dc.contributor.author | Tripathi, B. M. | |
dc.contributor.author | Sinha, K. | |
dc.date.accessioned | 2010-02-22T09:11:13Z | |
dc.date.available | 2010-02-22T09:11:13Z | |
dc.date.issued | 1986 | |
dc.identifier.uri | http://hdl.handle.net/123456789/562 | |
dc.description.abstract | Predicted equivalent widths and profiles of facular CN lines are used here as a diagnostic tool for different model atmospheres. | en_US |
dc.language.iso | en | en_US |
dc.relation.ispartofseries | sp106-43 | |
dc.subject | Sun Atmosphere | en_US |
dc.title | Cyanogen lines and facula models | en_US |
dc.type | Article | en_US |