Difference between revisions of "03/08/2012 11:00:00 UTC"
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=Comment Section= | =Comment Section= | ||
| − | *A slow ICME | + | *A slow ICME with extremely long duration as seen at 1 AU |
| + | *Seems an excellent example of the so-called "global" CME, or longitudinal extended CME (Jie) | ||
| + | **COR2 A: symmetric above both east and west limbs along the equator, indicating a global feature | ||
| + | **COR2 B: same as COR2, symmetric above both limbs | ||
| + | **Combining COR2 A and B, it seems a global CME, surrounding the entire solar equator | ||
| + | **Also a "stealth" CME: Need to check AIA and EUVI data to confirm the source | ||
| + | **There is no apparent halo-like feature as seen from LASCO | ||
=Image Data= | =Image Data= | ||
Revision as of 14:36, 2 June 2013
Comment Section
- A slow ICME with extremely long duration as seen at 1 AU
- Seems an excellent example of the so-called "global" CME, or longitudinal extended CME (Jie)
- COR2 A: symmetric above both east and west limbs along the equator, indicating a global feature
- COR2 B: same as COR2, symmetric above both limbs
- Combining COR2 A and B, it seems a global CME, surrounding the entire solar equator
- Also a "stealth" CME: Need to check AIA and EUVI data to confirm the source
- There is no apparent halo-like feature as seen from LASCO
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.
GOES X-RAY FLUX
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The GOES X-ray Flux of the flare associated with the event. The vertical line approximately denotes the flare peak time.
