09/17/2008 04:20:00 UTC

From heliophysics
Revision as of 17:09, 29 September 2014 by Davidwebb (talk | contribs) (Created page with "Yuming Wang suggests two reasons to study this event/period: (1) It looks like a stealth CME, and (2) it experienced deflected propagation to 1 AU. A comprehensive study of th...")
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)
Jump to: navigation, search

Yuming Wang suggests two reasons to study this event/period: (1) It looks like a stealth CME, and (2) it experienced deflected propagation to 1 AU. A comprehensive study of the CME will complete our understanding of the CME's origin, trigger, dynamic evolution in the corona and the interaction with ambient solar wind.

The event started on 12 September at about 15:00 UT. The ICNE date here is a MC observed at L1.



REFERENCE: Wang, Y., B. Wang, C. Shen, F. Shen, and N. Lugaz (2014), Deflected propagation of a coronal mass ejection from the corona to interplanetary space, J. Geophys. Res., Space Physics, 119, 5117–5132, doi:10.1002/2013JA019537

Retrieved from "http://solar.gmu.edu/heliophysics/index.php?title=09/17/2008_04:20:00_UTC&oldid=2228"