Difference between revisions of "05/28/2010 21:00:00 UTC"
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==In-Situ Data== | ==In-Situ Data== | ||
A combination of SWEPAM and MAG data from the ACE Satellite: <br /> | A combination of SWEPAM and MAG data from the ACE Satellite: <br /> | ||
| − | [[File: | + | [[File:plot_sw_mag_plasma_2010052800.png|350px]] |
| − | [[File: | + | [[File:plot_sw_mag_2010052800.png|400px]] |
| − | [[File: | + | [[File:plot_sw_vel_2010052800.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. | ||
Revision as of 13:28, 2 July 2013
Comment Section
- A "well-behaved" CME-ICME event
- Two consecutive halo CMEs originated from the Sun from almost the same region, one at ~ 18 UT, May 23, and the other at ~ 14 UT, May 24. The question is we should expect to find two consecutive ICMEs at 1 AU, as well as in SECCHI HI observations. Is this kind of double CMEs showing up?
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.
Video Data
References
- Lugaz, N., Farrugia, C. J., Davies, J. A., Möstl, C., Davis, C. J., Roussev, I. I., & Temmer, M. (2012). The Deflection of the Two Interacting Coronal Mass Ejections of 2010 May 23-24 as Revealed by Combined in Situ Measurements and Heliospheric Imaging. Astrophysical Journal, 759(1), 68. doi:10.1088/0004-637X/759/1/68
