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[STORMREPORTS] Geomagnetic Storm Ends/ New Storm Enroute
Our latest severe (Kp-8) to extreme (Kp-9) geomagnetic storm has come to an end. Unfortunately though the very fast moving (1000+ k/s) partial halo coronal mass ejection released by sunspot group #10696 on November 10th will arrive on UTC November 11-12, 2004 and create another strong (Kp-7) to severe (Kp-8) geomagnetic storm. An extreme (Kp-9) storm is less likely this time around as part of the CME will miss Earth.
Fortunately sunspot group #10696 will be rotating around the west limb within 24 hours and space weather and geomagnetic activity should slowly return to normal levels. It will take another two days for the current elevated energetic proton storm >10 mev to end so in the interim we can expect a continuation of some high latitude propagation path absorption on the MF AM broadcast band, 160 and 120 meters. we can also expect mid and lower latitude LF/MF propagation paths to stay depressed for a while until the geomagnetic equatorial ring current unloads it's cache of precipitated electrons. The DST index is a measuring gauge so to speak for the equatorial ring current. You can see the current DST index at: http://swdcdb.kugi.kyotou.ac.jp/dstdir/dst1/q/Dstqthism.html .
Also normally a Boulder K index of 9 is needed for low latitude visible aurora in the U.S. and this time around the Boulder K only reached an 8. But I would still be interested in getting any reports of visible aurora south of 30 deg. N/S latitude. Remember though that visible aurora is not automatic with geomagnetic storming. The magnetic (Bz) component of the solar wind must be a negative value in nt (nano tesla's) in unison with a geomagnetic storm for aurora to be seen.
73,
Propagation eGroup: http://lists.contesting.com/mailman/listinfo/propagation
----- Original Message -----
:Issued: 2004 Nov 11 1407 UTC
SOLAR INDICES FOR 10 Nov 2004
NOTICEABLE EVENTS SUMMARY
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