Pulsating radio emission at decameter wavelengths from the Sun

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DC Field	Value	Language
dc.contributor.author	Sastry, Ch.V.	-
dc.contributor.author	Krishan, Vinod	-
dc.contributor.author	Subramanian, K.R.	-
dc.date.accessioned	2005-12-29T04:57:42Z	-
dc.date.available	2005-12-29T04:57:42Z	-
dc.date.issued	1981	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, 1981, Vol. 2, p59-65.	en
dc.identifier.issn	0250-6335	-
dc.identifier.uri	http://hdl.handle.net/2289/952	-
dc.description.abstract	Observations on the pulsation pattern in the time profile of short duration solar radio bursts at decametre wavelengths are presented. The pulsations are found to be present predominantly in the saturation phase of the burst. A tentative physical model based on the non-linear development of the waves interacting in a turbulent medium is invoked to explain the origin of the pulsations.	en
dc.format.extent	666375 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences, Bangalore, India.	en
dc.rights	Indian Academy of Sciences, Bangalore, India.	en
dc.subject	Explosive instability	en
dc.subject	Pulsating burst	en
dc.title	Pulsating radio emission at decameter wavelengths from the Sun	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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