Difference between revisions of "04/05/2010 08:00:00 UTC"
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| + | [http://solar.gmu.edu/wiki/upload/phess4/20100403cor2A.avi COR2A] <br> | ||
| + | [http://solar.gmu.edu/wiki/upload/phess4/20100403cor2B.avi COR2B] <br> | ||
| + | [http://solar.gmu.edu/wiki/upload/phess4/20100403hi1A.avi HI1A] <br> | ||
| + | [http://solar.gmu.edu/wiki/upload/phess4/20100403hi1B.avi HI1B] <br> | ||
| + | [http://solar.gmu.edu/wiki/upload/phess4/20100403hi2A.avi HI2A] <br> | ||
| + | [http://solar.gmu.edu/wiki/upload/phess4/20100403hi2B.avi HI2B] <br> | ||
Revision as of 17:17, 4 June 2013
The April 05, 2010 CME erupted from Sun around 09:00 UT on April 03, associated with a flare from NOAA Active Region 11059 (S25 W03). The first signature as seen in ACE is of a shock front at 08:00 UT and a flux rope is observed by ACE at 11:30 UT.
Comment Section
- Manuela Temmer: we can provide for close to the Sun deprojected height-time, velocity-time, acceleration-time, mass-time/distance plots, as well as some movies (STEREO); have a look under 2010-Apr-03 Event
- A well-behaved CME-ICME event (Jie)
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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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.
