Spectral characteristics of a solar flare from ionospheric data

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5138

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DC Field	Value	Language
dc.contributor.author	Bhattacharyya, J. C	-
dc.contributor.author	Balakrishnan, T. K	-
dc.date.accessioned	2010-06-08T16:00:50Z	-
dc.date.available	2010-06-08T16:00:50Z	-
dc.date.issued	1967	-
dc.identifier.citation	Journal of Atmospheric and Terrestrial Physics, Vol. 29, No. 12, pp. 1573 - 1579	en
dc.identifier.uri	http://hdl.handle.net/2248/5138	-
dc.description	Restricted Access	-
dc.description.abstract	From the height variation of electron densities during a solar flare, ultra violet and X-ray contribution of ionization process has been estimated. The results thus obtained are in conformity with direct measurements of solar ultraviolet and X-ray spectra by rocket techniques.	en
dc.language.iso	en	en
dc.publisher	Pergamon Press Ltd	en
dc.relation.uri	http://dx.doi.org/10.1016/0021-9169(67)90109-2	en
dc.rights	© Elsevier Ltd.	en
dc.subject	Solar flare	en
dc.title	Spectral characteristics of a solar flare from ionospheric data	en
dc.type	Article	en
Appears in Collections:	IIAP Publications J.C.Bhattacharyya (1982 - 1990)

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