Difference between revisions of "02/18/2011 00:00:00 UTC"

From heliophysics
Jump to: navigation, search
Line 1: Line 1:
 
=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 (Jie).
+
*A "big" event of having everything: 2012/02/15 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 (Jie).
 +
*Question: on 2012/02/14 (18 UT), there was an Earth-directing CME as seen from C2 and CORs. Did this halo CME also reach the Earth, in addition to the one originated on 2012/02/15 (02 UT).
  
 
=Image Data=
 
=Image Data=

Revision as of 00:48, 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: 2012/02/15 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 (Jie).
  • Question: on 2012/02/14 (18 UT), there was an Earth-directing CME as seen from C2 and CORs. Did this halo CME also reach the Earth, in addition to the one originated on 2012/02/15 (02 UT).

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