Difference between revisions of "04/12/2010 01:00:00 UTC"
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=Comment Section= | =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= | =Image Data= | ||
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[[File:plot_sw_vel_2010041100.png|350px]] <br /> | [[File:plot_sw_vel_2010041100.png|350px]] <br /> | ||
The blue lines are an approximation of the CME cloud and the red line denotes the shock. | The blue lines are an approximation of the CME cloud and the red line denotes the shock. | ||
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| + | ==GOES X-RAY FLUX== | ||
| + | [[File:20100408_goes.png|500px]]<br /><br /> | ||
| + | The GOES X-ray Flux of the flare associated with the event. The vertical line approximately denotes the flare peak time. <br /> | ||
=Video Data= | =Video Data= | ||
| + | |||
| + | =References= | ||
| + | |||
| + | *Davis et al. 2011 Space Weather (summary of real time predictions) | ||
Latest revision as of 11:29, 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:
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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.
Video Data
References
- Davis et al. 2011 Space Weather (summary of real time predictions)
