Difference between revisions of "08/03/2010 16:00:00 UTC"
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*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 [http://www.uni-graz.at/igam-sophy/isest2013/20100801/ 2010-Aug-01 Events] | *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 [http://www.uni-graz.at/igam-sophy/isest2013/20100801/ 2010-Aug-01 Events] | ||
*A "well-behaved" CME-ICME event; clear eruption signature in EUV coronal images (Jie) | *A "well-behaved" CME-ICME event; clear eruption signature in EUV coronal images (Jie) | ||
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=Image Data= | =Image Data= | ||
Revision as of 11:30, 1 July 2013
Contents
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-Aug-01 Events
- A "well-behaved" CME-ICME event; clear eruption signature in EUV coronal images (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.
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.
