Wednesday, June 21, 2017

Odd differences between two (nearly) identical PV systems

I've had my 18-panel (two groups of 9) PV (solar) electric system in service for about a year and recently I decided to expand it a bit after realizing that I could do so, myself, for roughly $1/watt, after tax incentives.  An so it was done, with a bit of help from a friend of mine who is better at bending conduit than I:  Another inverter and 18 more solar panels were set on the roof - all done using materials and techniques equal to or better than that which was originally done in terms of both quality and safety.

Adding to the old system:

The older inverter, a SunnyBoy SB 5000-TL, is rated for a nominal 5kW and with its 18 panels, 9 of each located on opposite faces of my east/west facing roof (the ridge line precisely oriented to true north-south) would, in real life, produce more than 3900 watts for only an hour or so around "local noon" on late spring/early fall summer days that were both exquisitely clear and very cool (e.g. below 70F, 21C).  I decided that the new inverter need not be a 5kW unit so I chose the newer - and significantly less expensive SunnyBoy SB3.8 - an inverter nominally rated at 3.8kW.  The rated efficiencies of the two inverters were pretty much identical - both in the 97% range.
Figure 1:
The installed 3.8 kW inverter in operation with the 2kW
"SPS" (Secure Power System) island power outlet shown below.
Click on the image for a larger version.

One reason for choosing this lower-power inverter was to stay within the bounds of the rating of my main house distribution panel.  My older inverter, being rated for 5kW was (theoretically) capable of putting 22-25 amps onto the panel's bus, so a 30 amp breaker was used on that branch circuit while the new inverter, capable of about 16 amps needed only a 20 amp breaker.  This combined, theoretical maximum of 50 amps (breaker current ratings, not actual, real-world current from the inverters and their panels!) was within the "120% rule" of my 125 amp distribution panel with its 100 amp main breaker:  120% of 125 amps is 150 amps, so my ability to (theoretically) pull 100 amps from the utility and the combined capacity of the two inverters (again, theoretically - not real-world) being 50 amps was within this rating.

Comment:  The highest total power that power that I have seen from my system has been about 8000 watts - 3900 watts from the SB3.8 and just over 4100 watts from the SB 5000 for a maximum of about 36 amps at 220 volts (abnormally low line voltage!) or about 33 amps total with a more typical 240 volt feed-in - well under the "50 amp" maximum.

For the new panels I installed eighteen 295 watt Solarworld units - a slight upgrade over the older 285 watt Suniva modules already in place. In my calculations I determined that even with the new panels having approximately 3.5% more rated output (e.g. a peak of 5310 watts versus 5130 watts, assuming ideal temperature and illumination - the latter being impossible with the roof angles) that the new inverter would "clip" (e.g. it would hit its maximum output power while the panels were capable of even more power) only a few 10s of days per year - and this would occur for only an hour or so at most on each occasion.  Since the ostensibly "oversized" panel array would be producing commensurately more power at times other than peak as well, I was not concerned about this occasional "clipping".

What was expected:

The two sets of panels, old and new, are located on the same roof with the old array being higher, nearer the ridge line and the new being just below.  In my situation I get a bit of shading in the morning on the east side, and a slight amount in the very late afternoon/evening in mid summer on west side and the geometry of the trees that do this cause the shading of both the new and old systems to be almost identical.

With this in mind, I would have expected the two systems to behave nearly identically.

But they don't!

Differences in produced power:

Having the ability to obtain graphs of each system over the course of a day I was surprised when the production of the two, while similar, showed some interesting differences as the chart below shows. 

