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CH in the Solar Spectrum
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.
| Автори: | , |
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| Формат: | Online Стаття Текст |
| Мова: | English |
| Опубліковано: |
[Gaithersburg, MD] : U.S. Dept. of Commerce, National Institute of Standards and Technology
1959
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| Предмети: | |
| Онлайн доступ: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5287100/ https://www.ncbi.nlm.nih.gov/pubmed/31216139 http://dx.doi.org/10.6028/jres.063A.002 |