate thermally conductive insulator (same mounting technique as the main rectifier D4 as well but you do not need the insulating washer on the rectifier – only some thermal grease).  Each pass transistor will dissipate about 10W in a stereo set-up delivering full output power into the loudspeaker load.

    In normal operation, you will drop ~2  volts across each pass transistor, so if you want an output of say +-27 V, the loaded DC voltage into the PSU should be 29 V.  Note carefully as well, this power supply does NOT regulate the output – it will track the raw filtered DC voltage, but remove the ripple hence the ‘ripple eater’ name.

    How Can I use Ripple Eater PSU on class AB Amplifiers with Higher Supply Voltages?

    You can use this ripple eater power supply as is up to +-35V.  You can also use it on amplifier with higher supply voltages up to +-50V. However, you must change the filter capacitors to 50 or 63V types (this is C1 and C6 in the schematic).  In a class AB amplifier, you can use values that are about 3x LOWER than you would on a class A amplifier – so about 15 000 uF at 50 or 63V would be correct.  You must also change C5 and C7 to 50 or 63 Volts.  Finally, change R5 and R6 to 10k each. Note that the Ripple Eater PSU is not suitable for amplifiers with power supply rails much above +-50V because the series pass transistors (Q1 and Q3) are rated at 8A continuous and this places an upper limit on the output power.

    Can I Increase The Power Handling Capability of the Ripple Eater?

    Yes – you can.

    Replace Q1 with an NJW3281 or a MJW3281

    Replace Q3 with an NJW1302 or MJW1302

    The PCB mounting holes for Q1 and Q3 will NOT accept the larger types above, you  must run short wires from the PCB to the larger suggested power transistors above.  Do not mount the offboard transistors more than 10cm away from the PCB. Make sure the transistors have a good heatsink – again, I recommend you mount them to the chassis if it is constructed of 3mm thick or more aluminium.

    Remember, the transistor collectors must be insulated from the chassis – use a suitable silicon heatsink pad

    Performance

    The graphic below gives some indication of the performance (simulated) of the ripple eater supply. I used a ripple eater on the e-Amp to clean-up the supply to the amplifier front end and got better than 30 dB ripple rejection, so the technique works extremely well in practice. In the simulation below, for the first 40 ms, both LF and HF noise are presented to the input, and for the remaining 60 ms, just LF noise is presented. The aqua trace at bottom is the output and as you can see, the LF and HF noise is significantly attenuated.

    A Word of Warning

    There is a considerable amount of energy stored in the capacitors and there is NO CURRENT LIMITING on the ripple eater output.  If you accidently short the output of the power supply, the series pass transistors (Q1 and Q3) will blow up in spectacular fashion.  So, exercise caution when wiring up!

    Secondly, remember the series pass transistors are rated at 8A – so they are not designed to supply full load current into  a 4 Ohm load with continuous sine wave testing both channels driven – they will pop if you do this.  If you want to do full load continuous wave testing, short out the collector to emitter on Q1 and Q3.  Once testing is complete, remove the short.

    Component Overlays, Assembly and Some Pictures

    Here is the component overlay for the PSU.

    Below are some pictures of the finished board. Note carefully how the main bridge rectifier (D4) and the series pass transistors (Q1 and Q3) are mounted underneath the board and lay flat on the amplifier (metal) chassis.

    ATTENTION!

    YOU MUST USE AN INSULATING THERMAL WASHER BETWEEN Q1 AND Q3 AND THE AMPLIFIER CHASSIS!

    You do not need to insulate D4 from the chassis as the thermal pad on the underside of the device is electrically isolated from the internal diodes – you must use thermal grease however to thermally couple it to the chassis – it will overheat and fail if you don’t.  Remember to check with a DVM to see that there is no continuity between the chassis and the series pass transistor collectors.

    Further Notes on Heatsinking/Thermal Management

    If your chassis  base plate is made of aluminium of at least 3mm thick, you can mount the Ripple Eater PSU as suggested above. If however your chassis is made of steel, it probably wont be too efficient at dissipating the pass transistor heat, so its best then that you use a separate heatsink and mount the devices to that.  Here is a suitable one from Mouser Aavid 3.7C/W Heatsink

    If you do mount the series pass transistors (Q1 and Q3) off-board, remember to twist the base, collector and emitter wires from the PCB to the heatsink mounted transistors and keep them as short as practicable (avoid going much above 10cm if you can).

