Video: Iceland by drone and operating as TF/AE5X
FT8 - THIS is the "new" Ham Radio DXer. No skill required. Set your computer, go to dinner, come back after dessert and claim your DXCC "Participation Trophy".
The post FT8 – Lazy, Computer Scripted “Crapola” first appeared on N0UN.net.
I haven't had much time for radio these days. At this latitude, the return of the sunspots put the kibosh on my 160m dxing and with 322 (mixed, current) DXCC entities confirmed there haven't been any workable new ones available for me. My Station 2021 project has been languishing and even my existing station has fallen into disrepair. My rotator quit working in 2021 and this spring I accidentally overdrove my amp and blew something. Life was busy but sooner or later something would come along that motivated me to get back on the air. I still followed the DX news and was keeping an eye out for any new ones coming along. I followed (and donated to) the 3Y0J expedition to Bouvet Island, still on track for the end of January 2023, and also took note of the one-man operation heading for Crozet Island. When Thierry F6CUK arrived on Crozet and began operating as FT8WW over the Christmas holidays I knew that it was time to get it together.
When swapping out a couple of boards in the amplifier didn't solve the problem I determined it had to be an issue with my homebrew T/R switch and attenuator. After removing it and putting it on the bench I found that a 50 ohm resistor in the attenuator had failed. Stands to reason that accidentally pumping 100 watts into a 30 watt resistor too often would eventually lead to problems! I was already planning to replace one resistor in there to adjust for my new 10-watt IC-705 but I didn't have any spare non-inductive 50 ohm resistors. Nothing in the junk box either but I did find an old splitter/combiner set that each had a 25 ohm resistor so I put them in series and voila- problem solved. Fortunately, the antenna with the broken rotator
is pointed North over the pole so I didn't have to climb the tower in
the dark and 40 below, at least not until the Bouvet activation later this month.
Once all that and all the other minor repairs and software upgrades were done it was time make a contact! Well, that part was not going to be so easy. FT8WW was so far only using a low wire antenna . The active solar conditions would make signals very weak as the path between here (at 68 degrees North) and Crozet (nearly antipodal from here) travels straight over the North pole (which means passing through the aurora TWICE) and then all the way down the other side of the world. At least we marginally shared a grey line between midnight zulu and 0200z. That would be the best time to try.
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The entire eastern hemisphere is straight over the pole from here and Crozet is no exception. |
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Conditions were lousy all week. The elevated X-ray Flux attenuates signals like crazy up here! |
Nevertheless, I persevered. Finally, on New Year's Eve, FT8WW was on 30m around 0100z and as I watched the signals all started to get a bit stronger. Then I finally got ONE decode of FT8WW, only -18dB. Three minutes later I got another decode, this time -15dB. I started calling him. 4 periods (2 minutes) later he decoded again, this time I got both of his streams (he was using MSHV and running two carriers). Then nothing again for another 5 minutes. I could SEE his transmissions on the display but they just weren't decoding. Finally, I got another decode and it was the one I wanted to see. He was answering me! I acknowledged my report (sent RR73) and right away received an RR73 from him. Done and done. And that was it! I didn't get any more decodes after that. I only received a total of 7 transmissions from him and between calling and answering I transmitted 13 times over six minutes.
So what actually happened in that very short time span? Here is what I think was going on. The first thing was the auroral oval. Here is the NOAA Ovation forecast for that period around 0100z:
Shooting through the gap helped but the real answer was the solar wind. Like earthly wind, it "blows" fast or slow depending on the level of solar activity. The stronger the solar wind the worse the space weather is for HF radio in the polar regions. And again like the earthly wind, it also has "gusts" but these variations aren't changes in the speed. They are changes in the magnetic polarity. In the Northern auroral zone, the more negative the magnetic polarity the stronger the geomagnetic badness is. Here is the NOAA real-time solar wind plot for the time of my contact:
You can see right at the time I started getting a few decodes from FT8WW, the magnetic polarity (Bz) of the solar wind peaked in the positive direction which momentarily eased the distortion from the electromagnetism. This effect is especially pronounced on the lower HF bands. Our contact was on the 30m band which tends to share characteristics of both the lower and higher bands.
