dc.contributor.author |
Tripathi, B. M |
|
dc.contributor.author |
Pande, M. C |
|
dc.contributor.author |
Sinha, K |
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dc.date.accessioned |
2005-02-09T02:27:33Z |
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dc.date.available |
2005-02-09T02:27:33Z |
|
dc.date.issued |
1982-06 |
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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 |
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dc.format.mimetype |
application/pdf |
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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 |