Difference between revisions of "07/14/2012 17:00:00 UTC"
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==SDO observations== | ==SDO observations== | ||
[http://solar.gmu.edu/wiki/upload/JieZhang/20120712_1600-1730_AIA_171.mp4 AIA-171] <br> | [http://solar.gmu.edu/wiki/upload/JieZhang/20120712_1600-1730_AIA_171.mp4 AIA-171] <br> | ||
| − | [http://solar.gmu.edu/wiki/upload/JieZhang/20120712_1600- | + | [http://solar.gmu.edu/wiki/upload/JieZhang/20120712_1600-1730_HMI_B.mp4 HMI B] <br> |
==STEREO observations== | ==STEREO observations== | ||
Revision as of 02:30, 7 June 2013
Contents
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.
Flare Data
- File:Eve flare 2012 07 12.pdf EVE and GOES flare profiles
- 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.