    You must use 8 or 10mm stand-off’s  – not longer. Suitable Mouser Pt# 534-24337 or 534-24433 or 534-24443.  In Europe, you can try RS components 280-9023 (expensive) or Reichelt in Germany DI 10 (best price)


    Here are some photos of the ripple eater in action.  In this set-up I am running the kx-Amp off 33V rails with 400 mA per channel standing current.  I used 33 000 uF capacitors (the 47 000uF were not available). The voltage drop across the series pass transistors (Q1 and Q3) with 800 mA total load current   is 1.66V

    This is the input voltage and the 100 Hz  ripple is about 1.5V pk~pk

    This next shot is the output of the ripple eater, and shows virtually no noise – the scope vertical scale is the same at 500 mV/div.

    The final shot below zooms in on the ripple (vertical scale is now 20 mV/div) and we see it is in fact about  14 mV pk~pk,  which is a reduction of 40 dB and there are far fewer HF harmonics in the remaining (very low) ripple.


  • How to wire-up a Dual Mono Bloc Amplifier

    A few people have asked about wiring up a dual mono amp aka dual mono bloc. In a dual mono bloc there are separate power supplies and lots of opportunity for cross channel ground loops and ordinary ‘classic’ ground loops as well.

    This wiring scheme addresses the situation were unbalanced connections between the source equipment and the dual mono bloc is used and should allow a dual mono amp to be wired up that is quiet – i.e. no hum.

    The trick it to ensure that there is one and only one connection between the two amplifiers, and that is accomplished by bonding the input connector signal grounds together in this approach.

    The wiring scheme uses two ground lifters, although you could cheat and just lift one of the amps, and ground the other directly to the chassis, but I suggest you just spend a little extra effort and use two ground lifters.

    A major issue here, as in any DIY amp, is safety. Kindly note the chassis (assumed to be steel or aluminium) is bonded directly to the incoming safety ground (earth) on the IEC receptacle. You cannot under any circumstances omit this connection – it is the most important connection in DIY any amplifier. Using the ground lifters, the two amplifiers and their associated power supplies 0V then float +- 1.4V around the safety ground (earth). For the ground lifters, I always recommend you use a decent 35A 400V bridge rectifier – details in the presentation, although you can use large diodes with a high surge rating.

    For the transformers, use a Toroidy (based in Poland) audio grade device with a GOSS band to minimize the radiated mag field, or if specifying custom devices, ensure your order your transformer with a GOSS band. An interwinding screen will also help to minimize mains conducted common mode noise.

    One final point: there is a tendency for builders to mount the RCA input connectors on opposite sides of the rear panel. This creates a huge loop area inside the amplifier and the opportunity for a cross channel ground loop. Mount them next to each other and run the input wiring around the edge of the chassis in order to minimize the inter-channel loop areas – again, details in the presentation.


  • Noise in Electronic Circuits

    I’ve gathered a few articles here on noise as a go-to reference for anyone interested in the subject. These articles really focus on Johnson noise and not induced noise which is discussed in depth in the ‘Ground Loops’ post elsewhere on this site. I will update this post with new material as and when it becomes available.

  • Very Simple, Accurate RIAA Phono EQ Amp

    Very Simple, Accurate RIAA Phono EQ Amp


    Very High Quality Silk Screened PCB’s for this project are available from Jim’s Audio here:-

    Hifisonix RIAA Amplifier

    Here is a simple no-nonsense, accurate RIAA equalizer amp you can easily build.  The design uses an all-active topology and is based around an NE5534A low noise opamp. I make no claims for originality but you wont find any voodoo engineering, fairy tales or outrageous claims: It simply does what it says it does in the specification.

    A complete stereo board can be built for about £25 ($35), but probably less.

     

    The article provides some background information on the RIAA EQ standard, launched in 1954, and why it came to be the de facto industry standard after about 1960.

    hifisonix RIAA Phono EQ

    To use the PDF PCB layouts below, you must print the documents out on A4. Measure the reference line lengths to make sure they match. You printer should be 600 DPI resolution or better.  However, I strongly recommend you just buy the PCB’s from Jim’s Audio – link above.  These are very high quality boards, silk screened and gold flashed.

    Overlay and 1:1 PDF negative and positive for the EQ board:  Hifisonix Phono EQ Amp for Doc114

    Optional PSU Overlay and 1:1  PDF positive and negative: Hifisonix Phono EQ PSU106

    Gerbers for both the EQ amp and the PSU   Hifisonix RIAA EQ Gerbers      Hifisonix RIAA PSU Gerbers

    Any questions, feel free to email me.

