Solar and interplanetary signatures of intense geomagnetic storms during 1997-2000

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DC Field	Value	Language
dc.contributor.author	Srivastava, N	-
dc.date.accessioned	2008-04-23T10:01:40Z	-
dc.date.available	2008-04-23T10:01:40Z	-
dc.date.issued	2001	-
dc.identifier.citation	BASI, Vol. 29, No. 3, pp. 249 - 250	en
dc.identifier.uri	http://hdl.handle.net/2248/2251	-
dc.description.abstract	During the ascending phase of the recent solar cycle, the solar and interplanetary signatures of coronal mass ejections (CMEs) observed by Large Angle Spectrometric Coronagraphs (LASCO) aboard SOHO, have been examined. These CMEs were responsible for causing intense geomagnetic storms (Dst ≤ -100 nT) on the earth. In this paper, the relationship of these CMEs with halos, long-duration events, flares and eruptive prominences have been studied. In addition, investigation of the role of the initial expansion speeds of halos in determining the time of their arrival at the earth has also been made.	en
dc.format.extent	181013 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2001BASI...29..249S	en
dc.subject	Coronal mass ejection	en
dc.subject	Geomagnetic storm	en
dc.title	Solar and interplanetary signatures of intense geomagnetic storms during 1997-2000	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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