Difference between revisions of "10/08/2012 05:00:00 UTC"
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| =Comment Section= | =Comment Section= | ||
| − | 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) | + | *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= | =Image Data= | ||
Revision as of 01:41, 3 June 2013
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: 
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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 
