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CME productivity associated with Solar Flare peak X-ray emission flux

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dc.contributor.author Suryanarayana, G. S
dc.contributor.author Balakrishna, K. M
dc.date.accessioned 2020-11-11T01:36:30Z
dc.date.available 2020-11-11T01:36:30Z
dc.date.issued 2018-05-01
dc.identifier.citation Advances in Space Research, Vol. 61, No. 9, pp. 2482-2489 en_US
dc.identifier.issn 0273-1177
dc.identifier.uri http://prints.iiap.res.in/handle/2248/6873
dc.description Restricted Access © Elsevier; https://doi.org/10.1016/j.asr.2018.02.008 en_US
dc.description.abstract It is often noticed that the occurrence rate of Coronal Mass Ejections (CMEs) increases with increase in flare duration where peak flux too increase. However, there is no complete association between the duration and peak flux. Distinct characteristics have been reported for active regions (ARs) where flares and CMEs occur in contrast to ARs where flares alone occur. It is observed that peak flux of flares is higher when associated with CMEs compared to peak flux of flares with which CMEs are not associated. In other words, it is likely that flare duration and peak flux are independently affected by distinct active region dynamics. Hence, we examine the relative ability of flare duration and peak flux in enhancing the CME productivity. We report that CME productivity is distinctly higher in association with the enhancement of flare peak flux in comparison to corresponding enhancement of flare duration. en_US
dc.language.iso en en_US
dc.publisher Elsevier B.V en_US
dc.subject Sun:flares en_US
dc.subject Sun:coronal mass ejections en_US
dc.title CME productivity associated with Solar Flare peak X-ray emission flux en_US
dc.type Article en_US


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