May 17, 2026

My WA2EBY MOSFET Amplifier . A Homebrew Debugging Story

My WA2EBY MOSFET Amplifier

A Homebrew Debugging Story

After carefully building the WA2EBY dual-IRF510 MOSFET amplifier exactly as described in the original project article, I was disappointed to see only about 5 watts RF output on the bench. Each IRF510 was correctly biased at 10 mA, the amplifier was powered from a clean 13.8 VDC bench supply, and I even experimented with raising the supply to 19 volts. Yet the output stubbornly remained low. Even more suspicious was the current draw  over 2.5 amps on key-down , clear evidence that something in the amplifier was consuming power without converting it efficiently into RF.

The troubleshooting process began methodically. I verified the input attenuator pad values and wiring, checked all toroid windings against the published turns count and core types, and confirmed correct phasing on the transformers. Using an oscilloscope, I examined the RF signal splitting and combining networks; both appeared symmetrical and healthy. To eliminate any possibility of relay losses or T/R switching problems, I bypassed the relay entirely and connected the amplifier directly to a 50-ohm dummy load. Still, the meter stubbornly indicated only 5 watts output.

At that stage, suspicion naturally shifted toward the output transformer T3. In RF power amplifiers, excessive current draw combined with low RF output often points toward a partially shorted winding or a single shorted turn in the output transformer , effectively turning RF energy into heat instead of useful output power. I was already mentally preparing to rewind the toroid.

Before tearing the amplifier apart, however, I decided to perform one more measurement. I quickly built a simple RF probe and checked the RF voltage directly at both MOSFET drains during transmit. The result was surprising: both drains showed a healthy RF voltage swing of approximately 13 volts peak during key-down. That measurement changed everything. The RF voltage was clearly there, meaning the amplifier stage itself was functioning properly. The problem was not the amplifier,it was the wattmeter.

I replaced the suspect power meter with another unit, and instantly the amplifier came alive: approximately  +/- 20  watts RF output with only 1 watt of drive at 13.8 volts. Current consumption now made sense, efficiency looked reasonable for an IRF510 design, and the MOSFETs warmed normally without any signs of thermal stress or instability.

The final conclusion was both satisfying and educational. The WA2EBY amplifier design itself was solid all along; the real fault was a misleading RF power meter. Many inexpensive through-line wattmeters, especially older CB-style meters or low-cost HF meters can be wildly inaccurate at low power levels, frequency-dependent, or even introduce mismatch problems that affect measurements. A simple RF probe turned out to be the most trustworthy diagnostic tool on the bench.

One important lesson from this project is never to rely entirely on a single instrument when troubleshooting RF equipment. Cross-checking measurements with an RF probe, oscilloscope, dummy load, or second wattmeter can save hours of frustration and unnecessary rebuilding.

Now that the amplifier is delivering a solid  +/- 20 watts output, the project moves into its next stage. The immediate goals are building an RF sampler for safe monitoring with a PC-based oscilloscope and constructing proper low-pass filters for clean 40m and 20m operation. After that comes the most rewarding phase of any homebrew project real over-the-air testing. There is something deeply satisfying about watching a pile of components evolve into a fully functional on-air RF amplifier built with your own hands.

 

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Brainstorming ideas and layout concepts for a Manhattan-style RF circuit board before beginning final construction. Careful component placement, short RF paths, solid grounding, and logical stage separation are critical in Manhattan construction, especially for broadband HF power amplifiers. Much of the early design effort focused on minimizing stray inductance, maintaining symmetry in the push-pull layout, and ensuring adequate space for transformers, heatsinking, and future modifications.


 
 
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I introduced a modification to the original WA2EBY amplifier design to improve bias stability and overall push-pull balance. The original zener-diode bias arrangement was replaced with a dedicated linear voltage regulator based on an L7805CVA, providing a stable 5 VDC supply to both MOSFET bias networks. This produced cleaner and more thermally stable biasing of the IRF510 devices, improving amplifier consistency during operation.


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Before installing the IRF510 MOSFETs, I performed a complete signal-path verification using a signal generator and oscilloscope. Temporary 0.01 µF capacitors were installed across the gate and drain device positions, effectively coupling the RF signal through the entire amplifier chain without the transistors fitted. This allowed the signal to pass from the bifilar input splitter transformer, through the gate and drain PCB pads, into the output combiner transformer and bifilar RF choke network, and finally to the RF output connector.

Oscilloscope measurements taken at both gate connections showed equal-amplitude RF waveforms with an accurate 180-degree phase relationship, confirming correct operation of the push-pull input splitter. Repeating the measurements at the drain connections produced the same balanced out-of-phase signals, verifying proper transformer phasing and symmetry through the output combiner stage. Final checks at the secondary of the output transformer confirmed a clean, properly combined RF waveform. This pre-installation test fully validated the splitter and combiner circuitry before the IRF510 devices were soldered into the amplifier.



The RF power stage of the amplifier is built around a pair of IRF510 MOSFETs operating in push-pull configuration. Although originally intended as switching devices, the IRF510s have proven to be inexpensive, rugged, and very capable performers in low-voltage HF linear amplifiers when properly biased and matched. Each device was mounted to a large finned aluminum heatsink using insulating pads, shoulder washers, and thermal compound to ensure effective heat transfer while maintaining electrical isolation from the chassis.

