Brightness, polarization and electron density of the solar corona of 1980 February 16

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3787

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DC Field	Value	Language
dc.contributor.author	Sivaraman, K. R	-
dc.contributor.author	Jayachandran, M	-
dc.contributor.author	Scaria, K. K	-
dc.contributor.author	Babu, G. S. D	-
dc.contributor.author	Bagare, S. P	-
dc.contributor.author	Jayarajan, A. P	-
dc.date.accessioned	2008-09-22T16:28:22Z	-
dc.date.available	2008-09-22T16:28:22Z	-
dc.date.issued	1984-06	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol. 5, No. 2, pp. 149 - 158	en
dc.identifier.issn	0250-6335	-
dc.identifier.uri	http://hdl.handle.net/2248/3787	-
dc.description.abstract	During the eclipse of 1980 February 16 the authors photographed the solar corona at an effective wavelength of 6300 Å. Using a quadruple camera coronal pictures were obtained in polarized light for four polaroid orientations. These observations are used to derive the coronal brightness and polarization and from these the electron densities in the corona out to a distance of about 2.5 R_sun; from the centre of the disc. The coronal brightness matches well with that of the corona of 1958 October 12.	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://ads.ari.uni-heidelberg.de/abs/1984JApA....5..149S	en
dc.subject	Electron Density (Concentration)	en
dc.subject	Solar Corona	en
dc.subject	Solar Eclipses	en
dc.subject	Astronomical Photography	en
dc.subject	Brightness	en
dc.subject	Linear Polarization	en
dc.title	Brightness, polarization and electron density of the solar corona of 1980 February 16	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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