To: | "topband@contesting.com" <topband@contesting.com> |
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Subject: | Topband: weird propagation |
From: | "k9la@frontier.com" <k9la@frontier.com> |
Reply-to: | "k9la@frontier.com" <k9la@frontier.com> |
Date: | Mon, 10 Dec 2012 13:11:15 -0800 (PST) |
List-post: | <topband@contesting.com">mailto:topband@contesting.com> |
It would be good to pay heed to N7DF's e-mail about possible improved propagation when the IMF turns south. Two examples that come to mind are skewed paths (reflection/refraction from the intense ionization at the equatorward edge of the auroral oval) and enhanced paths right before the K index spikes up (possibly due to an improved electron density valley - giving ducting). One quick correction, though - the electrons that precipitate into the high-latitude atmosphere when the K index is elevated are those that were trapped in the Earth's magnetosphere - they don't come directly from the Sun (the electrons in the solar wind are way too low in energy). Carl K9LA _______________________________________________ Topband reflector - topband@contesting.com |
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