CH in the solar spectrum

descriptionPublicationkeyboard_double_arrow_right Article 01 Jul 1959 English Publisher:National Institute of Standards and Technology (NIST)Journal:Journal of Research of the National Bureau of Standards Section A: Physics and Chemistry, volume 63A, page 19 (issn: 0022-4332,

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Authors: Moore, Charlotte E.; Broida, Herbert P.;

doi: 10.6028/jres.063a.002 , 10.6028/jres.063a.023

pmid: 31216139 , 31216137

pmc: PMC5287100 , PMC5287041

CH in the solar spectrum

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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.

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