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Spectral Purity of a QRP Transmitter Driver Amplifier

Introduction

Some months ago, we reported on a commercially available, off-the-shelf 3W MMIC amplifier [1] to be used as part of a transmitter driver with receive bypass [2]. It was our intent to use as many COTS components as possible to simplify and shorten the construction timeline for a 10-band QRP SSB transceiver. An inexpensive amplifier that is widely available through AliExpress [3] is advertised to work from 2 to 700 MHz, which is more than adequate for our requirements (Figure 1. The gain of this amplifier was 45 dB.

Figure 1. Wideband 3W Shortwave Amplifier. This wideband shortwave amplifier is advertised as being capable of 3W output power. Our plan is to drive it to 1W so that our 10 dB gain power amplifier can be driven to 10W. The 3W MMIC amplifier works from 2 to 700 MHz, which is more than adequate for high-frequency use. The measured gain of the amplifier is 45 dB. Power dissipation is greatly improved by the application of diamond heatsink compound between the circuit board and the heatsink. The amplifier is operated at +9 VDC to reduce its thermal dissipation. Please click on the Figure to open it in a new window.

Since our last report, some changes have been made to the original circuit to reduce its gain, increase its stability, improve its spectral purity, and enhance its receive isolation. The 3W MMIC amplifier is of single-ended construction. Consequently, there is no cancellation of even (or odd) harmonics of the signal being amplified, and it turns out that when operated at +9 VDC, or even +13.8 VDC, the MMIC amplifier is quite nonlinear.

This article discusses all of the circuit improvements. In particular, the spectral purity of the transmitter driver amplifier is demonstrated. Use of the single-ended amplifier requires the addition of another low-pass filter bank [4] between the driver amplifier circuit and the transmitter, in addition to the one that is provided at the transmitter output.

Low Pass Filter Bank

Thanks to Hans Summers, G0UPL, at QRP Labs [5] for providing bare boards so that my original filter bank, consisting of 10 low-pass filters, Figure 2, that employed the Ed Wetherhold (SK), W3NQN, design [6] could be built and tested.

As we will soon demonstrate, an additional low-pass filter bank results in greatly improved spectral purity. Since an additional low-pass filter bank had not yet been built, we have employed the transmitter low-pass filter bank, as required, for measurements in this paper.

Figure 2. Ten-Band Low Pass Filter Bank on Its Interconnect Backplane. The 40m low-pass filter that was used to process the 7.1 MHz signal is located four filters from the left. All of the filters employ the Ed Wetherhold (SK), W3NQN, design. The bare boards for these filters were obtained from Hans Summers, G0UPL, at QRP Labs. Readily available Arduino relay boards were used throughout. Since these are power relays, the relay contacts are DC-wetted through bias-T’s, not shown, to reduce the contact resistance. The QRP Labs filters employ a single DPDT relay per filter band, whereas my filters employ two separate SPDT relays per band. Please click on the Figure to open it in a new window.

Revised Transmitter Driver With Receive Bypass Schematic
A revised schematic diagram is shown in Figure 3. Changes to the original design [7] include the removal of relay optical isolation for push-to-talk with the deletion of its attendant FET driver, and the addition of relay grounding for the receive bypass path during transmit. An additional relay pair was added to perform the grounding function. A 3 dB attenuator was added to the driver amplifier input to improve the amplifier stability and to reduce its gain. A photo of the completed design with the 3 dB coaxial attenuator installed is shown in Figure 4. If there is sufficient isolation, the 3 dB attenuator will be added to the back of the circuit card. The revised design uses a separate power management circuit board to supply +13.8 VDC to the +9 VDC onboard voltage regulator during transmit. This greatly simplifies the circuit board.

Figure 3. Revised Driver Schematic Diagram. The schematic has been simplified when compared to the previous iteration. The logic input has been removed so that the module may be keyed by the power management module during transmit. The receive bypass path is grounded at both ends during transmit. Power is supplied to the driver amplifier by an LM317 adjustable voltage regulator that receives power from the power management module during transmit. Please click on the Figure to open it in a new window.