Figure 2:
The two systems, with nearly identical PV arrays.  The production of the older SB5000 inverter with the eighteen 285 watt panels is represented by the blue line while the newer SB3.8 inverter with eighteen 295 watt panels is represented by the red line:  Each system has nine east-facing panels and nine west-facing panels.  The dips in the graph are due to loss of solar irradiance due to clouds.  Because the data for this graph is collected every 15 minutes, some of the fine detail is lost so the "dip" in production at about 1:45PM was probably deeper than shown.
The total production of the SB3.8 system (red line) for the day was 27.3kWh while that of the SB5000TL system (blue line) was 25.4kWh - a difference of about 7% overall.
Click on the image for a larger version.
In this graph the blue line is the older SB5000TL inverter and the red line is the newer SB3.8 inverter.  Ideally, one would expect that that the newer inverter, with its 295 watt panels, would be just a few percent higher than the older inverter with its 285 watt panels, but the difference, particularly during the peak hours, is closer to 10%, particularly during the peak times when there is no shading at all.

What might be the cause of this difference?
Figure 3:
 The two parallel east-facing arrays, the older one being closer to
the (north-south) peak of the roof.
Click on the image for a larger version.

Several possible explanations come to mind:
  1. The new panels are producing significantly more than their official ratings.  A few percent would seem likely, but 10%?
  2. The older panels have degraded more than expected in the year that they have been in service.
  3. The two manufacturers rate their panels differently.
  4. There may be thermal differences.  The "new" panels are lower on the roof and it is possible that the air being pulled in from the bottom by convection is cooler when it passes by the new panels, being warmer by the time it gets to the "old" panels.  If we take at face value that 3.5% of the 10% difference is due to the rating - leaving 6.5% difference unaccounted, this would need only about a 16C (39F) average panel temperature difference, but the temperature differences do not appear to be that large!
  5. The new panels don't heat up in the sun as much as the old.  The new panels, in the interstitial gap between individual cells and around the edges are white while the old panels are completely black, possibly reducing the amount of heating.  Again, there doesn't seem to be a 16C (39F) difference.
  6. The new inverter is better at optimizing the power from the panels than the old one.
It's a bit difficult to make absolute measurements, but in the case of #2, the possibility of the "old" panels degrading, I think that I can rule that out.  In comparing the peak production days for 2016 and 2017, both of which occurred in early May (a result of the combination of reasonably long days and cool temperatures) the best peak was about the same - approximately 28.25kWh on the "old" system even after I'd installed the "new" panels on the east side.

I suspect that it is a combination of several of the above factors, probably excluding #2, but I have no real way of knowing the amount of contribution of each.  What is surprising to me is that I have yet to see any obvious clipping on the new system on the production graphs even though I have "caught" it pegged at about 3920 watts on several occasions during local noon, so it seems that my calculation of "several dozen of hours" per year where this might happen is about right.

I'll continue to monitor the absolute and relative performance of the two sets of panels to see how they track over time.

* * *

Update - June, 2018:

The differences noted above still persist.  In comparing the overall power production results between this year and last, there are no obvious changes in the two systems.


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Tuesday, June 13, 2017

Adding a useful signal strength indication to an old, inexpensive handie-talkie for transmitter hunting

A field strength meter is a very handy tool for locating a transmitter, but a sensitive field strength meter by itself has some limitations as it will respond to practically any RF signal that enters its input.  This has the effect of limiting the effective sensitivity of the field strength meter, as any nearby RF source (or even ones far away, if the meter is sensitive enough...) will effectively mask the desired signal if it is weaker than these "background" signals.
Figure 1:
The modified Icom IC-2A/T HT with a broadband
field strength meter paired with the AD8307-based field
strength meter mentioned and linked in the article, below.
Click on the image for a larger version.

This property can be mitigated somewhat by preceding the input of the meter with a simple tuned RF stage and, in most cases, this is adequate for finding (very) nearby transmitters.  A simple tuned circuit does have its limitations:
  • It is only broadly selective.  A simple, single-tuned filter will have a response encompassing several percent (at best) of the operating frequency.  This means that sensitive meter preceded by a 2 meter filter will respond to nearly any signal near or within to the 2 meter band.
  • A very narrow filter can be tricky to tune.  This isn't usually too much of a problem as one can peak on the desired signal (if it is close enough to register) or use your own transmitter (on the same or nearby frequency) to provide a source of signal on which the filter may be tuned.
  • The filter does not usually enhance the absolute (weak signal) sensitivity unless an amplifier is used with it.
An obvious approach to solving this problem is to use a receiver, but while many FM receivers have "S-meters" on them, very few of them have meters that are truly useful over a very wide dynamic range, most firmly "pegging" even on relatively modest signals, making them nearly unusable if the signal is any stronger than "medium weak".  While an adjustable attenuator (such as a step attenuator or offset attenuator) may be used, the range of the radio's S-meter itself may be so limited that it is difficult to manage the observation of the meter and adjusting the signal level to maintain an "on-scale" reading.

