Krishna Swamy, K. S. (1975) Equivalent width of molecular lines in stars. I: Lyman and Werner bands of H2 in the solar atmosphere Solar Physics, 41 (2). pp. 301-312. ISSN 0038-0938
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Official URL: http://www.springerlink.com/content/h3767514788404...
Related URL: http://dx.doi.org/10.1007/BF00154068
Abstract
The expected equivalent widths of the individual rotational lines of the Lyman and Werner bands of the hydrogen molecule from the solar atmosphere have been calculated. These results are used to predict what one expects to observe with a specified wavelength bandpass. These are compared with the observation of Dupree and Reeves.
Item Type: | Article |
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Source: | Copyright of this article belongs to Springer-Verlag. |
ID Code: | 18296 |
Deposited On: | 17 Nov 2010 12:50 |
Last Modified: | 17 May 2016 03:01 |
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