Figure 4. The Completed Driver Amplifier Board As Revised. The black driver amplifier heatsink is visible. The lower relay pair provides the transmit/receive function. The upper relay pair grounds each end of the semi-rigid coax receive path during transmit. The LM317 adjustable regulator regulates +13.8 VDC from the power management module down to +9 VDC for use by the driver amplifier. This reduces the amplifier power dissipation. Please click on the Figure to open it in a new window.

The measured spectrum of the amplified 7.1 MHz signal without low-pass filtering is shown in Figure 5. The amplifier has been driven to 1W. Since the amplifier is single-ended, the even harmonics have not been suppressed, and the 2nd harmonic is barely 10 dB below the carrier. It is evident that this MMIC amplifier is nonlinear.

Figure 5. Spectral Purity of a 7.1 MHz Signal Prior to Low Pass Filtering. Even and odd harmonics are visible because the driver is single-ended, not push-pull. A push-pull amplifier would provide some attenuation of the even harmonics but not the odd harmonics. The spectrum analyzer display shows the 7.1 MHz carrier at 0 dBm. Since the spectrum analyzer input is padded by 30 dB, 0 dBm corresponds to 1W. The second harmonic is barely -10 dBc for this drive level. Please click on the Figure to open it in a new window.

The measured spectrum of the amplified 7.1 MHz signal with low-pass filtering is shown in Figure 6. The amplifier drive level was left unchanged from the previous measurement. With the low-pass filter applied to the signal, both the even and odd harmonics have been suppressed by nearly 60 dB.

Figure 6. Spectral Purity of a 7.1 MHz Signal After Low Pass Filtering. The even and odd harmonic content of the 7.1 MHz signal has been suppressed by nearly 60 dB. The implication is that the W3NQN 40m low-pass filter is doing a great job of attenuating the 2nd harmonic and higher-order products. About 1 dB of signal attenuation is observed after passing it through the low-pass filter, as one might expect. As in the previous figure, 0 dBm corresponds to 1W due to the presence of a 30 dB pad at the spectrum analyzer input. Please click on the Figure to open it in a new window.

Summary

We have described revisions to the original circuit design that result in a much simpler driver amplifier that retains a receive bypass function. The revised circuit is keyed from the power management module on transmit so that it does not have to be keyed directly from push-to-talk.

The spectral purity of the amplified signal before and after low-pass filtering has been demonstrated. Higher order harmonics are attenuated by nearly 60 dB by Ed Wetherhold, W3NQN, low-pass filters.

The low-pass filter bank that was used for spectral evaluation is at the transmitter output. Consequently, another low-pass filter kit has been ordered from QRP Labs that will cover 5 of the 10 bands. Another kit will be ordered at a later date to cover the remaining 5 bands. Since these low-pass filters come without an integral transistor interface for microprocessor I/O, one will have to be built.

A short YouTube video [8] of a test may be viewed at https://youtu.be/nTQk9CR1W9w

References

[1] 2 MHz-700 MHZ 3W HF VHF UHF FM Transmitter RF Power Amplifier For Radio https://www.aliexpress.us/item/3256807249993037.html?spm=a2g0o.order_list.order_list_main.25.1adb1802la12vX&gatewayAdapt=glo2usa

[2] Blustine, Martin, RF Driver Amplifier With Receive Bypass, N1FD, Nov. 1, 2025. https://www.n1fd.org/2025/11/01/rf-driver-amplifier/

[3] AliExpress, op. cit.

