Carbon monoxide and facula models

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/336

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DC Field	Value	Language
dc.contributor.author	Tripathi, B. M	-
dc.contributor.author	Pande, M. C	-
dc.contributor.author	Sinha, K	-
dc.date.accessioned	2005-02-09T02:27:33Z	-
dc.date.available	2005-02-09T02:27:33Z	-
dc.date.issued	1982-06	-
dc.identifier.citation	BASI, Vol. 10, No. 2, pp. 150-153	en
dc.identifier.uri	http://hdl.handle.net/2248/336	-
dc.description.abstract	Equivalent widths for a new lines of the first overtone band of carbon monoxide have been calculated in the solar infrared spectrum for five facular and two photospheric models. The calculations show a decrease in equilavent withds in the facular models of Stellmacher & Wiehr (1973), Stenflo (1975) and Chapman (1979) and an increase in the models of Schmahl (1967) and Shine & Linsky (1974). The modles are also discussed in the light of Polonskij's (1966) and Tsuji's (1977) observations.	en
dc.format.extent	290770 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Astronomical Society of India	en
dc.subject	Carbon monoxide	en
dc.subject	equalivent widths	en
dc.subject	facula models	en
dc.title	Carbon monoxide and facula models	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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