One- and multi-component models of the upper photosphere based on molecular spectra
- 1 September 1973
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 32 (1) , 13-30
- https://doi.org/10.1007/bf00152726
Abstract
No abstract availableKeywords
This publication has 17 references indexed in Scilit:
- A shock tube determination of the CN ground state dissociation energy and the CN violet electronic transition momentJournal of Quantitative Spectroscopy and Radiative Transfer, 1973
- True central intensities of Fraunhofer linesSolar Physics, 1971
- The Harvard-Smithsonian reference atmosphereSolar Physics, 1971
- Description of an observational method for determining absolute intensities in the solar spectrum between ? 2962 and ? 4087Solar Physics, 1970
- The Abundances of the Elements in the Solar Photosphere--I: Carbon, Nitrogen and OxygenMonthly Notices of the Royal Astronomical Society, 1968
- Mechanisms of Populating Electronically Excited CN in Active Nitrogen FlamesThe Journal of Chemical Physics, 1967
- Stellar Molecular Abudances. I. Polyatomic Molecules.The Astrophysical Journal, 1965
- On the Determination of Rotational Temperatures from Solar Lines of Cyanogen.The Astrophysical Journal, 1964
- The Interpretation of Band Spectra. Part IIc. Empirical Band typesReviews of Modern Physics, 1931
- The Quantum Theory of Band Spectra and its Application to the Determination of TemperatureThe Astrophysical Journal, 1922