Event # | CME Time | Solar Source Time | Locate | X-ray | Type | Helicity | MC Axis | Comment | ||
---|---|---|---|---|---|---|---|---|---|---|
MDI | MC | Cylinder | Torus | |||||||
16.1→16 | 2000/02/17 21:30 | 2000/02/17 20:17 | S29E07 | M1.3 | FL+EP | P | P | o | x | EP_from_EIT+MLSO,marge_with_16.2? |
16.2 | 2000/02/17 19:31 | 2000/02/17 18:41 | S25W16 | M2.5 | FL+EP | P | P | ? | o | EP_from_EIT+MLSO,marge_with_16? |
Event Details Result on 2011/12/20 Gopal, Hong, Cho, Pertti, Seiji, and Akiyama discussed this solar source. They agree about the previous result. ******Previous Memo********************************* #16.1 CME may merge with #16.2 CME. We select #16.1 CME as a 1st candidate, because CME speed is faster than another. | ||||||||||
Solar Source Images (Event 16.1→16) Yellow contour is a eruptive filament obseved by EIT and MLSO Ha movie. | ||||||||||
Solar Source Images (Event 16.2) Yellow contour is a eruptive filament obseved by EIT and MLSO Ha movie. |