Another possibility is to modify an existing receiver so that an external signal level meter with much greater range may be connected.

Picking a receiver:

When I decided to take this approach I began looking for a 2 meter (the primary band of interest) receiver with these properties:
  • It had to be cheap.  No need to explain this one!
  • It had to be synthesized.  It's very helpful to be able to change frequencies.
  • Having a 10.7 MHz IF was preferable.  The reasons for this will become apparent.
  • It had to have enough room inside it to allow the addition of some extra circuitry to allow "picking off" the IF signal.  After all, that's the entire point of this exercise.
  • It had to be easy to use.  Because one may not use this receiver too often, it's best not to pick something overly complicated and would require a manual to remind one how to do even the simplest of tasks.
  • The radio would still be a radio.  Another goal of the modification was that the radio had to work exactly as it was originally designed after you were done - that is, you could still use it as a transceiver!
Based on a combination of past familiarity with various 2 meter HTs and looking at prices on Ebay, at least three possibilities sprang to mind:
  • The Henry Tempo S-1.  This is a very basic 2 meter-only radio and was the very first synthesized HT available in the U.S.  One disadvantage is that, by default, it uses a threaded antenna connection rather than a more-standard BNC connector and would thus require the user to install one to allow it to be used with other types of antennas.  Another disadvantage is that it has a built-in non-removable battery.  It's power supply voltage is limited to under 11 volts.  (The later Tempo S-15 has fewer of these disadvantages and may be better suited for this application, but I am not too familiar with it.)
  • The Kenwood TH-21.  This, too, is a very basic 2 meter-only radio.  It uses a strange RCA (e.g. phono) like threaded connector, but this mates with easily-available RCA-BNC adapters.  Its disadvantage is that it is small enough that the added circuitry may not fit inside.  It, too, has a distinct limitation on its power supply voltage range and requires about 10 volts.
  • The Icom IC-2A/T.  This basic radio was, at one time, one of the most popular 2 meter HTs which means that there are still plenty of them around.  It can operate directly on 12-15 volts, has a standard BNC antenna connector, and has plenty of room inside the case for the addition of a small circuit.  (The "T" suffix indicates that it has a DTMF numeric keypad.  The "non-T" version such as the IC-2A is a bit less common, but would work just fine for this application.)
Each of these radios is a thumbwheel-switch tuned, synthesized, plain-vanilla radio. I chose the Icom IC-2AT (it is also the most common) and obtained one on Ebay for about $40 (including accessories) and another $24 bought a clone of an IC-8, an 8-cell alkaline battery holder (from Batteries America) that is normally populated with 2.5 amp-hour NiMH AA cells.  With its squelched receive current of around 20 milliamps I will often use this radio as a "listen around the house" radio since it will run for days and days!

"Why not use one of those cheap Chinese radios?"

Upon reading this you may be thinking "why spend $$$ on an ancient radio when you can buy a cheap chinese radio that has lots of features for $30-ish?"

The reason is that these radios have neither a user-available "S" meter with good dynamic range or an accessible IF (Intermediate Frequency) stage.  Because these radios are, in effect, direct conversion with DSP magic occurring on-chip, there is absolutely nowhere that one could connect an external meter - because that signal simply does not exist!

While many of these "single-chip" radios do have some built-in S-meter circuitry, the manufacturers of these radios have, for whatever reason, not made it available to the user - at least not in a format that would be particularly useful for transmitter hunting.

