Correction for the observed intensity distribution in solar corona

dc.contributor.author	Abhyankar, K. D
dc.contributor.author	Subrahmanyam, P. V
dc.date.accessioned	2005-12-06T09:58:29Z
dc.date.available	2005-12-06T09:58:29Z
dc.date.issued	1984-06
dc.identifier.citation	BASI, Vol. 12, No. 2, pp. 190-195	en
dc.identifier.uri	http://hdl.handle.net/2248/622
dc.description.abstract	An estimation of the correction for the broadening of the intensity profile of the solar corona caused by atmospheric turbulence, scattering in the photographic emulsion, focusing errors etc, is made from the coronal observations of the sun during 1980 Februuary 16 total solar eclipse.	en
dc.format.extent	281587 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Total solar eclipse	en
dc.subject	Solar corona	en
dc.subject	Atmospheric turbulence	en
dc.title	Correction for the observed intensity distribution in solar corona	en
dc.type	Article	en