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DSF/CME


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A long duration (LDE) C1 X-Ray event at 0710Z was associated with a disppearing filament (aka an aruptive filament) (DSF) which triggered a Category 1 radiation event with >10MeV proton flux at event levels and recently peaking at 54 pfu. A Full Halo CME was also observed by SOHO and is expected to reach Earth around 1430Z 28 Nov ±7 hours. The possibility exists that a Gemag event will result but the timing is poor for US and European aurora observers. The event points up the importance of filament eruptions in causing Gemags (the October event was also a DSF) since the X-Ray flare and radio bursts were very weak yet we are having significant Geophysical effects.

Steve

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A long duration (LDE) C1 X-Ray event at 0710Z was associated with a disppearing filament (aka an aruptive filament) (DSF) which triggered a Category 1 radiation event with >10MeV proton flux at event levels and recently peaking at 54 pfu. A Full Halo CME was also observed by SOHO and is expected to reach Earth around 1430Z 28 Nov ±7 hours. The possibility exists that a Gemag event will result but the timing is poor for US and European aurora observers. The event points up the importance of filament eruptions in causing Gemags (the October event was also a DSF) since the X-Ray flare and radio bursts were very weak yet we are having significant Geophysical effects.

Steve

well, that's disappointing...the last event was poorly timed for US viewing as well...

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