10/08/2012 05:00:00 UTC

From heliophysics
Revision as of 04:03, 19 June 2013 by Phess4 (talk | contribs) (Video Data)
Jump to: navigation, search

Comment Section

  • A good ICME, strong CME source, however, "stealth" surface signature (J. Zhang)
    • A good example of "stealth" CME: bright CME, but no or very weak surface signature (in terms of no flare, dimming, filament eruption etc)
  • This event has a very difficult to distinguish source region, if you look very closely at S22 W38 just before 00:00 UT on the 10/05 it is possible to see a very small disturbance on the Sun, especially in 304 Angstroms. (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.

Jmaps

Jmaps from STEREO A and B along the CME leading edge position angle

Error creating thumbnail: File missing
Error creating thumbnail: File missing


Video Data

AIA 304 Running Difference Movie
AIA 195 Running Difference Movie
STEREO EUVIA 304
STEREO COR2A
STEREO COR2B
STEREO HI1A
STEREO HI1B
STEREO HI2A
STEREO HI2B

References