    Can I use other op-amps with the Hifisonix RIAA?

    Yes, you can. I recommend that you use unity gain stable devices with will not require an external compensation capacitor, unlike the NE5534 used here. You must  first REMOVE C2 and C21 – these are the 10pF compensation capacitors.  The number of good opamps in 8 pin plastic DIP packages (PDIP or mini-DIP) is unfortunately not what it used to be, so you may have to use a SMD to PDIP adaptor if you want to go down this route.

     

     

    The plots below are for HIGH gain.

    The plot below is of the RIAA noise and distortion at 500mV output at 1 kHz A weighted. This was with board on the workbench, no screening or special precautions and the power supply located about 15cm away.  In a metal housing, you can expect about a 30 dB reduction in the 50/60Hz noise.  There is quite a bit of noise being picked up from the surrounding CFL lamps etc, but the distortion is almost entirely 3rd harmonic (at -70 dB), with a bit of 5th at about -85 dB.

     

     

    The plot below is the frequency response after the source signal is passed through a very accurate inverse-RIAA network. The white noise frequency response measurement technique used eliminates  extraneous noise sources and is therefore extremely useful.  It works by looking at the power spectral density of the amplifier output, which for a white noise source, is constant per octave. If the amplifier response (after passing through the inverse RIAA) is indeed flat, then the overall response will be flat. The A-D was set to 24bits /192 samples per second and the response display set to 30Hz to 100kHz. The RIAA conformity is excellent with no HF peaking and starts dropping off cleanly beyond about 30 kHz.

     

     

     

  • Amplifier History: The JBL SA-600

    Amplifier History: The JBL SA-600


    The beautifully styled JBL SA-600 amplifier was launched by the James B. Lansing company in 1966, and Bart Locanthi (the designer) wrote the  technical article (link further down) in January 1967.  This is one of the earliest – if not the earliest – example of a commercial  amplifier that addressed the potential for TIM/SID and that of Large Signal Non-linearity (LSN).

    In the mid 1960’s, most engineers were still working with tubes which had low loop gains and were not equipped to deal with the wider bandwidths, higher loop gains and attendant phase shifts that multi-stage solid state amplifiers offered. However, the SA-600 designer, Bart Locanthi, had cut his teeth on military guidance systems in the 1950’s – the heyday of the analog computer – and would have been, as I have remarked elsewhere on this site, highly cognisant of things like slew rate, slewing distortion, loop gain, phase margin, overshoot and so forth.  Unusually for the time, the front end diff pair (Q7 & Q8)  is degenerated and loop compensation provided by an 82 Ohm and 150 pF resistor across their collectors along with a 220 Ohm and 75pF network from the VAS output to ground.  It operates in inverting mode, which has been tried on numerous commercial amplifiers over the years (the modern take on this is that non-inverting mode offers advantages with respect to noise performance).  This design delivered 30 Watts RMS per channel, which was more than enough for the efficient loudspeakers of the day, and quite in line with the general power levels on offer from tube based gear.

    Locanthi’s EF3 output stage, nicknamed the ‘T’, has remained the go to circuit for high performance solid state amplifiers  – it features wide bandwidths, very high current gain, and can easily be scaled up by adding output transistors in parallel.  Because of the high gains involved, care is needed in layout along with good local decoupling.  Although we do not have the rest of the power supply details, it seems this was well taken care of along with the base stoppers preceding Q3 and Q4.

    Bart Locanthi

    Nowadays, we would do things a little differently insofar as compensation goes (for example, the VAS would not be loaded to ground), and the VAS would certainly be loaded with a current source in the manner described by Douglas Self’s ‘blameless’ amplifier.  Nevertheless, this design is a classic and was years ahead of its time in a number of very important aspects. Otala’s paper on TIM was still a few years away and he would regrettably draw the wrong conclusions from his findings i.e. that TIM is the result of feedback. We now know this is emphatically not the case – its all about how it is applied.

    It should be remembered that solid state devices were still in their infancy, and very expensive compared to todays prices – this required some creative engineering to minimize costs and still end up with reasonable performance which this design certainly does.

    However, the other fascinating thing about this amplifier is that it has held up its value remarkably – a bit like a Rolex watch.  If you root around on eBay or any of the pre-owned hi-fi websites, you are unlikely to pick up a cosmetically good working unit for less than about $2000 (!) and I’ve seen immaculate exemplars for sale at over $4000 (eBay Japan). So, highly regarded in its day for its liquid tube like sound,  and still sought after as a collector’s piece – which just goes to show that a well-engineered product – be it solid state or tube – can hold its value for decades and still deliver an outstanding listening experience when partnered with sympathetic ancillary gear.

