Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/620
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dc.contributor.authorSinha, K-
dc.date.accessioned2005-12-06T09:35:08Z-
dc.date.available2005-12-06T09:35:08Z-
dc.date.issued1984-06-
dc.identifier.citationBASI, Vol. 12, No. 2, pp. 172-181en
dc.identifier.urihttp://hdl.handle.net/2248/620-
dc.description.abstractUtilizing the KPNO atlas (Brault & Testerman 1972) for the (0-0) band of the Swan system of the C/sub2/ molecules, we determine rotational temperatures T/subrot/, for mu = 1.0 and mu = 0.2. When saturation in the observed equivalent widths is accounted for, the model-based result for T/subrot/ comes out slightly lower than observations at a near limb position (mu = 0.2). There is no evidence for an increase in temperature towards the solar limb discussed earlier (Sinha 1979a, b).en
dc.format.extent729808 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectSolar Spectrumen
dc.subjectC2 moleculesen
dc.subjectRotational temperatureen
dc.subjectModel atmosphereen
dc.titleCenter-to-limb behaviour of molecular rotational temperatures IIIen
dc.typeArticleen
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