Difference between revisions of "02/18/2011 00:00:00 UTC"
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=Comment Section= | =Comment Section= | ||
| − | Manuela Temmer: we can provide for close to the Sun deprojected height-time, velocity-time, acceleration-time, mass-time/distance plots (direction E7) as well as some movies (STEREO); have a look under [http://www.uni-graz.at/igam-sophy/isest2013/20110215/ 2011-Feb-15 Event] | + | *Manuela Temmer: we can provide for close to the Sun deprojected height-time, velocity-time, acceleration-time, mass-time/distance plots (direction E7) as well as some movies (STEREO); have a look under [http://www.uni-graz.at/igam-sophy/isest2013/20110215/ 2011-Feb-15 Event] |
| + | *A "big" event of having everything: X2 flare, coronal dimming and wave, fast halo CME in LASCO, strong signature in COR2, and high magnetic field in the ICME sheath region as seen in in-situ | ||
=Image Data= | =Image Data= | ||
Revision as of 00:42, 2 June 2013
Comment Section
- Manuela Temmer: we can provide for close to the Sun deprojected height-time, velocity-time, acceleration-time, mass-time/distance plots (direction E7) as well as some movies (STEREO); have a look under 2011-Feb-15 Event
- A "big" event of having everything: X2 flare, coronal dimming and wave, fast halo CME in LASCO, strong signature in COR2, and high magnetic field in the ICME sheath region as seen in in-situ
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.
