[NZ4O Spaceweather] Discussion Of Solar Space & Geomagnetic Weather Conditions
Thomas F Giella NZ4O
nz4o at tampabay.rr.com
Mon Oct 1 09:48:41 EDT 2012
Published on Monday October 01, 2012 at 1330 UTC. Valid for the next 24
hours.
1.) DISCUSSION OF SOLAR, SPACE & GEOMAGNETIC WEATHER CONDITIONS THAT CAN
IMPACT MF & HF RADIO WAVE PROPAGATION IN A NEGATIVE MANNER-
A coronal mass ejection (CME) may arrive at earth's geomagnetic field later
today causing geomagnetic storming that would lower the maximum useable
frequency (MUF) and negatively impact radio wave propagation conditions on
10 and 12 meters.
Per the guess cast I made above yesterday morning, the CME arrived early
this morning UTC and produced a geomagnetic storm peaking at a Kp of 7,
which is "strong" geomagnetic storming. The storm is now subsiding but could
continue to bring intermittent unsettled (Kp-3) to active (Kp-4) geomagnetic
conditions for the remainder of the day.
As of 1300 UTC there are still significant impediments to good radio wave
propagation on the HF bands of 20-10 meters as far as solar, space and
geomagnetic weather, as it will take the rest of the day today or more for
the ionosphere to recover after the strong (Kp-7) geomagnetic storm. Also as
the excessive number of electrons from the strong (Kp-7) geomagnetic storm
continue to precipitate down our planets magnetic field lines through the
mid latitudes and then settling into the equatorial ring current, mid and
low latitudes will see a reduction in the MUF as is occurring at high
latitudes.
Also the daily sunspot number needs to be higher than the present 95, as the
higher the sunspot number (100 & >) (150 & > best) the more ultraviolet
light available to increase ionization in the F/F2 layer, for more
consistent east-west radio wave propagation openings on 12 and 10 meters.
\Also on the medium frequency (MF) band there exists the normal absorption
of RF signals in the D layer due to incoming cosmic rays and hard x-rays.
Also the background x-ray flux is running in the C range so there is some
additional absorption of RF signals in the D layer.
73 & GUD DX,
Thomas F. Giella NZ4O
Lakeland, FL, USA
nz4o at tampabay.rr.com
NZ4O Amateur Radio & SWL Autobiography: http://www.nz4o.com
NZ4O MF/HF/6M Radiowave Propagation Forecast: http://www.solarcycle24.org
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