07/14/2012 17:00:00 UTC
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.
The results from geometrical modeling in comparison to the in situ data from the Wind spacecraft (C. Moestl)
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Heliospheric Imaging
CME track observed in STEREO-A Jmap with SATPLOT software: (C. Moestl)
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results of geometrical modeling (C. Moestl):
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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.