[4] QRP Labs, Ultimate Relay-Switched LPF Kit, https://qrp-labs.com/ultimatelpf.html

[5] QRP Labs, Low Pass Filter Kit, https://qrp-labs.com/lpfkit.html

[6] Wetherhold, Ed, W3NQN, Second-Harmonic Optimized Low-Pass Filters, QST, Feb. 1999, pp. 44 – 46.

https://www.arrl.org/files/file/Technology/tis/info/pdf/9902044.pdf

[7] Blustine, Martin, op. cit.

[8] YouTube Test Video, https://youtu.be/nTQk9CR1W9w

Disclaimers

This circuit design is provided for informational and educational purposes only and is supplied “as is” and without warranties of any kind, express, implied, or statutory. No representations or warranties are made regarding the accuracy, adequacy, completeness, legality, reliability, or usefulness of this information, either in isolation or in the aggregate. This circuit design may contain links to or information based on external sources or third-party content. Endorsement and responsibility for the accuracy or reliability of such third-party information or for the content of any linked websites are not taken.

Hamilton Stewart, A Friend and and a Great Mentor, SK

We received some very sad news recently. A long-time member and supporter of the Nashua Area Radio Society and Amateur Radio, Hamilton Stewart, K1HMS, has become a silent key.

I first met Hamilton at a NARS exam session where he earned his  Extra Class license, by passing the Technician, General, and Extra exams all in one session. He became active with NARS and began contributing almost immediately. Hamilton made many contributions to NARS.

Hamilton served as an instructor for our license classes and presented some of the most difficult topics in a way students could understand. He was famous for his Yagi antenna demos, which will be missed at our license classes.

Hamilton explaining a design of his at Project Night

Hamilton was an engineer’s engineer – one of the best that I have had the pleasure to know. He would always take the time to patiently explain the most difficult ideas in simple terms, helping them master technical concepts. When members need help repairing a radio or another piece of gear, Hamilton helps them get back on the air. His workshop was impressive, and he really knew how to use his gear.

Pierce, K1FOP and Hamilton, K1HMS Testing CW Stations
Hamilton, K1HMS Testing CW Stations

Hamilton loved Field Day and served as co-chairman. He was always there to help us build our stations and to operate them. We would find a way to pitch in and help with whatever the team needed to succeed at Field Day. He was always team-focused.

Hamilton was also a past Treasurer of NARS, and served on our non-profit incorporation/501(c)(3) committee

Hamilton loved to mentor and wrote many articles on our website to help newer folks learn about Amateur Radio station building, operating, and electronics. You can find his contributions in this area here.

It was a privilege to have known Hamilton. I have the highest respect for him as a person. Even when he was very sick and fighting to regain his health, he found time to continue contributing to NARS’ educational work and to share his knowledge and mentor others. I will miss him very much.

You can find information on the final arrangements and his obituary here.

Fred, AB1OC

Winter Field Day 2026 6 Band Multiplier Prep

It’s that time again, and Winter Field Day will be here before you know it.   Planning is well underway.  Once again, Fred and Anita have opened their home and shack for Winter Field Day operation, and we will be operating QRP (10 Watts or less), which is a score multiplier.   This year a new multiplier category was added to operate on an additional six (6) bands to make it a total of twelve (12) bands.

This past weekend, Fred, AB1OC, and I tested six additional bands with overwhelming success from his QTH to a mobile location I operated, acting as the roving team.   They say sharing is caring, so I thought I would write a blog about how we got here and the tools that helped along the way.

Winter Field Day Rules

All the rules are available here; the three specific ones to note are as follows.

Bands: All Amateur bands may be used except 12, 17, 30, and 60 meters. To qualify as a band worked, at least one valid, two-way QSO must have taken place on the said band during the event.