Under normal SSB operation, the heatsink remains only moderately warm, even at approximately +/- 20 watts RF output. However, to improve long-term thermal reliability during extended key-down or digital-mode operation, I added a small 12 VDC cooling fan to provide continuous airflow across the heatsink. Particular attention was also given to the physical layout: the MOSFETs were mounted as close as possible to the output transformer and combiner network in order to minimize drain lead length, reduce stray inductance, and maintain good RF symmetry within the push-pull stage.


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                    A short clip with bad focusing and shaking picture frame 😁😂

 

April 22, 2026

May 24, 2022

DXCC Silver Award and Bronze Award ....

DXCC Silver Award,for working 100 unique DXCC entities via QO-100 satellite.



 https://qo100dx.club/

December 28, 2021

ARISS SSTV Award

 


Hello ST2NH,
This ARISS SSTV event is dedicated to "Present ISS Space Agency Contributions to Lunar Exploration, Past, Present and Future.” The SSTV slides provide some historical context to several missions, some not well known, that significantly contributed to Lunar Exploration either from a technology or scientific perspective. General intention of the ARISS SSTV slides is to provide aspects to the observers that may not be known before and could offer a base for own investigations on space history.

Amateur Radio on the International Space Station (ARISS) is a cooperative venture of international amateur radio societies and the space agencies that support the International Space Station (ISS). The primary goal of ARISS is to promote exploration of science, technology, engineering, the arts, and mathematics topics. ARISS does this by organizing scheduled contacts via amateur radio between crew members aboard the ISS and students. Before and during these radio contacts, students, educators, parents, and communities take part in hands-on learning activities tied to space, space technologies, and amateur radio.
More info:

The ARISS Ad-hoc Award Committee:
- Oliver DG6BCE (chair)
- Armand SP3QFE
- Francesco IK0WGF
- Bruce W6WW
- Shizuo JE1MUI
- Darin VE3OIJ
- Ian VE9IM

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Greetings - Slawek SQ3OOK
ARISS SSTV Award Manager

June 26, 2021

ARISS SSTV Award

Hello Nader Omer -ST2NH,
This time the SSTV images series is dedicated to radio amateur astronauts and cosmonauts and their activities on board of the Space Shuttle, Mir Space station and International Space Station. The ARISS SSTV Award presents  three special people.
On the left: Musa Manarov U2MIR - Russian cosmonaut who launched amateur radio equipment on board of the Mir space station. He made the first amateur radio communication in October 1988. Consequently, the MAREX (Mir Amateur Radio Experiment) and MIREX (Mir International Amateur radio EXperiment) programs were created.
Center: Sergey Krikalyov U5MIR - Russian cosmonaut, member of the Expedition 1 on the International Space Station. In November 2000 launched an amateur radio station on board of the ISS. This event was the beginning of ARISS (Amateur Radio on the International Space Station) school contacts. Many cosmonauts and astronauts also conducted unscheduled radio communications, which made a lot of joy for the radio amateurs around the world.

On the right: American Owen Garriott W5LFL who was the first astronaut and amateur radio operator to take with him on the space shuttle Columbia (STS-9 mission in 1983) amateur radio equipment and conducted radio communications with radio amateurs on Earth. Hereby the SAREX program (Shuttle Amateur Radio Experiment later called Space Amateur Radio Experiment) was created.

Greetings - Slawek SQ3OOK
ARISS SSTV Award Manager


#
 
Photo received from ISS over Sudan  




June 23, 2021

Mir-Sat-1 Received Over Africa

 

Mir-Sat-1 (Mauritius Imagery and Radio Communication Satellite -1) is the first Mauritian satellite. It is a 1U cubesat deployed from the ISS Tuesday at 10.55 UTC by JAXA .At a very low pass telemetry received and decoded over Khartoum.Congratulation #MIRSAT1 team.
 

 

May 7, 2021

JIDXM Friendship award 2020.

I'm so honored and grateful to be the recipient the beautiful plaque of JIDXM Friendship award 2020.

 


 

April 24, 2021

Radio amateur G3YJO on BBC Radio 4

 

Radio amateur Professor Sir Martin Sweeting G3YJO, was the guest on the Radio 4 show The Life Scientific that was broadcast on Tuesday, April 20.

Martin Sweeting G3YJO pioneered the original SmallSats revolutions with the UOSAT-1 and UOSAT-2 spacecraft that carried amateur radio payloads and launched in the early 1980’s. They led to the founding of Surrey Satellite Technology Ltd (SSTL) of which he is Executive Chairman.

You can listen to, or download, an MP3 recording of the BBC show which mentions amateur radio and AMSAT from the BBC website at https://bbc.co.uk/programmes/m000v7pb

 

 

 read more @ https://amsat-uk.org/

March 30, 2021

DIY-1 Satellite RTTY telemetry received over Africa !

Mode rtty 100 BD 7N2 telemetry of  DIY-1 satellite  received and decoded  Orbit #79 over Africa. .Object Y(47954) Congratulation DIY-1 diysatellite.com
 
  YRYRYRIsRYRYRYRYRYRY$$COn>K00364R940,02-mc3c3U124,06.50,16,3d]4kl6-%