Sunspot continuum from 1 to 10 mum and the umbral temperature models

dc.contributor.author	Punetha, L. M
dc.contributor.author	Joshi, G. C
dc.date.accessioned	2005-12-06T11:28:40Z
dc.date.available	2005-12-06T11:28:40Z
dc.date.issued	1984-09
dc.identifier.citation	BASI, Vol. 12, No. 3, pp. 233-236	en
dc.identifier.uri	http://hdl.handle.net/2248/628
dc.description.abstract	Infrared 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 suggested	en
dc.format.extent	1600157 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Sunspot intensity	en
dc.subject	Line haze opaciy	en
dc.subject	Umbral model	en
dc.title	Sunspot continuum from 1 to 10 mum and the umbral temperature models	en
dc.type	Article	en