Difference between revisions of "10/08/2012 05:00:00 UTC"

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**A good example of "stealth" CME: bright CME, but no or very weak surface signature (in terms of no flare, dimming, filament eruption etc)
 
**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)
 
*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)
* Manuela: clear on-disk signatures - movie from SDO (October 4, 15UT, central south) - are visible. It is a "silent" CME, hard to catch for space weather forecasters, but not a "stealth" in sense of no solar surface signatures at all.
+
* M. Temmer: clear on-disk signatures - movie from SDO (October 4, 15UT, central south) - are visible. It is a "silent" CME, hard to catch for space weather forecasters, but not a "stealth" in sense of no solar surface signatures at all.
 
http://sdowww.lmsal.com/sdomedia/SunInTime/2012/10/04/daily_211-193-171.mov
 
http://sdowww.lmsal.com/sdomedia/SunInTime/2012/10/04/daily_211-193-171.mov
 
* timing - evolution from SDO FoV to coronagraph - is an issue and needs to be looked at in detail  
 
* timing - evolution from SDO FoV to coronagraph - is an issue and needs to be looked at in detail  

Revision as of 08:16, 19 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)
  • M. Temmer: clear on-disk signatures - movie from SDO (October 4, 15UT, central south) - are visible. It is a "silent" CME, hard to catch for space weather forecasters, but not a "stealth" in sense of no solar surface signatures at all.

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

  • timing - evolution from SDO FoV to coronagraph - is an issue and needs to be looked at in detail


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