    You can read Locanthi’s original description of his design below :-

    Locanthi Amplifier 1966

    Here is a short review of the amplifier done in 1966 by Julian Hirsch

    JBL – SA-600 Stereo Amplifier (J.D.Hirsch) (1966)

    A vintage JBL SA600, recently restored for a member of Audio Science Review, underwent technical assessment by the ‘Chief Fun Officer’, Amirm. While the restoration was extensive, my analysis suggests the amplifier still exhibits residual faults. Specifically, the measured level of hum and noise, even by 1966/67 standards, would have been considered unacceptable for a product of this calibre. Modern, well-engineered amplifiers will surpass the JBL SA600 in terms of absolute hum, noise floor, and distortion levels and this simply reflects the maturation of audio design, where knowledge has disseminated widely since the SA600’s era.

    Despite these observations, reviewer Amirm acknowledged the amplifier’s performance considering its 60-year vintage. Notably, Julian Hirsch’s original review cited measured hum and noise figures exceeding -100 dB, a remarkable achievement. In my view, this discrepancy suggests the restored unit tested by ASR may still harbour unresolved issues. At the time, the SA600 competed primarily with tube amplifiers, which exhibited higher noise, hum, and distortion while delivering significantly less power than the SA600’s conservatively rated 30 to 40 watts, as noted by Hirsch.

    Interestingly, the placement of input and power connectors on the amplifier’s bottom chassis reflects the prevailing audio system design of the time. In an era where systems were often integrated into wooden consoles, this configuration facilitated efficient cable management.

     

  • Solid State Feedback Amplifiers: A Short History

    “Why, sometimes I’ve believed as many as six impossible things before breakfast.”
    Lewis Carroll, Alice in Wonderland   

     A Future Without Feedback by Martin Colloms

    There is no mysticism in amplifier design, just serious science.
    Andrey A. Danilov

    Introduction

    You will recall from the The Theory of TIM by Matti Otala elsewhere on this site, that one of the consequences of the discovery of TIM in early solid state amplifiers was the erroneous conclusion that it was caused by feedback. By the time high loop gain solid state amplifiers really made their presence felt in the mid 1970’s (remember those Japanese receivers with the cool looking dials and green and blue lights?), vacuum tube amplifiers had ruled the roost for close to 50 years.  The  problem more often than not with tube amplifiers was lack of loop gain, or due to transformer coupling and attendant phase shifts, the inability to apply large amounts to linearize the system – 1% distortion was the norm, but really good designs might get you to the 0.3~0.5% mark at 1 kHz. Reading through solid state technical literature of the time, one comes away with the sense that most designers were groping around in the dark, trying to make sense of the new solid state paradigm, wide bandwidths, high feedback and  how to manage this combination effectively. It is clear with hindsight that although the solutions were ultimately simple, the real cause of the dilemma was that there were a number of interlinking factors, which we will touch on a little later, that took some time to tease apart.

    Dealing with the 20 dB loop gains and limited bandwidths that were the norm in tube equipment left the vast majority of designers ill-equipped technically to make the transition to solid state Voltage Feedback Amplifiers  (VFA) where the figures were 40 ~ 50 dB and open loop unity gain loop frequencies of 500 kHz or more. There were a few notable exceptions of course, one of them being Bart Locanthi of JBL who, judging from this design dating from the mid 1960’s was already cognisant of the challenges of high(er) feedback. He employed degeneration of the LTP stage of what was then an early high power solid state amplifier in order to improve the dynamic performance and linearity.  Earlier in his career he had worked in analog computing where much of the research in the 1950’s was around military equipment and  servo systems. He would therefore have been aware of things like loop gain, slewing, transient recovery, phase and gain margin – all critical parameters in servo systems, and as the industry came to learn years later, solid state audio amplifiers, but a rather alien world to vacuum tube consumer electronics designers in the 1960’s.

    Prior to Otala’s work, most amplifier designers naively saw feedback as some sort of panacea, to be applied in huge quantities to reduce distortion, invariably quoted at 1 kHz, which masked a host of evils that would be plainly evident at 30 kHz. One could arguably conclude that Otala discovered in TIM what was already known in another engineering discipline (servo and control theory), but  failed to interpret and apply his findings correctly – a point Bruno Putzeys’ touches on in ‘The F Word’.  We owe Otala a debt of gratitude for spurring the industry wide investigation into feedback his paper triggered, but the road to understanding the intricacies of feedback as applied to solid state audio amplifiers, and to being able to build high performance products, was to take at least another twenty years.

