Difference between revisions of "09/30/2012 23:00:00 UTC"
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| − | [http://solar.gmu.edu/wiki/upload/phess4/20120928cor2A.avi COR2A] | + | [http://solar.gmu.edu/wiki/upload/phess4/20120928cor2A.avi COR2A] <br> |
| − | [http://solar.gmu.edu/wiki/upload/phess4/20120928cor2B.avi COR2B] | + | [http://solar.gmu.edu/wiki/upload/phess4/20120928cor2B.avi COR2B] <br> |
| − | [http://solar.gmu.edu/wiki/upload/phess4/20120928hi1A.avi HI1A] | + | [http://solar.gmu.edu/wiki/upload/phess4/20120928hi1A.avi HI1A] <br> |
| − | [http://solar.gmu.edu/wiki/upload/phess4/20120928hi1B.avi HI1B] | + | [http://solar.gmu.edu/wiki/upload/phess4/20120928hi1B.avi HI1B] <br> |
| − | [http://solar.gmu.edu/wiki/upload/phess4/20120928hi2A.avi HI2A] | + | [http://solar.gmu.edu/wiki/upload/phess4/20120928hi2A.avi HI2A] <br> |
| − | [http://solar.gmu.edu/wiki/upload/phess4/20120928hi2B.avi HI2B] | + | [http://solar.gmu.edu/wiki/upload/phess4/20120928hi2B.avi HI2B] <br> |
Revision as of 14:38, 6 June 2013
Comment Section
- Complex ejecta at 1 AU (J. Zhang)
- strong B
- possibly multiple CMEs interacting; need to check all halo CMEs in the plausible launch window
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.