Unfortunately these radios can overload quite easily when near a strong signal.  This property - and the fact that they use audio processing that can vary based on signal quality - make many of these radios generally unsuitable for direction-finding!
Modifying the IC-2A/T (and circuit descriptions):

This radio is the largest of those mentioned above and has a reasonable amount of extra room inside its case for the addition of the few small circuits needed to complete the modification.  When done, this modification does not, in any way, affect otherwise normal operation of the radio:  It can still be used as it was designed!

An added IF buffer amplifier:

This radio uses the Motorola MC3357 (or an equivalent such as the MP5071) as the IF/demodulator.  This chip takes the 10.7 MHz IF from the front-end mixer and 1st IF amplifier stages and converts it to a lower IF (455 kHz) for further filtering and limiting and it is then demodulated using a quadrature detector.  Unfortunately, the MC3357 lacks an RSSI (Receive Signal Strength Indicator) circuit - which also explains why this radio doesn't have an S-meter.  Since we were planning to feed a sample of the IF from this receiver into our field strength meter, anyway, this isn't too much of a problem.

Figure 2:
The source-follower amplifier tacked atop the IF amplifier chip.
Click on the image for a larger version.
We actually have a choice to two different IFs:  10.7 MHz and 455 kHz.  At first glance, the 455 kHz might seem to be a better choice as it has additionally amplified and it is at a lower frequency - but there's a problem:  It compresses easily.  Monitoring the 455 kHz line, one can easily "see" signals in the microvolt range, but by the time you get a signal that's in the -60 dBm range or so, this signal path is already starting to go into compression.  This is a serious problem as -60 dBm is about the strength that one gets from a 100 watt 2 meter transmitter that is clear line-of-sight at about 20 miles (about 30km) distant, using unity-gain antennas on each end.  What this means is that if we were to use this signal tap, we might still be a fair distance away from the transmitter we were seeking when its signal saturated the meter.

The other choice is to tap the signal at the 10.7 MHz point, before it goes into the MC3357.  This signal, not having been amplified as much as the 455 kHz signal, does not begin to saturate until the input reaches about -40 dBm or so, reaching full saturation by about -35 dBm.  Given our example, above, -35 to -40dBm is roughly equivalent to a line-of-sight 100 watt 2 meter transmitter at 1-3 miles (approx. 1.6-5km) - which means that we'll get much closer before the signal path saturates - but we can easily deal with that as we'll discuss shortly.

One point of concern here was the fact that at this point, the signal has less filtering than the 455 kHz, with the latter going through a "sharper" bandpass filter.  While the filtering at 10.7 MHz is a bit broader, the 4 poles of the crystal filter do attenuate  a signal 20 kHz away by at least 30 dB - so unless there's another very strong signal on this adjacent channel, it's not likely that there will be a problem.  As it turns out, the slightly "broader" response of the 10.7 MHz crystal filters is conducive to "offset tuning" - that is, deliberately tuning the radio off-frequency to reduce the signal level reading when you are nearby the transmitter being sought and it starts to saturate the IF stages.

To tap this signal without otherwise affecting the performance of the receiver requires a simple buffer amplifier, and a JFET source-follower does the job nicely (see figure 6, below for the diagram).  Consisting of only 6 components (two resistors, three capacitors and an MPF102 JFET - practically any N-channel JFET will do) this circuit is simply tack-soldered directly onto the MC3357 as shown in figures 2 and 3.  This circuit very effectively isolates the (more or less) 50 ohm load of the field strength meter from the high-impedance 10.7 MHz input to the MC3357 and it does so while only drawing about 700 microamps, which is only 3-4% of the radio's total current when it is squelched.

Figure 3:
A wider view of the modifications to the radio.
Click on the image for a larger version.
As can be seen from the pictures (figure 2 and 3) all of the required connections were made directly to the pins of the IC itself, with the 330 pF input capacitor connecting directly to pin 16.  The supply voltage is pulled from pin 4, and pins 12 and/or 15 are used for the ground connection. 

