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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/628
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dc.contributor.authorPunetha, L. M-
dc.contributor.authorJoshi, G. C-
dc.date.accessioned2005-12-06T11:28:40Z-
dc.date.available2005-12-06T11:28:40Z-
dc.date.issued1984-09-
dc.identifier.citationBASI, Vol. 12, No. 3, pp. 233-236en
dc.identifier.urihttp://hdl.handle.net/2248/628-
dc.description.abstractInfrared flux in Zwaan`s (1974) and Boyer`s (1980) sunspot models has been calculated in the wavelength range 1 to 10 mu m, taking into account the molecular line haze opacity (Joshi et al. 1979). The calculations are compared with Sitnik`s (1980) observations in the available wavelenght region 1 to 2.1 mu m and corrections in the corresponding models are suggesteden
dc.format.extent1600157 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectSunspot intensityen
dc.subjectLine haze opaciyen
dc.subjectUmbral modelen
dc.titleSunspot continuum from 1 to 10 mum and the umbral temperature modelsen
dc.typeArticleen
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