Difference between revisions of "10/24/2011 17:38:00 UTC"
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=Comment Section= | =Comment Section= | ||
*I believe this is a complex event, caused by a merger between a partial halo CME on October 21 and the shock wave of a CME at the North Eastern Limb on the 22nd. I believe the halo CME was propagating towards the Earth, then the shock wave caught the CME front and accelerated it faster.(Hess) | *I believe this is a complex event, caused by a merger between a partial halo CME on October 21 and the shock wave of a CME at the North Eastern Limb on the 22nd. I believe the halo CME was propagating towards the Earth, then the shock wave caught the CME front and accelerated it faster.(Hess) | ||
| − | *Two full halo CMEs are involved in this event (J. Zhang) | + | *Two full halo CMEs are involved in this event, but it would be good to know exactly which event produced the ICME at 1 AU (J. Zhang) |
=Image Data= | =Image Data= | ||
Revision as of 20:41, 2 June 2013
Comment Section
- I believe this is a complex event, caused by a merger between a partial halo CME on October 21 and the shock wave of a CME at the North Eastern Limb on the 22nd. I believe the halo CME was propagating towards the Earth, then the shock wave caught the CME front and accelerated it faster.(Hess)
- Two full halo CMEs are involved in this event, but it would be good to know exactly which event produced the ICME at 1 AU (J. Zhang)
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.
