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) | ||
| + | *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= | ||
| + | ==In-Situ Data== | ||
| + | A combination of SWEPAM and MAG data from the ACE Satellite: <br /> | ||
| + | [[File:plot_sw_mag_plasma_2011102400.png|350px]] | ||
| + | [[File:plot_sw_mag_2011102400.png|400px]] | ||
| + | [[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. | ||
| + | |||
| + | ==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= | ||
| + | |||
| + | |||
| + | =References= | ||
Latest revision as of 16:40, 24 June 2013
Contents
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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Error creating thumbnail: File missing
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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
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.
