Pulsating radio emission at decametre wavelengths from the sun

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4163

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DC Field	Value	Language
dc.contributor.author	Sastry, Ch. V	-
dc.contributor.author	Krishan, V	-
dc.contributor.author	Subramanian, K. R	-
dc.date.accessioned	2008-12-23T15:15:10Z	-
dc.date.available	2008-12-23T15:15:10Z	-
dc.date.issued	1981-03	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol. 2, No. 1, pp. 59 - 65	en
dc.identifier.issn	0250-6335	-
dc.identifier.uri	http://hdl.handle.net/2248/4163	-
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.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1981JApA....2...59S	en
dc.relation.uri	http://dx.doi.org/10.1007/BF02714242	en
dc.subject	Explosive instability	en
dc.subject	Pulsating burst	en
dc.title	Pulsating radio emission at decametre wavelengths from the sun	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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