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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7055
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dc.contributor.authorSuryanarayana, G. S-
dc.contributor.authorBalakrishna, K. M-
dc.date.accessioned2020-11-17T02:45:56Z-
dc.date.available2020-11-17T02:45:56Z-
dc.date.issued2017-01-
dc.identifier.citationResearch in Astronomy and Astrophysics, Vol. 17, No. 1, 7en_US
dc.identifier.issn1674-4527-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/7055-
dc.descriptionRestricted Access © IOP Publishing https://doi.org/10.1088/1674-4527/17/1/7en_US
dc.description.abstractFeatures 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 associationsen_US
dc.language.isoenen_US
dc.publisherIOP Publishingen_US
dc.subjectSun: activityen_US
dc.subjectSun: flaresen_US
dc.subjectSun: coronal mass ejectionsen_US
dc.titlePeak flux of flares associated with Coronal Mass Ejectionsen_US
dc.typeArticleen_US
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