CCD Observations of the Total Solar Eclipse of October 24, 1995

dc.contributor.author	Verma, V. K
dc.contributor.author	Wahab Uddin
dc.contributor.author	Gaur, V. P
dc.contributor.author	Joshi, G. C
dc.contributor.author	Bondal, K. R
dc.date.accessioned	2005-01-17T10:35:07Z
dc.date.available	2005-01-17T10:35:07Z
dc.date.issued	1997
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 13, pp. 29-35	en
dc.identifier.issn	0374-3632
dc.identifier.uri	http://hdl.handle.net/2248/236
dc.description.abstract	The observations of the solar corona during the Total Solar Eclipse of October 24, 1995 were attempted in white light and in narrow band filters with peak wavelenghts centered at 5303 Armstrong (FeXIV) and at 6474 Armstrong [Fe X], the coronal emission lines. The site for the observations of the eclipse was the campus of Jawahar Navodaya Vidyalaya, Meja Khas, Allahabad (longitude: 82 degree 07 minutes 32.5 seconds E, lattitude: 25 degree 07 minutes 36.4 seconds N, and altitude of about 134 meters above msl). The equipment used for the observations is briefly discussed. Nine coronal images in the red line were successfully obtained. The preliminary results of the observations are also presented.	en
dc.format.extent	178330 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Total solar eclipse	en
dc.subject	Coronal emission lines	en
dc.subject	Electron density	en
dc.title	CCD Observations of the Total Solar Eclipse of October 24, 1995	en
dc.type	Article	en