Occurrence of Metric Noise Storms and the Onset of Coronal Mass Ejections in the Solar Atmosphere

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2894

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DC Field	Value	Language
dc.contributor.author	Ramesh, R	-
dc.contributor.author	Sundaram, G. A. S	-
dc.date.accessioned	2008-07-28T04:45:57Z	-
dc.date.available	2008-07-28T04:45:57Z	-
dc.date.issued	2001-05	-
dc.identifier.citation	Solar Physics, Vol. 202, No. 2, pp. 355 - 361	en
dc.identifier.issn	0038-0938	-
dc.identifier.uri	http://hdl.handle.net/2248/2894	-
dc.description	Restricted Access	en
dc.description.abstract	We performed a statistical study of the metric noise-storm continuum sources (located close to/off the solar limb, and whose start time are precisely known) observed during the period January 1997 - June 1998. The main results are: (i) a majority of the events considered were temporally followed by a coronal mass ejection off the solar limb, and (ii) the noise-storm sources were located within the angular span of the latter.	en
dc.format.extent	117268 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://www.springerlink.com/content/j51814661tr62432/	en
dc.subject	Statistical study:Metric Noise Storms	en
dc.subject	Metric Noise Storms	en
dc.subject	Solar Atmosphere	en
dc.subject	Coronal Mass	en
dc.subject	Solar	en
dc.title	Occurrence of Metric Noise Storms and the Onset of Coronal Mass Ejections in the Solar Atmosphere	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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