Difference between revisions of "07/14/2012 17:00:00 UTC"
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== Heliospheric Imaging == | == Heliospheric Imaging == | ||
CME track observed in Jmap with SATPLOT software (STEREO-A): <br /> | CME track observed in Jmap with SATPLOT software (STEREO-A): <br /> | ||
| − | [[File:satplot_jmap_july122012.png|300px | + | [[File:satplot_jmap_july122012.png|300px]] <br /> |
results of geometrical modeling: <br /> | results of geometrical modeling: <br /> | ||
| − | [[File:Geometry_12_july2012.jpeg|300px | + | [[File:Geometry_12_july2012.jpeg|300px]] <br /> |
==Flare Data== | ==Flare Data== | ||
Revision as of 05:14, 12 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.
Heliospheric Imaging
CME track observed in Jmap with SATPLOT software (STEREO-A):
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results of geometrical modeling:
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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.