    The Four Evils

    In the first of what I shall term the four evils, many amplifiers from the time ran the front end LTP transistors at very low tail currents in the 1 mA region and I’ve seen power amplifier designs with 500 uA tail currents – so 250 uA in each LTP half. This immediately limited the peak current that could be supplied to the TIS integrator (trans-impedance stage aka VAS), and severely hobbled the LTP’s ability to handle input transients because it lacked the current needed to charge and discharge the compensation capacitor rapidly at HF.  The second evil was the failure to degenerate the LTP transistors – the gm as a result was high, contributing to the high overall loop gain.  Worse however, the high gm results in a narrow linear operating region such that each half of the pair can be ‘flipped’ ON or OFF with very small differential input signals – and that, as we shall see, is a serious shortcoming. The third evil was the lack of high fT, large SOA output devices – the 2N3055/2N2955 and later MJ15003/MJ15004 devices  featured pedestrian 1~2 MHz fT’s – in other words, they were incredibly bandwidth limited and would only work in a system if the unity loop gain frequency (ULGF) was low. All the more reason why Bart Locanthi’s amplifier was such a breakthrough as he built a credible amplifier with what by today’s standards would be seriously compromised output devices.  If one has to try to design an amplifier with these devices today, the unity loop gain frequency would have to be set to 300 kHz – about 5 times lower than in modern amplifiers where  devices like the  NJW3281/1302  are employed that have fT’s of 30 MHz, very high Ic vs hFE linearity and superb SOA capability. This in turn would have then limited the amount of feedback available to correct distortion and is one of the reasons amplifiers from the period generally have distortion figures of 0.007 to 0.01% – about 10x to 15x modern amplifier figures. There were a number of cases where commercial amplifiers would self-destruct if the wrong type of speaker cable was used (it needed to have high inductance to isolate any capacitive load). These products were marginally stable with insufficient gain/phase margin to deal with real world loads.  The fourth evil was that in order to tame the tendency to break into oscillation given the high loop gains and slow output stages, heavy MC (Miller Compensation) around the TIS (VAS) was applied, where I have seen capacitor values as high as 1 nF.  In an attempt to tame the amplifiers predilection to break into oscillation, all sorts of frequency shaping networks were applied across LTP load resistors, or heavy handed shunt compensation was used from the TIS output to ground in these old designs. With modern circuit simulation CAD tools like LTspice, amplifier compensation design and optimization is a cinch – designers in the 1970’s were in effect ‘flying blind’ in this area.

    When you present an amplifier with a fast transient on its input,  the LTP pair has to charge the compensation capacitor around the 2nd stage TIS integrator. In an amplifier that suffers from the evils mentioned earlier (and especially evils one, two and four – low tail current, high gm and oversized compensation capacitor), the LTP transistor halves will switch fully ON or fully OFF depending on the signal slope (+ve or -ve). When the amplifier does this, it runs open loop – i.e. without feedback and the output then slews towards one of the supply rails. The result in severe cases is the output rams up against one of the supply rails until the LTP regains control again a few micro seconds later and the loop runs normally again until the next fast music transient. This is what TIM is and it sounded terrible to audiophiles who were used to the smooth, euphonic sound of tubes. In designs that did not go ‘fully TIM’, the amplifier would slew for a shorter period, but not ram up against either of the supply rails. The sound was equally objectionable and this is called SID or Slewing Induced Distortion. There are plenty of commercial amps and DIY designs from the period, that with a full power sine wave stimulus, went into slewing at 30 or 35 kHz  – already absolutely unthinkable by the standards of 1998 when Colloms piece was published.

    Superbly Low 1kHz Distortion But Flawed Sonics

    With a steady state 1 kHz sine wave input stimulus and near full output power (a typical 1970’s test regime),  a highly compromised amplifier suffering from the 4 evils would test out superbly. How can this be? Amplifier distortion performance  used to be assessed at full power using a 1kHz stimulus.  The output rate of change of a 1 kHz sine wave at the zero crossing on a 100 W amplifier is only about 250 mV per microsecond – a snails pace even for our compromised amplifier, which would pass this test with flying colours, and because of the very high loop gain, distortion would low. Now feed a fast rise time  – say 10 us – 1 kHz square wave stimulus for full output power (about 8 V/us slew rate) and our amplifier performance falls to pieces. Full power square wave testing, or indeed full power HF sine wave testing, was almost never carried out on these products because of cross conduction problems in the output stage – so square wave testing was always small signal – i.e. 1~2 V peak output and the problems alluded to above thus never showed up. Further, testing was usually conducted with a resistive load, so marginally stable designs often slipped through the net and went on to fail in the field because they broke into oscillation with real world capacitive loads.

