The “official” kick-off for contesting season is really CQ WW SSB at the end of October, but many of us clear our throats here in August with a set of North American QSO Party events sponsored by the National Contest Journal. We have CW and SSB in August; the RTTY event was mid-July. See the August Contest Notes below for some opportunities to “warm up” for contest season this fall.
Exchange: 10-10 members: Name + 10-10 number + SPC, non-members give a zero for their 10-10 number (same format)
[Remember SPC is State, Province, or Country]
This might be an interesting contest, if only to see whether 10m comes alive. Go to a band like 10m and listen nearly anytime during the low point in the solar cycle and you’ll likely hear nothing at all. But, put a big contest on the air and suddenly 10m is alive with activity. (Maybe not, but you might be surprised how often this is true!) Check out the rules, of course, as I always recommend, but this seems like a pretty easy contest. Remember, the 10m band has more spectrum than all the other HF bands put together! Everybody gets to spread out. It makes for a very relaxing experience. Try it!
Hey, look at that! Lots of overlap with the 10-10 contest. And, it has almost the same exchange (the 10-10 contest wants a zero between your name and SPC). Here’s yet another change to work on your WAS award.
At risk of repeating myself, if you are new to contesting, or if you just like to do something relaxing, and you can speak at all, this contest is your speed. Put some states in the log!
Hawaii QSO Party [0400Z Aug 24 to 0400Z Aug 26]
Exchange: HI: RS(T) + QTH, non-HI: RS(T) + SPC
I’m highlighting this contest because for many of us moping our way through the doldrums of this solar cycle Hawaii is a tough place to reach. It is the world’s most isolated island chain, after all. So, a whole contest chock-full of Hawaiians sounds like a great opportunity to put them in the log. Remember, Hawaii isn’t just a state, it’s a DXCC entity, too. Two-Fer!
That’s All for This Month
Remember that contesting.com always has great stuff, including the complete list of contests for this month (and every month). Even if you’re a little shy, even if you feel inexperienced, even if you don’t think contesting is for you, get on the air, listen for a bit, then make a few QSOs, and see if it doesn’t put a smile on your face.
It’s difficult to believe that half of 2019 is already behind us. We’re only a few months away from the start of the 2019-2020 contesting season. As the NARS Field Day totals have shown, there is still plenty of good propagation out there so don’t believe all that talk about the bands being dead. The bands, especially during contests, often have a surprising amount of activity. Take advantage of it.
13 Colonies
The height of Summer brings us things that are an equal amount of fun and competition. Though not a contest, per se, the 13 Colonies Special Event will bring you pile-ups worthy of CQ WW. If you’ve not found some slots to work already, check out the NARS club 13 Colonies effort and get involved.
A Couple of Highlights
I’ll start with one of my favorite contests of July: the RSGB IOTA Islands on the Air contest.
Exchange: RS(T) + Serial No. + IOTA No. (if applicable)
I have often done this contest from the Boston Harbor Islands (NA-148), either Georges Island or camping on Lovells Island. There may be a club field-trip to Georges for a Saturday 6-hour effort. Keep a watch on the Forums section of the website for more information.
I’ve done this contest from the top of Mount Wachusett and it is a ton of fun. Of course New Hampshire has a bunch of mountains to try your luck. Walk up the slope and get SOTA points, too!
Take your 6m and 2m all band radio and do SSB, FM, and CW from a mountaintop and rack up the grid squares. This is a really fun way to spend an afternoon.
Exchange: Name + state (DC/province/country) for North America. Just name for those outside North America.
The National Contest Journal holds QSO parties and sprints for each mode twice a year. These contests are fun because they are not jam-packed with people. If your new to a mode, or if you just want to sharpen your skills, these are great contests to try.
Until Next Time
Summer is a good time to catch up with family, see a few baseball games [Go Spinners!], or do that outside project you’ve been putting off. But, if you do have some time, get on the air!
The RockMite is a very small, but complete, transceiver. We covered most of the radio’s components in the first three parts, but it is worth reviewing. Instead of just rehashing the previous text, we should explore those ideas from a different angle.
A great place to start any investigation is asking the question, “What problem are we trying to solve?” This is a very relevant question when dissecting a radio. Answering questions like, “What does this particular thing do?” and “Why is this here?” helps us not only understand the results better, but I contend they help us remember the answers better, too.
In part one we explored the receiver. The problem to be solved there was “How do I take energy at radio frequencies and turn them into sounds my ears can hear?” We did that with an oscillator (discussed later) and a mixer, combining two frequencies to produce the four frequencies from two A and B:A, B, A+B, and A-B. It was the A-B (the free-running oscillator and the received signal) that combined to result in a frequency in the audible range.
In part two we looked at the user interface (UI) of the device, what little of it there is. There were a couple of points there, however, including problems solved like “Can I have an iambic keyer? and “How can we operate this radio on multiple frequencies?” and “How do we turn on the transmitter?” All of these things were controlled by the small Microchip PIC processor.
