Spectroscopic studies of the solar corona during total solar eclipse of October 24, 1995

dc.contributor.author	Ananda Rao, B. G
dc.contributor.author	Ashok, N. M
dc.contributor.author	Chandrasekhar, T
dc.contributor.author	Desai, J. N
dc.contributor.author	Nanda Kumar, M. S
dc.date.accessioned	2006-06-13T11:54:59Z
dc.date.available	2006-06-13T11:54:59Z
dc.date.issued	1997
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 13, pp. 113	en
dc.identifier.issn	0374-3632
dc.identifier.uri	http://hdl.handle.net/2248/1003
dc.description.abstract	We have obtained Fabry-Perot Interferograms of the solar corona during the 1995 total solar eclipse, in two emission lines, Fe X line at 6374Å and Fe XIV line at s303 Å. We have also obtained a Fabry-perot-gram of the corona in the high temperature Ca XV Å line at 569 4 nm. The Co. XV FP-gram showed two concentrated blobs of emission from the equatorial regions of the Sun.
dc.format.extent	864297 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Indian Institute of Astrophysics	en
dc.title	Spectroscopic studies of the solar corona during total solar eclipse of October 24, 1995	en
dc.type	Article	en