Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7267
Title: Flares before and after coronal mass ejections
Authors: Suryanarayana, G. S
Keywords: Sun: flares;Sun: flare durations;Sun: peak flux of flares;Sun: coronal mass ejections
Issue Date: Mar-2018
Publisher: IOP Publishing
Citation: Research in Astronomy and Astrophysics, Vol. 18, No. 3, 34
Abstract: Flare characteristics such as the flare occurrence number density and the distribution of peak flux as well as duration of flares occurring on either side of a coronal mass ejection (CME) onset time are studied. While the flares are rather evenly distributed statistically on either side of the CME onset time, the flare peak flux and duration tend to decrease depending upon their occurrence either before or after the CME onset. This is consistent with the earlier findings that flares emit higher energy before a CME whereas the energy is less in flares occurring after a CME.
Description: Restricted Access
URI: http://hdl.handle.net/2248/7267
ISSN: 1674-4527
???metadata.dc.relation.uri???: https://doi.org/10.1088/1674-4527/18/3/34
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Flares before and after coronal mass ejections.pdfRestricted Access259.7 kBAdobe PDFView/Open    Request a copy


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.