Peak flux of flares associated with Coronal Mass Ejections

dc.contributor.author	Suryanarayana, G. S
dc.contributor.author	Balakrishna, K. M
dc.date.accessioned	2020-11-17T02:45:56Z
dc.date.available	2020-11-17T02:45:56Z
dc.date.issued	2017-01
dc.identifier.citation	Research in Astronomy and Astrophysics, Vol. 17, No. 1, 7	en_US
dc.identifier.issn	1674-4527
dc.identifier.uri	http://prints.iiap.res.in/handle/2248/7055
dc.description	Restricted Access © IOP Publishing https://doi.org/10.1088/1674-4527/17/1/7	en_US
dc.description.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	en_US
dc.language.iso	en	en_US
dc.publisher	IOP Publishing	en_US
dc.subject	Sun: activity	en_US
dc.subject	Sun: flares	en_US
dc.subject	Sun: coronal mass ejections	en_US
dc.title	Peak flux of flares associated with Coronal Mass Ejections	en_US
dc.type	Article	en_US