A word of warning:  Care should be taken when soldering directly to the pins of this (or any) IC to avoid damage.  It is a good idea to scrape the pin clean of oxide and use a hot soldering iron so that the connection can be made very quickly.  Excess heat and/or force on the pin can destroy the IC!  It's not that this IC is particularly fragile, but this is care that should be taken.

Getting the IF signal outside the radio:

The next challenge was getting our sampled 10.7 MHz IF energy out of the radio's case.  While it may be possible to install another connector on the radio somewhere, it's easiest to use an existing connector - such as the microphone jack.

One of the goals of these modifications was to retain complete function as if it were a stock radio, so I wanted to be sure that the microphone jack would still work as designed, so I needed to multiplex both the microphone audio (and keying) and the IF onto the tip of the microphone connector as I wasn't really planning to use the signal meter and a remote microphone at the same time.  Because of the very large difference in frequencies (audio versus 10.7 MHz) it is very easy to separate the two using capacitors and an inductor:  The 10.7 MHz IF signal is passed directly to the connector with a series capacitor (such as 100pF) while the 10.7 MHz IF signal is blocked from the radio's internal microphone/PTT line with a small choke:  Anything from 4.7uH to 100uH will work fine.
Figure 4:
The modifications at the microphone jack.
Click on the image for a larger version.

The buffered IF signal is conducted to the microphone jack using some small coaxial cable:  RG-174 type will work, but I found some slightly smaller coax in a junked VCR.  To make the connections, the two screws on the side of the HT's frame were removed, allowing it to "hinge" open, giving easy access to the microphone connector.  The existing microphone wire connected to the "tip" connection was removed and the choke was placed in series with it, with the combination insulated with some heat-shrinkable tubing.

The coax from the buffer amp was then connected directly to the "tip" of the microphone connector.  One possible coax routing is shown in Figure 4 but note that this routing prevents the two halves of the chassis from being fully opened in the future unless it is disconnected from one end.  If this bothers you, a longer cable can be routed so that it follows along the hinge and then over to the buffer circuit.  Note:  It is important to use shielded cable for this connection as the cable is likely to be routed past the components "earlier" in the IF strip and instability could result if there is coupling.

Interfacing with the Field Strength meter:

Using RG-174 type coaxial cable, an adapter/interface cable was constructed with a 2.5mm connector on one end and a BNC on the other.  One important point is that a small series capacitor (0.001uF) is required in this line somewhere as a DC block on the microphone connector:  The IC-2A/T (like most HTs) detects a "key down" condition on the microphone by detecting a current flow on the microphone line and this series capacitor prevents current from flowing through the 50 ohm input termination on the field strength meter and "keying" the radio.

Dealing with L.O. leakage:

As soon as it was constructed I observed that even with no signal, the field strength meter showed a weak signal (about -60 to -65 dBm) present whenever the receiver was turned on, effectively reducing sensitivity by 20-25 dB.  As I suspected when I first noticed it, this signal was coming from two places:
  • The VHF local oscillator.  On the IC-2A/T, this oscillator operates 10.7 MHz lower than the receive frequency.  In other words, tuned to 146.520 MHz, the local oscillator is running at 135.82 MHz.
  • The 2nd IF local oscillator.  On the IC-2A/T this oscillator operates at 10.245 MHz - 455 kHz below the 10.7 MHz IF as part of the conversion to the second IF.
The magnitude of each of these signals was about the same, roughly -65 dBm or so.  The VHF local oscillator would be very easy to get rid of -  A very simple lowpass filter (consisting of a single capacitor and inductor) would adequately suppress it - but the 10.245 MHz signal poses a problem as it is too close to 10.7 MHz to be easily attenuated enough by a very simple L/C filter without affecting it.

