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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/622
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dc.contributor.authorAbhyankar, K. D-
dc.contributor.authorSubrahmanyam, P. V-
dc.date.accessioned2005-12-06T09:58:29Z-
dc.date.available2005-12-06T09:58:29Z-
dc.date.issued1984-06-
dc.identifier.citationBASI, Vol. 12, No. 2, pp. 190-195en
dc.identifier.urihttp://hdl.handle.net/2248/622-
dc.description.abstractAn 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.extent281587 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectTotal solar eclipseen
dc.subjectSolar coronaen
dc.subjectAtmospheric turbulenceen
dc.titleCorrection for the observed intensity distribution in solar coronaen
dc.typeArticleen
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