Difference between revisions of "04/23/2012 02:30:00 UTC"
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*A slow CME swept up by a CIR (J. Zhang) | *A slow CME swept up by a CIR (J. Zhang) | ||
*Not sure about the source CME (1) 04/19 15 UT CME, or (2) 04/18 03 UT CME (also other halo CMEs on 04/18); need further work on this. | *Not sure about the source CME (1) 04/19 15 UT CME, or (2) 04/18 03 UT CME (also other halo CMEs on 04/18); need further work on this. | ||
| − | **It is always a problem of identification when a slow ICME occurs. | + | **It is always a problem of identification when a slow ICME occurs. |
| + | *In Moestl's list, CME (1) on April 19 16:24 (first image in COR2A) is the source for the ICME | ||
=Image Data= | =Image Data= | ||
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=Video Data= | =Video Data= | ||
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| + | =References= | ||
Latest revision as of 02:35, 20 June 2013
Comment Section
- A slow CME swept up by a CIR (J. Zhang)
- Not sure about the source CME (1) 04/19 15 UT CME, or (2) 04/18 03 UT CME (also other halo CMEs on 04/18); need further work on this.
- It is always a problem of identification when a slow ICME occurs.
- In Moestl's list, CME (1) on April 19 16:24 (first image in COR2A) is the source for the ICME
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.