In part three we looked at the oscillator and saw how the output of the oscillator fed into the mixer for the receiver, and how it also fed forward into the transmitter section of the radio to be discussed today. The magic of the varactor tuning diode gave us a second frequency for the radio that could be directly controlled by the simple microprocessor.
In this last article on the RockMite we will look at the final stages of the transmitter, and specifically the filtering between the transmitter and the antenna.
The Schematic
Below is a schematic for the RockMite that we’ve been using for these articles.
Schematic for the RockMite transceiver (from QRPMe.com)
The particular part of the schematic we are interested in today is highlighted in the following:
We will discuss each part in turn.
Final Amplifier Stage
The final amplifier Q6 in the RockMite is the versatile and ubiquitous 2N2222A in the nice metal can. We put a heat-sink on the can to keep the transistor cool. The transistor amplifier is fed by a capacitive couple to the first stage amplifier Q5. (Q5 is fed by the oscillator.)
Q6 is connected to Vdc via an inductor, and to ground when the switching transistor Q3 is turned on. The Q3 transistor is connected to the transmit-receive (T-R) line on the PIC processor and when it powers the gate a connection is made through Q3 to ground, activating Q6. When Q3 is not turned on Q6 is quiet and the receiver can operate.
Filtering
Again, we should begin a discussion with “What problem are we trying to solve?” The final amplifier Q6 is solving the problem of “How do we get our signal amplified to a reasonable level?” Q6 does a nice job with this and the RockMite puts out somewhere around a half-of-a-Watt of power.
But, the trouble with generating signals like this is we also generate unwanted signals as harmonics. So, the question becomes, “How can we pass through the signal we want, but none of the harmonics?”
A good answer to that question is a low-pass filter. Filter design is far beyond the scope of this brief article, but it might be useful to walk through a simple filter design exercise.
I went to rf-tools.com and found a filter design tool. I’ve captured a screen-shot of my work creating a low-pass filter for a 40m radio. That appears below.
I used some straight-forward parameters for our filter. I want the cutoff frequency to be above 40m so I chose 8 MHz. I left the Passband Ripple (dB) to the value defaulted by the program. And, I left the impedance in-and-out be 50 Ohms. Finally, I told it to choose values that exist in parts catalogs (“standard” values).
The program generated the schematic near the top, and chose appropriate values for the parts to create the intended filter. The response curve of the filter appears in the graph below the schematic.
Examine the schematic for the transmitter section, especially the components just before the antenna connection. We have five parts of interest L2, L3, C15, C17, and C19. (Note that C16 and C18 are not populated and are reserved for future versions of the kit.) These five components are the low-pass filter for the radio. The specific parts to be used depend upon the band we want. The values for a 40m band radio are:
L2 and L3: 1 µH
C15, C19: 470 pF
C17: 1000 pF
If you check, these values from the RockMite design are very close to the values selected by our filter design program. (The designers of the RockMite, K1SWL and W1REX, are likely a lot smarter about filter design than I am, so we’ll take it on faith that their value selections are better.) The differences are small: L2 and L4 have 1.0 µH in the RockMite design; the corresponding parts in our designed filter are 1.3 µH. C15 and C19 in the RockMite design match perfectly to the corresponding parts in our filter’s design. And C17 is 1000 pF in the RockMite design, and 820 pF in our filter design. These are all very close.
The “Insertion Loss and Return Loss” graph for our filter’s design estimates the filter’s performance. The blue line that runs from upper left to the lower right corner shows the loss for a given frequency. Our first harmonic will be at 14 MHz. The line intersects 14 MHz at 27.6 dB, meaning any outputted frequency entering the filter will be diminished by 27.6 dB. Our second harmonic at 21 MHz is reduced by nearly 48 dB.
Why do we care about keeping harmonics down?
The FCC demands it.
97.307 Emission standards.
(d) For transmitters installed after January 1, 2003, the mean power of any spurious emission from a station transmitter or external RF power amplifier transmitting on a frequency below 30 MHz must be at least 43 dB below the mean power of the fundamental emission. For transmitters installed on or before January 1, 2003, the mean power of any spurious emission from a station transmitter or external RF power amplifier transmitting on a frequency below 30 MHz must not exceed 50 mW and must be at least 40 dB below the mean power of the fundamental emission. For a transmitter of mean power less than 5 W installed on or before January 1, 2003, the attenuation must be at least 30 dB. A transmitter built before April 15, 1977, or first marketed before January 1, 1978, is exempt from this requirement.
So, just guessing, the values in the RockMite’s design for the components probably make the roll-off just a little steeper. Our circuit designed in the on the RF Tools website did a good job, though. If we were really worried about it we could have put another few components in. Check out the following 7th order low-pass filter. At our first harmonic 14 MHz, our harmonics are down over 47 dB. That more than satisfies the FCC.
Wrapping Up
One of the things I love about QRP and low-power operating is I can (almost) understand all the components in the radio. I know what most things do, and I even understand why most things work. I’m still learning.
This is the last installment of the RockMite teardown. I hope you’ve enjoyed it!
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