    Otala’s Misguided Legacy: Feedback is Bad

    Following Otala’s paper, a number of old wives tales about feedback emerged that still persist despite 40 years of engineering evidence and scholarly research to the contrary – and regrettably repeated in the Colloms article. One enduring fallacy for example, is that the open loop, low corner frequency (a few Hz to maybe a few hundred Hz) that one finds in Miller compensated (MC) amplifiers mean these are ‘slow’ and cannot follow fast music transients and this leads to TIM and the solid state sound.  This is entirely incorrect at every level – the MC open loop corner frequency has nothing to do with slew rate of an amplifier – almost all VFA opamps (other than uncompensated or de-compensated types) use dominant pole (i.e. MC) compensation with corner frequencies of just 1 or 2 Hz that are blindingly fast and even at closed loop gains of 10x or 20x will have -3 dB bandwidths of 3 to 5 MHz,  slew rates of 20 to 50 V/us and full power undistorted rail-to-rail bandwidths of 200kHz. And it is no different with power amplifiers. Slew rate and the open loop bandwidth are set completely independently of each other.

    Another fallacy is that feedback is ‘slow’ and there must be a delay around the loop, or that feedback goes multiple times around the loop. Again, on both counts completely incorrect. The loop transit time or loop  ‘flight time’ of a audio power amplifier is about 15 nanoseconds i.e. 0.000000015 seconds to go from the non-inverting input through the amplifying stages to the output and back around via the feedback network to the inverting input. It is not at all dependent on how many stages are involved – 1,2 or 5 its all around the same time give or take a few nano-seconds.  There is therefore no delay in practical terms – only phase shift which is a completely different mechanism and a property of all circuits with reactive components  – with vacuum tube amplifiers exhibiting much greater phase shifts than solid state types. This has nothing to do with the TIM mechanism mentioned above. An amplifier feedback loop is near instantaneous and occurs at relativistic speeds and should not be confused with the slewing in TIM/SID which are entirely down to a combination of  insufficient current to control the TIS compensation capacitor and the high LTP gm.

    The feedback ‘doing multiple passes around the loop’ myth grew out of an analysis carried out by Peter J Baxandall  wherein he took a simple single stage amplifier and gradually increased the feedback, monitoring the distortion as he did so. At moderate feedback levels, distortion that was originally less than objectionable 2nd and 3rds folded into higher order harmonics, albeit at lower levels,  that were objectionable. There are a number expositions on this subject (Pass and Boyk and Sussman for example) on the web wherein this phenomena is used to bolster the zero or low feedback argument, but they  use highly compromised, non-linear circuits to try to make their point which is not representative of 21st century SOTA linear amplifier design. These very basic single ended circuits would be seen in hobbyist magazines from the 1950’s and early 1960’s. If you increase the loop gain i.e. feedback, beyond 20 dB, the distortion starts to decrease dramatically, so that at 40 dB loop gain and above, you are getting massive reductions in distortion and it is well below the threshold of human hearing at < 0.01%. The ‘sour’ spot for feedback is indeed the 6 dB to 20 dB region if and only if the amplifier distortion is high in the open loop condition. If it is, either don’t apply any, or make sure you apply plenty as Putzeys points out.  Importantly, the focus on open loop linearity in modern solid state amplifiers means that even with low feedback, they are still superbly linear. Today, we start off with an amplifier that at full power open loop shows much less than 1% THD (good designs are about 0.1%) and we then apply feedback around it – we don’t start with something producing 5%, 10% or 20% which is what Colloms suggests.  Notice also that many of these low feedback/zero feedback designs only quote distortion at low power levels, or at just 1 Watt output. Further, in Pass’ article referenced above, he talks about the problem of IMD in feedback amplifiers. Again, in amplifiers that start off with low open loop distortion, IMD is a non-issue – in modern designs -100 dB down on the test tones which are at full power. Zero and low feedback amplifiers cannot match this performance.

