07/14/2012 17:00:00 UTC

From heliophysics
Revision as of 02:21, 7 June 2013 by JieZhang (talk | contribs)
Jump to: navigation, search

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.

Flare Data

  • 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.

Video Data

COR2A
COR2B
HI1A
HI1B
HI2A
HI2B