Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1976
Full metadata record
DC FieldValueLanguage
dc.contributor.authorBappu, M. K. V-
dc.contributor.authorBhattacharyya, J. C-
dc.contributor.authorSivaraman, K. R-
dc.date.accessioned2007-11-24T08:13:08Z-
dc.date.available2007-11-24T08:13:08Z-
dc.date.issued1972-10-
dc.identifier.citationSolar Physics, Vol. 26, No. 2, pp. 366-369en
dc.identifier.urihttp://hdl.handle.net/2248/1976-
dc.description.abstractEmission lines of the Balmer series, D3 and H and K are reported present on a coronal spectrogram obtained at the March 7, 1970 eclipse. Arguments are presented to show that these could not have originated from scattering in the Earth's atmosphere and hence possibly have a coronal origin.en
dc.format.extent407390 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherD. Reidel Publishingen
dc.relation.urihttp://adsabs.harvard.edu/abs/1972SoPh...26..366Ben
dc.subjectEmission Linesen
dc.subjectSolar Coronaen
dc.subjectCoronal Spectraen
dc.subjectM.K.V. Bappuen
dc.titleOn emission lines of hydrogen, helium and ionized calcium seen on a coronal spectrogram of the march 7, 1970 eclipseen
dc.typeArticleen
Appears in Collections:J.C.Bhattacharyya (1982 - 1990)
M.K. Vainu Bappu ( 1960 - 1982 )

Files in This Item:
File Description SizeFormat 
bappu.vol..26.pdf397.84 kBAdobe PDFThumbnail
View/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.