Is just looking for abnormalities in the wider pattern good enough, or is this not the correct way to try to decipher the WSPR data? Should I limit the results to those below 3000km in distance, or is it okay to include multi-hop transmissions as well?
Thank you so much for reading through my email, any help, comments, or observations is much appreciated, I will include more information that I couldn't fit into this message below,
Thanks
Isobel Smith,
73 de M5DUK
Dear Isobel,
I would think that to be a very difficult task. There are no more space shuttle flights or launches, and when there were, there was not a wide and deep WSPR network, with the current level of multiband WSPR transmitters (often Turn Island Systems ‘wsprsonde’ units), nor multiband WSPR receivers (‘wsprdaemon’, often based on the Rx888 SDR device.)
The last shuttle flew in July of 2011.
73,
George K9TRV
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The following graph shows the 20m band on the proceeding day of the launch (05.11.2025), the day of the launch (06.11.2025), and the following day (07.11.2025).
The highlighted section on the 06/11/2025 after the launch (21:13) looks much more sparse when compared to the previous day, and the following day. That a change was observed, at roughly the time we expected it to occur, looked initially promising.
(I again reached the message limit so I will split this over yet another email).
However, according to the paper "First Observations of Large Scale Traveling Ionospheric Disturbances Using Automated Amateur Radio Receiving Networks" (https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2022GL097879 ), you should look at distances on the 20m band below 3000km to avoid transmissions with multi-hops.
Therefore, when looking at the data for the 20m band again, with the distance reduced to below 3000km, you can see that the distances around 500km tend to increase on the 31.10.2025, compared to the day preceding and after it.
To make the data readable, the tx.loc was reduced to only include the maidenhead locators DM, CM, DL, DN.

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