Difference between revisions of "04/12/2010 01:00:00 UTC"
(→Comment Section) |
(→References) |
||
| (4 intermediate revisions by 3 users not shown) | |||
| Line 1: | Line 1: | ||
=Comment Section= | =Comment Section= | ||
*Good event well observed in STEREO COR2 A/B, but appeared weak in LASCO C2 (Jie) | *Good event well observed in STEREO COR2 A/B, but appeared weak in LASCO C2 (Jie) | ||
| + | *Well behaved post-eruption loop arcade as seen from EUV coronal images | ||
=Image Data= | =Image Data= | ||
| Line 15: | Line 16: | ||
=Video Data= | =Video Data= | ||
| + | |||
| + | =References= | ||
| + | |||
| + | *Davis et al. 2011 Space Weather (summary of real time predictions) | ||
Latest revision as of 12:29, 1 July 2013
Contents
Comment Section
- Good event well observed in STEREO COR2 A/B, but appeared weak in LASCO C2 (Jie)
- Well behaved post-eruption loop arcade as seen from EUV coronal images
Image Data
In-Situ Data
A combination of SWEPAM and MAG data from the ACE Satellite:
Error creating thumbnail: File missing
Error creating thumbnail: File missing
Error creating thumbnail: File missing
The blue lines are an approximation of the CME cloud and the red line denotes the shock.
GOES X-RAY FLUX
Error creating thumbnail: File missing
The GOES X-ray Flux of the flare associated with the event. The vertical line approximately denotes the flare peak time.
Video Data
References
- Davis et al. 2011 Space Weather (summary of real time predictions)
