dc.contributor.author |
Tripathi, B. M |
|
dc.contributor.author |
Pande, M. C |
|
dc.date.accessioned |
2005-02-05T04:49:44Z |
|
dc.date.available |
2005-02-05T04:49:44Z |
|
dc.date.issued |
1981-12 |
|
dc.identifier.citation |
BASI, Vol. 9, No. 4, pp. 287-290 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/323 |
|
dc.description.abstract |
An attempt has been made to show that the profile of the Brackett-gamma line can distinguish between different facula models. It is suggested that low noise high resolution scans of Brackett lines can help improve the existing facula models. |
en |
dc.format.extent |
258005 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 |
Brackett line |
en |
dc.subject |
facula models |
en |
dc.title |
Brackett-gamma line and facula models |
en |
dc.type |
Article |
en |