Type-I Solar Radio Bursts

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/370

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DC Field	Value	Language
dc.contributor.author	Gopalswamy, N	-
dc.date.accessioned	2005-02-11T05:47:17Z	-
dc.date.available	2005-02-11T05:47:17Z	-
dc.date.issued	1986	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 6, pp. 77-85	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/370	-
dc.description.abstract	A brief review of the recent work done on Type-I radio emission in the Indian Institute of Astrophysics is presented. The most plausible low frequency turbulence needed to generate the type-I bursts is shown to be ion-sound turbulence. A method is presented to evaluate the coronal magnetic field using type-I radio emission data.	en
dc.format.extent	322979 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Radio Bursts	en
dc.subject	Solar Radio Bursts	en
dc.subject	Type-I Solar Radio Bursts	en
dc.title	Type-I Solar Radio Bursts	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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