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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/279
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dc.contributor.authorPande, M. C-
dc.contributor.authorGaur, V. P-
dc.contributor.authorBondal, K. R-
dc.contributor.authorDubey, R. C-
dc.date.accessioned2005-02-03T02:37:15Z-
dc.date.available2005-02-03T02:37:15Z-
dc.date.issued1980-03-
dc.identifier.citationBASI, Vol. 8, No. 1, pp. 27-29en
dc.identifier.urihttp://hdl.handle.net/2248/279-
dc.description.abstractSpectrophotoelectric observations of the CH lines have been presented to determine the centre-to-limb behaviour of rotational temperatures for the (0-0) and (1-1) bands of the electronic transition A(power 2 delta) - X (power 2 pi) of the molecules. Taking into account the large probable errors in measurements, we find that the rotational remperature from centre to limb appears practically constant. Further accurate observations upto the extreme limb with a larger set of data appears necessary in order to minimise the probable errors.en
dc.format.extent353233 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectCH Moleculesen
dc.subjectSolar Photosphereen
dc.titleCentre to Limb Variation of Rotational Temperature of the CH Molecules in the Solar Photosphereen
dc.typeArticleen
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