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:
Error creating thumbnail: File missing
Error creating thumbnail: File missing
Error creating thumbnail: File missing
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)
Error creating thumbnail: File missing
Heliospheric Imaging
CME track observed in STEREO-A Jmap with SATPLOT software: (C. Moestl)
Error creating thumbnail: File missing
results of geometrical modeling (C. Moestl):
Error creating thumbnail: File missing
Jmaps along the CME leading edge position (about <math>7^{\circ}</math> S of the ecliptic) from STEREO A and B
Error creating thumbnail: File missing
Error creating thumbnail: File missing
Flare Data
- File:Eve flare 2012 07 12.pdf EVE and GOES flare profiles
- GOES X-RAY FLUX
Error creating thumbnail: File missing
The GOES X-ray Flux of the flare associated with the event. The vertical line approximately denotes the flare peak time.
