Observations and interpretation of solar decametric absorption bursts

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1053

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DC Field	Value	Language
dc.contributor.author	Gopalswamy, N.	-
dc.contributor.author	Thejappa, N.	-
dc.contributor.author	Sastry, Ch.V.	-
dc.date.accessioned	2006-01-03T04:47:24Z	-
dc.date.available	2006-01-03T04:47:24Z	-
dc.date.issued	1983	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, 1983, Vol. 4, p215-224.	en
dc.identifier.issn	0250-6335	-
dc.identifier.uri	http://hdl.handle.net/2289/1053	-
dc.description.abstract	The observations of intensity reductions or absorption bursts in the solar decametric radio-continuum are reported. The reductions are interpreted as the absorption of continuum radiation by a shock-generated ion sound turbulence present in the layer above the continuum level. The duration of the absorption is attributed to the life-time of the ion-sound turbulence while the depth of absorption is determined by the level of Langmuir waves generated as a result of absorption.	en
dc.format.extent	1018567 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	Sun	en
dc.subject	Decametric absurption bursts	en
dc.subject	Ion-sound turbulence	en
dc.title	Observations and interpretation of solar decametric absorption bursts	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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