Difference between revisions of "07/14/2012 17:00:00 UTC"
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**classical ICME feature: shock + sheath + magnetic cloud | **classical ICME feature: shock + sheath + magnetic cloud | ||
**strong solar signature: X1 flare (S17W08); halo CME, fast and bright | **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= | =Image Data= | ||
Revision as of 16:36, 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.
