Difference between revisions of "10/08/2012 05:00:00 UTC"
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=Video Data= | =Video Data= | ||
| − | [http://solar | + | [http://solar.gmu.edu/wiki/upload/phess4/aia3041005.avi AIA 304 Running Difference Movie] <br /> |
| − | [http://solar | + | [http://solar.gmu.edu/wiki/upload/phess4/aia1931005.avi AIA 195 Running Difference Movie] <br /> |
| − | [http://solar | + | [http://solar.gmu.edu/wiki/upload/phess4/euvi1005.avi STEREO EUVIA 304] <br /> |
| − | [http://solar | + | [http://solar.gmu.edu/wiki/upload/phess4/cor2A1005_good.avi STEREO COR2A] <br /> |
| − | [http://solar | + | [http://solar.gmu.edu/wiki/upload/phess4/cor2B1005_good.avi STEREO COR2B] <br /> |
| − | [http://solar | + | [http://solar.gmu.edu/wiki/upload/phess4/hi1A1005.avi STEREO HI1A] <br /> |
| − | [http://solar | + | [http://solar.gmu.edu/wiki/upload/phess4/hi1b1005.avi STEREO HI1B] <br /> |
| − | [http://solar | + | [http://solar.gmu.edu/wiki/upload/phess4/hi2A1005.avi STEREO HI2A] <br /> |
| − | [http://solar | + | [http://solar.gmu.edu/wiki/upload/phess4/hi2b1005.avi STEREO HI2B] <br /> |
=References= | =References= | ||
Revision as of 15:09, 5 August 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 - 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 [October 4, 15UT, central south]
- C. Moestl: looking at the whole October 4 SDO movie, there are also two other minor eruptions which I find very hard to distinguish from the 15 UT one (1. 7 UT, slightly west of disk center; 2. 0930 UT, south-east quadrant)
- 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
