On emission lines of hydrogen, helium and ionized calcium seen on a coronal spectrogram of the march 7, 1970 eclipse

Bappu, M. K. V; Bhattacharyya, J. C; Sivaraman, K. R

dc.contributor.author	Bappu, M. K. V
dc.contributor.author	Bhattacharyya, J. C
dc.contributor.author	Sivaraman, K. R
dc.date.accessioned	2007-11-24T08:13:08Z
dc.date.available	2007-11-24T08:13:08Z
dc.date.issued	1972-10
dc.identifier.citation	Solar Physics, Vol. 26, No. 2, pp. 366-369	en
dc.identifier.uri	http://hdl.handle.net/2248/1976
dc.description.abstract	Emission 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.extent	407390 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	D. Reidel Publishing	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1972SoPh...26..366B	en
dc.subject	Emission Lines	en
dc.subject	Solar Corona	en
dc.subject	Coronal Spectra	en
dc.subject	M.K.V. Bappu	en
dc.title	On emission lines of hydrogen, helium and ionized calcium seen on a coronal spectrogram of the march 7, 1970 eclipse	en
dc.type	Article	en