Peak flux of flares associated with Coronal Mass Ejections

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7055

Title:	Peak flux of flares associated with Coronal Mass Ejections
Authors:	Suryanarayana, G. S Balakrishna, K. M
Keywords:	Sun: activity Sun: flares Sun: coronal mass ejections
Issue Date:	Jan-2017
Publisher:	IOP Publishing
Citation:	Research in Astronomy and Astrophysics, Vol. 17, No. 1, 7
Abstract:	Features of flares that occur in association with coronal mass ejections (CMEs) have often displayed variations compared to flares with no associated CMEs. A comparative estimation of peak flux values of flares associated with CMEs and those without CMEs is made. Peak flux values of flares associated with CMEs show distinctly higher values in comparison to flares with no associated CMEs. Higher peak flux of CME associated flares may be attributed to the heating of plasma to higher temperature when associated with CMEs. While providing a distinct difference between the flux values of flares clearly associated with CMEs compared to flares associated with no CMEs, this study also highlights an evident difficulty in making distinct flare-CME associations
Description:	Restricted Access © IOP Publishing https://doi.org/10.1088/1674-4527/17/1/7
URI:	http://prints.iiap.res.in/handle/2248/7055
ISSN:	1674-4527
Appears in Collections:	IIAP Publications

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