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#323 finally in the log! |
Next up at the end of January is a two-fer: Bouvet Island and Burundi, both of which I have been waiting for a chance at for a long time! The last attempt at both of those did not end well but I have a feeling that 2023 is going to be the year they finally make it into the log. Fingers crossed!
Shortly after I wrote my last annual 'DX Year' post in early 2020, things changed pretty fast once all the travel restrictions came into effect from the global pandemic. Nevertheless, despite the lack of DXpeditions, in November I finally managed to break my two year dry spell and worked JX2US on Jan Mayen Island for an all-time new one #322.
Despite its relative proximity to me, there has not been much activity from Jan Mayen in the last 10 years and I somehow managed to miss every dxpedition and the occasional operator at the Norwegian weather station there. Ken LA7GIA put in a brief appearance (only a couple of hours) from there in 2019 but was planning a much larger operation for 2021. Then Eric, LA2US, was posted to the island around the same time the dxpedition was announced, and eventually it was cancelled when Eric announced his intention to make an effort to fulfill the needs of DXers such as myself (which he did admirably!). I never did catch him on 160m as I had hoped but I did manage a few contacts on 40m and 60m during his time there.
In early February I started to notice that I had amassed almost 1000 DXCC Challenge points and a little push was all it took to confirm enough on LoTW to qualify for the award. A couple of years ago I had passed on the new plastic 5-Band DXCC Plaque (I ended up just getting the certificate and making my own 'old-school' plaque) but the new plastic DXCC Challenge plaque looks pretty nice hanging on the wall of the shack here.
I spent a lot of time on 160m this season (September through December) and picked up a dozen new ones there to bring my total up to 70 confirmed on that band. Those four months are really the only productive ones for DXing on 160m from here. I'm not sure why but long-distance 160m propagation always tanks right after the new year even though we still have lots of dark hours left. It will be interesting to see what happens next season with the increasing solar activity. I'm not expecting conditions to be very good on Top Band from under a mostly disturbed auroral oval.
That said, in keeping with the start of the new solar cycle I'm already making plans for higher bands and some other interesting activities. Stay tuned!
73
On November 16th, 2020 the reported sunspot number was zero. Since then it has rocketed up to an astonishing 83 as of November 29th. The sunspot number wasn't forecast to hit that level until 2023 but, ready or not, here it comes: solar cycle 25. The starting date of a solar cycle is actually determined retroactively and a few months ago it was determined that cycle 25 really began a year ago in December 2019. For hams, though, the real beginning of a new cycle is when the solar flux starts getting high enough for the upper HF bands to open up and starts generating stronger signals than we are used to on the middle bands. I had noticed quite a few times recently that the 12m band was open, mostly to the US west coast and Asia. Last Friday, however, even 10m was open and I made my first new contacts on that band since 2015. Just for fun, I even made a series of QSOs that started on 10m and progressed through each band all the way down to 160m (I didn't have any luck on 60m, even though I was hearing a few weak European stations). A couple of days before that I had worked a guy in Washington state on 40m FT8, off the back of my beam, only running driver power (15 watts) and I got a report from him of +23dB. I was seeing him at +31!! I can see how the effectiveness of the FT8 mode may soon become somewhat degraded as more and more powerful signals are crammed into such a tiny sliver of spectrum on each band. Some expansion of the FT8 sub bands seems very likely in the coming years.
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Ol' Sol has unexpectedly become quite active! |
Its not all fun and games, though. The more active the sun becomes, the more it tends to disrupt propagation for high-latitude stations like mine. The more active part of the cycle is marked with lots of minor disturbances that stir up the aurora and generally degrade propagation. Now the increased solar flux is making for stronger signals that can more easily break through the disturbed conditions. On days when the absorption is low and the flux is high (like last Friday) radio conditions here can be outstanding. There is also an increase in major disturbances like the little M-class solar flare that we saw this past weekend. I saw icons and colors on my propagation monitoring software that I haven't seen for years as the D-layer absorption spiked here and both the x-ray flux and proton flux climbed off the bottom of the scales where they've generally been sitting for the past few years. I blogged about how this tends to degrade the signals here back at the beginning of the last cycle and the details haven't changed at all. See here and here. An active sun makes for some very interesting effects up here in the polar region.
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Colorful, isn't it? :( |
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The dates in this table are the UTC dates which roll over in the evening here.
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Since the auroral oval is directly overhead it absorbs signals in all directions! |