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Topband: 160 Meter Propagation

To: "a Topband COL" <topband@contesting.com>
Subject: Topband: 160 Meter Propagation
From: "Thomas F. Giella KN4LF" <kn4lf@earthlink.net>
Reply-to: "Thomas F. Giella KN4LF" <kn4lf@earthlink.net>
Date: Mon, 12 Jan 2009 13:49:42 -0500
List-post: <topband@contesting.com">mailto:topband@contesting.com>
Carl K9LA is correct in his assertion that change in height of the 
ionosphere in the equatorial region during solar minimum does not translate 
to a change in the height of the mid and high latitude ionosphere. However 
at and near solar minimum the mid and high latitude D layer of the 
ionosphere at mesosphere altitude cools approximately 2 degrees C, contracts 
in thickness and signal absorption in the layer increases.

Also a solar flux in the mid 100's is necessary for routine stable formation 
of the E Valley/F Layer ducting mechanism. Therefore formation of the duct 
is less prevalent at the bottom of solar cycle and long haul propagation 
poorer at solar minimum.

73 & GUD DX,
Thomas F. Giella, KN4LF
Lakeland, FL, USA
kn4lf@arrl.net

KN4LF Daily Solar Space Weather & Geomagnetic Data Archive: 
http://www.kn4lf.com/kn4lf5.htm 

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