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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/8011
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dc.contributor.authorSuryanarayana, G. S-
dc.date.accessioned2022-08-23T05:43:24Z-
dc.date.available2022-08-23T05:43:24Z-
dc.date.issued2022-07-01-
dc.identifier.citationAdvances in Space Research, Vol. 70, No. 1, pp. 223-228en_US
dc.identifier.issn0273-1177-
dc.identifier.urihttp://hdl.handle.net/2248/8011-
dc.descriptionRestricted Accessen_US
dc.description.abstractActive 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.isoenen_US
dc.publisherElsevieren_US
dc.relation.urihttps://doi.org/10.1016/j.asr.2022.04.027-
dc.subjectSolar flaresen_US
dc.subjectFlare durationen_US
dc.subjectPeak fluxen_US
dc.subjectCumulative fluxen_US
dc.titleAssociation between the number of flares in an active region and cumulative fluxen_US
dc.typeArticleen_US
dcterms.rights© Elsevier B.V.-
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