    Amplifier Feedback: Figuring it All Out

    It took until the mid-1980’s for engineers to figure out what was going on  – although people like Bob Cordell and Bob Sickler were years ahead of the general industry curve –  and another few years for this to percolate through the design community so that only by the early 1990’s do really capable solid state amplifiers that address all of the shortcomings outlined above, become the norm. Alas, those that bought into the idea that feedback was bad, ended up corrupting the whole science of amplifier design for  large parts of the audio amplifier design community, and the press,  and a sub-culture of subjectivism emerged wherein sub-standard products – in every sense of the word – are feted as ‘jaw dropingly good’ or ‘providing fundamentally new insights’ into music never before experienced.  Reality says it’s an amplifier and simply needs to have zero distortion, zero TIM and drive any speaker load down to 2 Ohms with better than 0.2 dB flatness from 20 Hz to 20 kHz. Insofar as slew rates are concerned, the minimum figure acceptable in modern amplifiers is 1 V/us per peak output volt. Thankfully in 2017 all of these requirements are fully realizable at reasonable cost (figure on $30-$35 per stereo watt 2017 retail price on a high end class AB amplifier). In the semiconductor industry, no feedback qualms exist, and hundreds of millions of opamps working in end customer feedback loops are sold and applied every year and work flawlessly – including the ones present in the output stages of every high performance Audio DAC on the market.

    Ensuring amplifiers (and specifically VFA types) don’t suffer excessive distortion nowadays is straightforward  because the associated mechanisms are fully and completely understood. And, in 2017 we really do understand the intricacies of negative feedback as applied to audio amplifiers, which it turns out in the big scheme of things, is an exceedingly simple application of control theory science. Firstly, make the amplifier linear in the open loop condition. This is easy to do and a well designed exemplar will be well below 1% at full power open loop i.e. zero feedback and nothing like the 20% Martin Colloms mentions which is the kind of open loop distortion one would expect to see in a sub-par tube amp. Secondly, ensure the LTP is degenerated so that under a worst case full scale input transient with fast rise times (1-2 us), it still operates in the linear portion of its transfer curve and does not approach cut-off.  In most cases this will necessitate some bandwidth limiting of the input signal but in high performance designs, this will be at 300+ kHz. Third, run the front end LTP stage ‘rich’ – i.e. at a high tail current.  Combined with the degeneration this will provide a large linear operating region of 1~1.5 Volts resulting in very low open loop distortion of the LTP; the high tail current means large transient currents can be supplied into and out of the TIS integrator stage. The result is no chance of TIM ever arising. Separately, the LTP must also be well balanced – a point Self stresses in Audio Power Amplifier Design.  Fourth, use modern, high fT, sustained beta output devices like the MJL1302/1381. Finally, close the global feedback loop such that there is a minimum of 45 degrees phase margin at the unity loop gain frequency – typically about 1.5 MHz in modern amplifiers employing EF3 output stages and higher than this in EF2’s. This is not an exhaustive list –  see Douglas Self and Bob Cordell’s books on amplifier design for a more in-depth treatment of the subject.

    The Zero TIM Amplifier

    Current Feedback Amplifiers  (CFA) first became available in IC form in the early 1980’s. Their prime application in the IC realm was (and still is) in very wideband, high speed  amplifiers – video drivers, telephony systems and test and measurement gear. Their operation is not as intuitive as VFA’s and they really have only come into more widespread use in audio power amplifiers the last 10 or 15 years. Had they been around in the 1960’s, it is arguable that most of the problems discussed in the preceding paragraphs would not have arisen – perhaps only compensation design and that is a relatively easy problem to get ones head around. Matti Otala would never written about the solid state amplifier sound or TIM, and the ‘solid state’ sound would have been a thing of wonder, and not a derogatory remark hurled at some highly compromised amplifier.  Why would this have been the case? CFA’s cannot  produce TIM since the front end quiescent current is not fixed as it is in VFA’s  – it is directly related to the output voltage and the value of the feedback resistor so it is expansive, and not compressive, providing current on demand to charge the compensation capacitor – typically up to 8x the standing value in a practical audio amplifier It is not possible to get a CFA’s to slew rate limit  – something even modern VFA’s will do when the LTP runs out of steam at 150~300 kHz (this is 5~10x the figure one would encounter in a mid 1970’s amplifier by the way).  With modern output devices, CFA  power amplifiers are quite capable of reproducing a very credible 100 kHz square wave at full output power into an 8 ohm load – see  the Ovation nx-Amplifier write up for example, page 14.  Lets also be clear here, modern VFA amplifiers that apply the cures for ‘The Four Evils’ discussed above will never go into slew rate limiting with music signals – the TIM problem  that plagued this topology in the 1970’s and early 1980’s is long gone – the issue is completely and wholly solved.