Figure 5:
The inline 10.7 MHz bandpass using filter using a ceramic
filter.  The diagram for this may be seen in the upper-right
corner of Figure 6, below.
Click on the image for a larger version.
Fortunately, with the IF being 10.7 MHz, we have another (cheap!) option:  A 10.7 MHz ceramic IF filter.  These filters are ubiquitous, being used in nearly every FM broadcast receiver made since the 80s, so if you have a junked FM broadcast receiver kicking around, you'll likely have one or more of these in them.  Even if you don't have junk with a ceramic filter in it, they are relatively cheap ($1-$2) and readily available from many mail-order outlets.  This filter is shown in the upper-right corner of the diagram in Figure 6, below.

The precise type of filter is not important as they will typically have a bandpass that is between 150 kHz and 300 kHz wide (depending on the application) at their -6 dB points and will easily attenuate the 10.245 MHz local oscillator signal by at least 30 dB.  With this bandwidth it is possible to use a 10.7 MHz filter (which, themselves, vary in exact center frequency) for some of the "close - but not exact" IF's that one can often find near 10.7 MHz like 10.695 or 10.75 MHz.  The only "gotcha" with these ceramic filters is that their input/output impedances are typically in the 300 ohm area and require a (very simple) matching network (an inductor and capacitor) on the input and output to interface them with a 50 ohm system.  The values used for matching are not critical and the inductor, ideally around 1.8uH, could be anything from 1.5 to 2.2 uH without much impact of performance other than a very slight change in insertion loss.

While this filter could have been crammed into the radio I was concerned that the L.O. leakage might find its way into the connector somehow, bypassing the filter.  Instead, this circuit was constructed "dead bug" on a small scrap of circuit board material with sides, "potted" in thermoset ("hot melt") glue and covered with electrical tape, heat shrink tubing or "plastic dip" compound, with the entire circuit installed in the middle of the coax line (making a "lump.")  Alternatively, this filter could have been installed within the field strength meter itself, either on its own connector or sharing the main connector and being switchable in/out of the circuit.

Figure 6:
The diagram, drawn in the 1980s Icom style, showing the modified circuity and details of the added source-follower JFET amplifier (in the dashed-line box) along with the 10.7 MHz bandpass filter (upper-right) that is built into the cable.
Click on the image for a larger version.
With this additional filtering the L.O. leakage is reduced to a level below the detection threshold of the field strength meter, allowing sub-microvolt signals to be detected by the meter/radio combination.

Operation and use:

When using this system, I simply clip the radio to my belt and adjust it so that I can listen to what is going on.

There's approximately 30 dB of processing gain between the antenna to the 10.7 MHz IF output - that is, a -100 dBm signal on the antenna on 2 meters will show up as a -70 dBm signal at 10.7 MHz.  What this means is that sub-microvolt signals are just detectable at the bottom end of the range of the Field Strength meter.  From a distance, a simple gain antenna such as a 3-element "Tape Measure Yagi" (see the article "Tape Measure Beam Optimized for Direction Finding - link) will establish a bearing, the antenna's gain providing both an effective signal boost of about 7dB (compared to an isotropic) and directivity.

While driving about looking for a signal I use a multi-antenna (so-called) "Doppler" type system with four antennas being electrically rotated to get the general bearings with the modified IC-2AT being the receiver in that system.  With the field strength meter connected I can hear its audio tone representing the signal strength without need to look at it.  As I near the signal source and the strength increases, I have both the directional indication and the rising pitch of the tone as dual confirmation that I am approaching it.

The major advantage of using the HT as tunable "front end" of the field strength meter means that the meter has greatly enhanced selectability and sensitivity - but this is not without cost:  As noted before, this detection system will begin to saturate at about -40 dBm, fully saturating above -35 dBm - which is a "moderately strong" signal.  In "hidden-T" terms, it will "peg" when within a hundred feet or so of a 100 mW transmitter with a mediocre antenna.

