Correction for the observed intensity distribution in solar corona

Abhyankar, K. D. ; Subrahmanyam, P. V. (1984) Correction for the observed intensity distribution in solar corona Bulletin of the Astronomical Society of India, 12 (2). pp. 190-195. ISSN 0304-9523

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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.

Item Type:Article
Source:Copyright of this article belongs to Astronomical Society of India.
Keywords:Total Solar Eclipse; Solar Corona; Atmosphere Turbulence
ID Code:24010
Deposited On:01 Dec 2010 12:45
Last Modified:17 May 2016 07:47

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