Difference between revisions of "10/24/2011 17:38:00 UTC"
(→Comment Section) |
(→In-Situ Data) |
||
| Line 9: | Line 9: | ||
[[File:plot_sw_vel_2011102400.png|350px]] <br /> | [[File:plot_sw_vel_2011102400.png|350px]] <br /> | ||
The blue lines are an approximation of the CME cloud and the red line denotes the shock. | The blue lines are an approximation of the CME cloud and the red line denotes the shock. | ||
| + | |||
| + | ==GOES X-RAY FLUX== | ||
| + | [[File:20111022_goes.png|500px]]<br /><br /> | ||
| + | The GOES X-ray Flux of the flare associated with the event. The vertical line approximately denotes the flare peak time. <br /> | ||
=Video Data= | =Video Data= | ||
Revision as of 14:44, 28 May 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)
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.
