Difference between revisions of "10/08/2012 05:00:00 UTC"
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[[File:plot_sw_vel_2012100700.png|350px]] <br /> | [[File:plot_sw_vel_2012100700.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. | ||
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| + | ==Jmaps== | ||
| + | Jmaps from STEREO A and B along the CME leading edge position angle <br /> | ||
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| + | [[File:jmapA20101005.png|500px]] | ||
| + | [[File:jmapB20101005.png|500px]] | ||
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=Video Data= | =Video Data= | ||
Revision as of 14:30, 28 May 2013
Comment Section
This event has a very difficult to distinguish source region, if you look very closely at S22 W38 just before 00:00 UT on the 10/05 it is possible to see a very small disturbance on the Sun, especially in 304 Angstroms. (Hess)
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.
Jmaps
Jmaps from STEREO A and B along the CME leading edge position angle
Video Data
AIA 304 Running Difference Movie
AIA 195 Running Difference Movie
STEREO EUVIA 304
STEREO COR2A
STEREO COR2B
STEREO HI1A
STEREO HI1B
STEREO HI2A
STEREO HI2B