Make three contacts on at least six (6) different bands: Conditions may change throughout an event. Log operations on at least six different bands by making a minimum of three contacts per band. You should be able to accomplish this objective by utilizing HF, VHF, and UHF frequencies. Don’t forget about 1.25 meters (220)!  It’s an excellent band for local emergencies. OM x6

Make three contacts on at least twelve (12) different bands: Was six too easy?  You may have to pull out your microwave equipment to achieve this one. Log operations on at least twelve different bands by making a minimum of three contacts per band. The six bands from the previous objective count toward this one. OM x6

The first 6 bands are the typical contesting bands: 10m, 15m, 20m, 40m, 80m, 160m.   No problem for the AB1OC shack.   The other 6 bands will be 6M, 2M, 1.25M, 70CM, 33cm, and 23cm. Here are the challenges.

1) We can’t use a repeater.  Simplex only.
2) Since it is VHF and UHF, we need a decent Line of Sight (LOS) with little or no trees to cause interference.
3) We are running QRP, so distance is a factor.
4) We need equipment for the 33cm and 23cm bands.
5) We need at least three contacts.

VHF/UHF Roving

As part of the planning and to address these problems, we decided to send a Roving team to serve as the club’s three contacts.  Rules dictate that contacts must be outside a 1000 ft circle from the Field Day base of operation.    I started by using Google Earth Pro, setting the coordinates for AB1OC QTH and using the circle ruler to determine our 1000-foot perimeter.  The two circles represent the VFH and HF Towers’ location.

Based on the knowledge of the surrounding area, we chose the location southeast of the intersection of RT 122 and Blood Road.

Then we used the HeyWhatsThat website to generate ideas for where we could get a signal based on the topology.

And the Scadacore LOS website to confirm the topology.

Both are very simple to use.

We looked at a few other locations, but tested this site first and had great success, so we called it a win for Winter Field Day.

Another interesting tool is Radio Mobile. This software is a popular, free radio propagation simulation software for planning wireless networks (especially for amateur radio).

They offer both web and download versions.   The download version has more features and is worth a peek.   This YouTube video is a great tutorial that walks you through installing your first propagation map.   Could be a Tech Night session!

I started loading all the variables, but since our field test was successful, I didn’t complete the simulation.

Rover Radios and Antennas

For equipment, Fred’s SDR can handle all the required bands, and his antennas are up to the task.

15 Band SDR Remote Gateway at AB1OC
15 Band SDR Remote Gateway at AB1OC

Here is what we are working with for antennas at the base station:

  • 6m Loop Yagi (14.1 dBi)
  • 1.25m Yagi (11.9 dBi)
  • 2m Circularly Polarized Yagi (14.4 dBic)
  • 70cm Circularly Polarized Yagi (18.9 dBic)
  • 33cm Yagi (15.2 dBi)
  • 23cm Yagi (17 dBi)

Even at the QRP level, the gain and ability to point the antennas helped overcome distance issues.  For the roving team location, I used a 33 cm Alinco HT with a short radial, a 23 cm Alinco HT also with a short radial, a Kenwood HT for 2M, 70cm, and 1.25m from Fred’s stash—finally, a Yaesu 891 with ATAS 120 Antenna for 6M as part of my mobile rig.

K1BER Mobile Station
K1BER Mobile Station
HTs Covering 2m - 23cm
HTs Covering 2m – 23cm

Specifically, we tested the following:

2M        146.415 MHz             Vertically Polarized

1.25M  223.500 MHz           Horizontally Polarized

70CM   445.925 MHz           Vertically Polarized

33cm   902.500 MHz             Horizontally Polarized

23cm   1296.700 MHz          Horizontally Polarized.

6M        50.150 MHz SSB      Horizontally Polarized

As we cycled through the bands and our QSO, the signal reports were between 57 and 59 at both ends.  Our 5 challenges were easily overcome.

With a month to go before Winter Field Day, we are ready and excited to have fun, learn, and earn points.   We are still looking for volunteer rovers, which is an excellent opportunity for Techs.   Don’t worry if you’re new; you will have help.   If you are interested in participating in any part of Winter Field Day or in planning, please contact us or join the planning meeting.

Dave, K1BER

Radio Amateurs Developing Skills Worldwide