When the signals become this strong, you can do one of several things:
  • Detune the receiver by 5, 10, 15 or even 20 kHz.  This will reduce the sensitivity by moving the signal slightly out of the passband of the 10.7 MHz IF filters.  This is usually a very simple and effective technique, although heavy modulation can cause the signal strength readings to vary.
  • Add attenuation to the front-end of the receiver.  The plastic case of the IC-2A/T is quite "leaky" in terms of RF ingress, but it is good enough for a step attenuator on the antenna lead to work nicely and will thus extend usable range to at least -10dBm dBm.  I use a switchable step attenuator for this and I have found that I can drive to the location (house, yard, park) where the transmitter is located and still have sufficient adjustment range.
  • When you are really close (e.g. 10s of yards/meters) to the transmitter being sought you can forgo the receiver altogether, connecting the antenna directly to the field strength meter!
If you want to be really fancy, you can build the 10.7 MHz bandpass filter and add switches to the field strength meter so that you can switch 20 dB of attenuation in and out as well as routing the signal either to the receiver, or to the field strength meter using a resistive or hybrid splitter to make sure that the receiver gets some signal from the antenna even when the field strength meter is connected to the antenna.

What to use as the field-strength meter:

The field strength meter used is one based on the Analog Devices AD8307 which is useful from below 1 MHz to over 500 MHz, providing a nice, logarithmic output over a range that goes below -70dBm to above +10dBm.  It is, however, broad as the proverbial "barn door" and the combination of this fact and that its sensitivity of "only" -70dBm is nowhere near enough to be useful with weak signals - especially if there are any other radio transmitters nearby - including radio and TV stations within a few 10s of miles/kilometers.  The integration of this broadband detector with the narrowband, tuneable receiver IF along with its gain makes for a complete system useful for signals that range from weak to strong.

The description of an audible field-strength meter may be found on the web page of the Utah Amateur Radio club in another article that I wrote, linked here:  Wide Dynamic Range Field Strength Meter - link.  One of the key elements of this circuit is that it includes an audio oscillator with a pitch that increases in proportion with the dB indication on the meter, allowing "eyes-off" assessment of the signal strength - very useful while one is walking about or in a vehicle.

There are also other web pages that describe the construction of an AD8307-based field strength meter (look for the "W7ZOI power meter" as a basis for this type of circuit) - and you can even buy pre-assembled boards on EvilBay (search for "AD8307 field strength meter" or "AD8307 power metetr").  The downside of most of these is that they do not include an audible signal strength indication to allow "eyes off" use, but this circuit could be easily added, adapted from that in the link above.

Another circuit worth considering is the venerable NE/SA605 or 615 which is, itself, a stand-alone receiver.  Of interest in this application is its "RSSI" (Receive Signal Strength Indicator) circuit which has both good sensitivity, is perfectly suited for use at 10.7 MHz,  has a nice logarithmic response and a wide dynamic range - nearly as much as the AD8307.  Exactly how one would use just the RSSI pin of this chip is beyond the scope of this article, but information on doing this may be found on the web in articles such as:
  • NXP Application note AN1996 - link (see figure 13, page 19 for an example using the RSSI function only)

Additional comments:
  • At first, I considered using the earphone jack for interfacing to the 10.7 MHz IF, but quickly realized that this would complicate things if I wanted to connect something to the jack (such as pair of headphones or a Doppler unit!) while DFing.  I decided that I was unlikely to be needing to use an external microphone while I was looking for a transmitter!
  • I haven't tried it, but these modifications should be possible with the 222 MHz and 440 MHz versions (the IC3 and IC4) of this radio - not to mention other radios of this type.
  • Although not extremely stable, you can listen to SSB and CW transmissions with the modified IC-2A/T by connecting a general-coverage/HF receiver to the 10.7 MHz IF output and tuning that receiver to about 10.7 MHz, +/- a few kHz.  Signals may be slightly "warbly" - but they should be easily copyable!
Finally, if you aren't able to build such a system and/or don't mind spending the money and you are interested in what is possibly the best receiver/signal strength meter combination device available, look at the VK3YNG Foxhunt Sniffer - link.  This integrates a 2 meter receiver (also capable of tuning the 121.5 MHz "ELT" frequency range) and a signal strength indicator capable of registering from less than -120dBm to well over +10dBm with an audible tone.

Comment:  This article is an edited/updated version of one that I posted on the Utah Amateur Radio Club site (link) a while ago.


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