Event # | CME Time | Solar Source Time | Locate | X-ray | Type | Helicity | MC Axis | Comment | ||
---|---|---|---|---|---|---|---|---|---|---|
MDI | MC | Cylinder | Torus | |||||||
24.1→24 | 2000/09/16 05:18 | 2000/09/16 04:06 | N14W07 | M5.9 | FL | P | P | x | x | FL_from_EIT+SXT,unmatch_MC |
24.2 | 2000/09/16 05:18 | 2000/09/16 03:31 | N12W01 | C7.2 | FL | U:P,D:M | P | U:?,L:o | U:?,L:x | marge_with_24.1 |
Event Details Result on 2011/12/20 Gopal, Hong, Cho, Pertti, Seiji, and Akiyama discussed this solar source. We decieded that #24.2 was not important and was removed from the list. ******Previous Memo********************************* #24.1 CME may merge with a eruption associated with #24.2 flare which occur just 30 minutes before at the same AR). Zhang et al. (2007) listed four CME candidates. All CMEs are halo/p-halo and come from the same AR(AR 9165). But CMEs except for 1st one (#24.1 V=1213) are fainter and slower (V=285,481,633). Therefore most probable candidate is #24.1 CME. **************************************************** From Nitta's E-mail (2011/09/26 3:48 PM) this was one of the events in Jie Zhang paper in 2007, where we could not convincingly identify the solar source (confidence level 3). So I now wonder what you have done to improve the identification of the solar source for the following events since Jie's paper. Most of them are confidence level 3 events. #22, 24, 25, 27, 30, 54. I appreciate it if you let us know how you have picked up one of the possibilities. [Additional Information] Zhang et al. 2007 listed four candidates. 1st = 2000/09/16 05:18 CME 2nd = 2000/09/15 21:50 CME 3rd = 2000/09/15 15:26 CME 4th = 2000/09/15 12:06 CME | ||||||||||
Solar Source Images (Event 24.1→24) Yellow contour is a neutral line under arcade loops. | ||||||||||
Solar Source Images (Event 24.2) Yellow contour is a neutral line under arcade loops. |