Difference between revisions of "03/08/2012 11:00:00 UTC"
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*A fair ICME event, but strong solar source | *A fair ICME event, but strong solar source | ||
**X1 flare, fast CME, originated from the eastern hemisphere (~N18E42) | **X1 flare, fast CME, originated from the eastern hemisphere (~N18E42) | ||
| − | **Solar wind plasma data is corrupted. | + | **Solar wind plasma data is corrupted. |
| − | + | *Ying Liu et al. 2013 ApJ | |
=Image Data= | =Image Data= | ||
Revision as of 02:24, 20 June 2013
Contents
Comment Section
- A fair ICME event, but strong solar source
- X1 flare, fast CME, originated from the eastern hemisphere (~N18E42)
- Solar wind plasma data is corrupted.
- Ying Liu et al. 2013 ApJ
Image Data
In-Situ Data
A combination of SWEPAM and MAG data from the ACE Satellite:
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The blue lines are an approximation of the CME cloud and the red line denotes the shock.
GOES X-RAY FLUX
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The GOES X-ray Flux of the flare associated with the event. The vertical line approximately denotes the flare peak time.
