Sunspot Continuum from 1 to 10 µm and the umbral temperature models

dc.contributor.author	Punetha, L. M.
dc.contributor.author	Joshi, G. C.
dc.date.accessioned	2010-08-19T08:53:36Z
dc.date.available	2010-08-19T08:53:36Z
dc.date.issued	1984
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/736
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 µm, taking into account the molecular line haze opacity (Joshi et al. 1979). The calculations are compared with Sitnik's (1980) observations in the available wavelength region 1to 2.1 µm and correction in the corresponding models are suggested.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi12-233
dc.subject	Sunspot intensity, Line haze opaciy, Umbral model	en_US
dc.title	Sunspot Continuum from 1 to 10 µm and the umbral temperature models	en_US
dc.type	Article	en_US