CH in the solar spectrum
- 1 July 1959
- journal article
- Published by National Institute of Standards and Technology (NIST) in Journal of Research of the National Bureau of Standards Section A: Physics and Chemistry
- Vol. 63A (1) , 19-53
- https://doi.org/10.6028/jres.063a.002
Abstract
CH lines in the solar spectrum have been identified by direct comparison of measured laboratory and solar wavelengths and intensities. The comparisons of individual rotational lines are included in a series of tables arranged according to electronic and vibrational transitions.Keywords
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