     Sighted Evaluation and Subjectivism

    Studies have shown that  human auditory memory is extremely fickle. We are designed to remember the information (who, what, where etc) encoded in sounds and speech, and much less so the exact details of the frequency, harmonic content, precise timing and so forth (note that this is not the same thing as remembering or being able to play a tune or sing in tune which is covered in the cognitive neuroscience of music). Double blind and ABX tests make this abundantly clear where most individuals struggle to tell the difference between amplifiers producing 0.5% distortion and those producing only a fraction of that. Further, we may be able to tell that there is a difference on switching from one to the other, but 5 or ten minutes later, assuming the differences are not gross – which they never are anyway – the chances of a correct identification are indeed slim, and research suggests short term auditory memory of the type being discussed here is about 10 seconds. We do also know that people find higher order harmonics objectionable and lower orders (2nds and 3rds particularly) euphonic. What science also tells us is that when it comes to hearing, like sight, as a species we are susceptible to inference – we believe what is suggested or inferred we heard because we have been told, or because A looks better than B. Therefore, claims that amplifier x is better than y based on sighted testing should always be questioned.  If you want to get to the truth of an amplifier comparison, there is no other way than the scientific way and that means DBT or ABX test methodology. Now, none of this means a thing if someone’s prime motivation for buying a piece of equipment is for looks, bling factor, bragging rights or some other subjective criteria – but then we are not talking about accurate sound reproduction, but about fashion.

    The Golden Age of Audio

    Today, in both professional and consumer markets, and in the DIY community, you can find solid state feedback amplifiers featuring distortion levels of <10 parts per million at 20 kHz, slew rates of 200 V/us or more along with the ability to drive enormously difficult, reactive loads. None of these amplifiers – VFA or CFA – have a hint of TIM, SID or any other kind of distortion – they are as close as it comes to a piece of wire with gain – Peter Walker’s famous aphorism.  Over the last decade or so, newer, more in-depth understanding of the way humans perceive distortion has emerged. We know, based on research that simple THD and IMD distortion metrics may not tell us the whole truth about what kind of non-linearity we can tolerate when we listen to  a piece of music. However, it is my contention (and Douglas Self no doubt would agree) that a modern, well engineered amplifier’s distortion profile (THD, IMD, GedLee, Rnonlin etc) is orders of magnitude below the hearing threshold. There is no distortion and the amplifier is effectively ‘blameless’.  I know from my experience with a high resolution system that it is very easy to pick out CD’s and LP’s in which clipping and other distortion artefacts can be discerned that have arisen in the recording chain that in all likelihood would not be audible on a legacy system – be it solid state or tube based. We are truly living in the golden age of amplification – and it has everything to do with a thorough and in-depth understanding of feedback and compensation design at an engineering level and all of the mechanisms of non-linearity in the amplifier.

    How do these modern, well engineered audio amplifiers sound? Open, effortless, smooth, detailed and supremely accurate – sound quality and performance that could only be dreamt of 40 years ago.

  • Technical Requirements of Phono Preamplifiers by Tomlinson Holman

    Technics Direct Drive Turntable (Photograph by David Gallard)

    The two articles below were written in the 1970’s, nearly a decade before the arrival of the CD and the ‘perfect sound forever’ claim made by Philips. There was a lot of focus on phono amplifier performance at the time which it could be argued was triggered by the arrival of very high performance turntables – the Linn Sondek and Japanese Direct Drive systems from Technics for example – but there were others like Micro Seki, Thorens and so forth as well. These turntables were for the most part, quiet with low motor noise and decent quality pickup arms.


    The arrival of Quadraphonic systems required much greater bandwidths and this had to be matched with improved cartridges that offered better tracking performance and a newer, greater understanding of the electro-mechanics of the pickup itself, and in particular the stylus, emerged as a result.

    Holmans first article investigated the dynamic requirements of phono amplifiers and represented the best effort at the time – and probably still so – to understand the absolute outer limits of phono amp overload requirements. The general consensus that was cemented from this work, and that of other investigators and cartridge manufacturers at the time (Shure being chief amongst them) was that a typical phono amp should deal with peak outputs of at least 25cm/sec (5cm/sec being the nominal output). This of course does not include factors like ‘hot cartidges’ providing 6-10mV re the nominal 5mV output levels and ‘hot recordings’ where the general levels on the disc, and associated peaks, were higher than average. On top of this, overhead for the inevitable crackles and pops was also required.

    The second article presents a practical MM design which should be read in the context of the available semiconductor devices at the time.