Association between the number of flares in an active region and cumulative flux

dc.contributor.author	Suryanarayana, G. S
dc.date.accessioned	2022-08-23T05:43:24Z
dc.date.available	2022-08-23T05:43:24Z
dc.date.issued	2022-07-01
dc.identifier.citation	Advances in Space Research, Vol. 70, No. 1, pp. 223-228	en_US
dc.identifier.issn	0273-1177
dc.identifier.uri	http://hdl.handle.net/2248/8011
dc.description	Restricted Access	en_US
dc.description.abstract	Active region (AR) flux is released in the form of flares and Coronal Mass Ejections and a host of several other energetic events. The development of an AR is an indication of the accumulation of flux which reflects the non-potentiality of the region. Hence, the total flux released by all the flares associated with a given AR may be indicative of the total magnetic energy although not exhaustive. In this context, we report the good association between the number of flares occurring in a given AR and the cumulative flare duration in that AR. Hence, the number of flares occurring in an AR and consequently the cumulative flare duration therein can be regarded as a good measure of the underlying mechanism of that AR.	en_US
dc.language.iso	en	en_US
dc.publisher	Elsevier	en_US
dc.relation.uri	https://doi.org/10.1016/j.asr.2022.04.027
dc.subject	Solar flares	en_US
dc.subject	Flare duration	en_US
dc.subject	Peak flux	en_US
dc.subject	Cumulative flux	en_US
dc.title	Association between the number of flares in an active region and cumulative flux	en_US
dc.type	Article	en_US
dcterms.rights	© Elsevier B.V.