Image: IRF/Kiruna |
Aurora visibility at 23:30UT. Image: NOAA. |
At 21:14UT, 8P9HA appeared and, over the coming few minutes built up to -20dB SNR/2500Hz.
Shortly thereafter, HC6PE appeared. He built up to a remarkable -08dB SNR/2500Hz at 22:10UT. Keep in mind the geometry of his station and mine, relative to the sunlit atmosphere, no part of which has been visible from Wales at this point for maybe 2 hours or so:
Path to HC6PE and terminator at 22:10UT, 2018 December 01. Image with permission, DX Atlas. |
My RX spots at the times relevant to this post. |
Even more intriguingly, K6MCS appears shortly thereafter, but only briefly. You may recall this post concerning K6MCS making an identical sort of appearance in early January this year.
The paths are interesting to consider. The model for the aurora shows a small patch further to the south in the Atlantic than the main oval. These appear regularly, so they don't seem to be artefacts of the model, though that is a possibility that needs checking out with NOAA. If this patch is real, it might indicate a limited area that could have facilitated propagation to HC6PE.
The path for K6MCS seems to go through dense regions of the aurora. Clearly, with so many (as of this morning, 300) WSPR stations active on 14MHz, there remains something to explain about how that station seems to make a regular appearance under disturbed conditions.
As always, any ideas welcome under comments!
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