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  5. M.K. Vainu Bappu ( 1960 - 1982 )
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1987
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dc.contributor.authorBappu, M. K. V-
dc.contributor.authorSivaraman, K. R-
dc.date.accessioned2007-11-29T06:54:35Z-
dc.date.available2007-11-29T06:54:35Z-
dc.date.issued1969-12-
dc.identifier.citationSolar Physics, Vol. 10, No. 2, pp. 496-501en
dc.identifier.urihttp://hdl.handle.net/2248/1987-
dc.format.extent597269 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherD. Reidel Publishingen
dc.relation.urihttp://adsabs.harvard.edu/abs/1969SoPh...10..496Ben
dc.subjectSolar Winden
dc.subjectSunspot Cycleen
dc.subjectSodium Emissionen
dc.subjectM.K.V. Bappuen
dc.titleSome characteristics of the solar wind inferred from the study of sodium emission from cometary nucleien
dc.typeArticleen
Appears in Collections:M.K. Vainu Bappu ( 1960 - 1982 )

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