Type-I Solar Radio Bursts

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