The Halo CME Event Of 23 October 1997 - Low-Frequency Radio Observations Of The Pre-Event Corona

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3146

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DC Field	Value	Language
dc.contributor.author	Ramesh, R	-
dc.date.accessioned	2008-08-14T11:24:14Z	-
dc.date.available	2008-08-14T11:24:14Z	-
dc.date.issued	2000-09	-
dc.identifier.citation	Solar Physics, Vol. 196, No. 1, pp. 213 - 220	en
dc.identifier.issn	0038-0938	-
dc.identifier.uri	http://hdl.handle.net/2248/3146	-
dc.description.abstract	We report low-frequency observations of an enhancement in the solar corona prior to the halo coronal mass ejection of 23 October 1997, with the Gauribidanur radioheliograph. The Sun was `quiet' and no radio bursts were observed either prior to or in the aftermath of the event. The radio method would be useful in studying the pre-event structures associated with the eruptive solar activity, particularly from the ground.	en
dc.format.extent	98521 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://www.springerlink.com/content/k57018776036jv55/	en
dc.subject	Low-Frequency Observations	en
dc.subject	Solar Corona	en
dc.subject	Halo Coronal Mass Ejection	en
dc.subject	Radio Bursts	en
dc.subject	Solar Activity	en
dc.title	The Halo CME Event Of 23 October 1997 - Low-Frequency Radio Observations Of The Pre-Event Corona	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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