Once again we did M/2 from the station of my friend Vlad VE3JM. His station is similar in size to mine and he does extremely well from there. He is also a better contest operator, especially 2BSIQ, so he almost always beats me when we enter contests in the same category. This year we have a full complement of 5 operators; last year there was just the two of us when the others cancelled due to a ferocious snowstorm. This year's storm didn't impede travel even for those driving up from the Toronto area.
This edition of the ARRL DX CW contest made it clear that we are past the peak of cycle 25. Our score was lower with 5 operators than with 2 of us in 2025. Geomagnetic disturbances are up and the sunspot count is down. The latter was actually zero (0) on Monday. We are unlikely to see many contest records broken for the next half dozen years.
Although I didn't remember to take a snapshot soon enough after the contest the Sunday K-index chart tells the tale. It wasn't good. Not terrible, but definitely not good. That said, there was a lot of DX on offer and many fantastic runs.
Although conditions affect everybody, which ought to burden competitors equally, opportunities do not skew equitably when you move a few hundred kilometers near the auroral zone. That noticably affected us, though to what degree is difficult to say. Of course our challenges pale in comparison to those even farther north. This is not an excuse but an explanation for regional variation.
This is the setup we used. From left to right are Dave VE3KG on the in-band station, Nick VE3EY on one run station and Les VE3NNT on the other run station. In the background you can see that Vlad has an outstanding set of high power filters and triplexers from VA6AM. We still had interaction issues, especially harmonics that regularly plague CW. You will regularly find yourself near those harmonics due to simple arithmetic.
The in-band station has no filters other than what the receiver can provide, and by the separation and polarity of the antenna. The in-band antenna is a multi-band (no trap) 40-to-10 meter vertical about 100 meters from the various towers. The in-band station has no amplifier since the proximity of the antennas does not allow use of higher power without impacting the run stations. Interference in the other direction is acceptable but often problematic.
This was my first experience operating with an in-band station and I was impressed despite the inter-station interference and limited power and antenna. Many contacts and some multipliers were logged. This is important since many stations mostly run so this may be the only way to work them. It also allows the run station to keep running, and eager operators can get in there and contribute.
The interlocks worked well (DXLog) and it was easy for the operators to learn how to coordinate. I'm tempted to add this capability to my own station. Techniques to reduce interference were discussed among the operators.
In-band capability is not a universal solution. The run stations, with higher power and superior antennas, did a lot of the work. Also, the in-band station could not be manned full time. One reason was that the in-band station had no antenna for 80 or 160 meters. The worse conditions on the second day further limited its effectiveness due to weaker signals. Working spotted stations on the run radios risked loss of the run frequency and wasting time with busted spots, both human and skimmer generated. There were a lot of busted spots that wasted our time.
Propagation played a critical role in our competitiveness. We were at a disadvantage compared to those to the south and therefore farther from the auroral oval. That's not a complaint, just a feature of where we live. It happens whenever conditions are disturbed or marginal.
The following is a brief description of several interesting propagation factors that we experienced, both pro and con:
- On Sunday morning when 10 meter propagation to Europe was poor, one of our operators (VE3EY) turned the 7-element yagi east, and then a little further south. Signals from Europe strengthened and the rate shot up. That was a smart move. I've known that this can happen for more than 40 years yet never suspected skew path this weekend. It is a common occurrence during solar minima years that Europeans on 10 meter peak towards the sun. Whether scatter or true skew path it is worth turning the yagi to check for this phenomenon. More southerly areas get more sunlight and therefore have a higher MUF.
- This weekend provided another lesson in paying less attention to SSN (sunspot number) and more to SFI (10.7 cm solar flux index). On Sunday the SSN was 0. Even so the high bands were open. SFI is a better proxy for ionospheric MUF.
- The first night and to a lesser extent the second, 40 meters stayed open to Europe until long after their sunrise. This often happens when geomagnetic conditions are quiet and the solar flux is low. Signals get weaker as the sun rises in Europe but remain workable. Unlike in CQ WW they stay on the low bands rather than moving to the high bands since they can only work North Americans. My rate was very good for longer than one might think possible.
- 20 meters opened for about one hour overnight to Europe at the same time 40 was still going strong after their sunrise. Sometimes it happens and sometimes not, so you must pay attention. After that hour the band died and didn't reopen until a little before our sunrise.
- 80 meter conditions to Japan and the north Pacific were better than expected. Overnight we worked quite a few stations. Signals were weak but many stations were workable. We usually can't work east Asia until our sunrise enhancement. Several welcome multipliers were logged on 80 this way.
Despite excellent activity our results were down. That mirrors the experience of others. Propagation played a part as did participation. CW in particular is less popular with younger generations, especially in North America. Outside VE/W there is less interest in this contest since it is more of a QSO party than a global contest. For those on the other side of the globe there is little to work, so why would they bother. We should be thankful to those that participate and make the contest what it is.
It must also be noted that not everyone taking part is familiar with the rules. We had many US callers and even a few from Canada. They are of course worth zero points. As for dupes, it is better to work them than to try to explain the rules to each caller or to ignore or admonish them. I would never want to discourage their enthusiasm. If they encounter rudeness these casual operators won't call you in the next contest when the points they give you will contribute to your success.
As usual, we used the online scoreboard. I rarely use it when I operate alone, but it was interesting to see how our nearest competitors were doing. In ARRL DX we are on an equal footing with US participants so the comparisons are meaningful. In some respects watching the scoreboard was discouraging since there was little we could do about what we witnessed. We were already motivated and working hard on our score as I am sure were the others.
I consider the scoreboard a needless distraction which is why I have yet to use it for my single op contest efforts. It wouldn't change what I do. Many others feel differently. However I see its value to non-participants that want to follow the competitors. In the future I may post my score even though I am unlikely to look at the scoreboard during the contest. Perhaps my opinion will change in the future.
I'll close with a note about technology and training. Most of us don't use DXLog in our own stations. I only use it when operating at Vlad's station. As I have with N1MM, his station automation systems are tightly integrated with DXLog. There is a learning curve. A crib sheet with common commands isn't really adequate since these software packages are feature rich and can behave in ways that neophytes can't predict or deal with. All we could do was fumble or call out for help when in trouble.
The only solution is pre-contest training. That means using and studying the software before the contest weekend. That is in addition to learning about the antennas and selection process in a large station. There is a lot to digest and use effectively, or at least with minimal friction. It is worth consideration in advance of your next multi-op contest, whether at your station or elsewhere.


























