| 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 | |
| dc.format.mimetype | application/pdf | |
| 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 |