Revision as of 14:45, 14 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)

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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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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Jmaps along the CME leading edge position (about 7 <math>/deg<math> S of the ecliptic) from STEREO A and B

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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.

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 results of geometrical modeling (C. Moestl): <br />
 [[File:Geometry_12_july2012.jpeg‎|400px]] <br />
+Jmaps along the CME leading edge position (about 7 <math>/deg<math> S  of the ecliptic) from STEREO A and B
+[[File:20120712JmapA.png|500 px]] [[File:20120712JmapB.png|500 px]] <br>
 ==Flare Data==