Multi-wavelength view of flare events on 20 November 2003

dc.contributor.author	Kumar, P
dc.contributor.author	Manoharan, P. K.
dc.contributor.author	Uddin, W.
dc.date.accessioned	2010-05-25T04:59:23Z
dc.date.available	2010-05-25T04:59:23Z
dc.date.issued	2010
dc.identifier.uri	http://hdl.handle.net/123456789/672
dc.description.abstract	We analyze two flare events that occurred in active region NOAA 501 on 20 November 2003. The Hα and magnetogram measurements show interaction between two filaments, which produced a slowly rising flare event, corresponding to two stages of magnetic reconnection. The relative clockwise rotation between the two sunspot systems caused filament destabilization. The cusp-shaped magnetic field in the main phase of the second flare and its evolution in correlation with ribbon separation provide evidence for the cause of the CME eruption. The propagation and orientation of the CME with respect to the ecliptic plane is illustrated by IPS images.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	assp2010-471
dc.subject	Multi-Wavelength, Flare	en_US
dc.title	Multi-wavelength view of flare events on 20 November 2003	en_US
dc.type	Article	en_US