10/08/2012 05:00:00 UTC

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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)
  • http://sdowww.lmsal.com/sdomedia/SunInTime/2012/10/04/daily_211-193-171.mov


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.

Jmaps

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

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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

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