Difference between revisions of "07/14/2012 17:00:00 UTC"
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[http://solar.gmu.edu/wiki/upload/phess4/cor2A.avi COR2A] | [http://solar.gmu.edu/wiki/upload/phess4/cor2A.avi COR2A] | ||
| + | [http://solar.gmu.edu/wiki/upload/phess4/cor2B.avi COR2B] | ||
| + | [http://solar.gmu.edu/wiki/upload/phess4/hi1Ard.avi HI1A] | ||
| + | [http://solar.gmu.edu/wiki/upload/phess4/hi1Brd.avi HI1B] | ||
| + | [http://solar.gmu.edu/wiki/upload/phess4/hi2Ard.avi HI2A] | ||
| + | [http://solar.gmu.edu/wiki/upload/phess4/hi2Brd.avi HI2B] | ||
Revision as of 16:39, 4 June 2013
Comment Section
- A perfect CME-ICME chain event (J. Zhang)
- classical ICME feature: shock + sheath + magnetic cloud
- strong solar signature: X1 flare (S17W08); halo CME, fast and bright
- Propagation Direction is very close to the Sun Earth Line, making this a good event for comparing observations nearer the Sun to in-situ signatures (P. Hess)
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.
