Can the ion H3 + account for missing opacity in the solar ultraviolet?
- 1 February 1970
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 11 (2) , 198-207
- https://doi.org/10.1007/bf00155220
Abstract
No abstract availableKeywords
This publication has 18 references indexed in Scilit:
- The Dissociation Equilibrium of H- in Stellar AtmospheresMonthly Notices of the Royal Astronomical Society, 1968
- The Abundances of the Elements in the Solar Photosphere--III: SiliconMonthly Notices of the Royal Astronomical Society, 1968
- The Abundances of the Elements in the Solar Photosphere--II: Sodium, Aluminium, Phosphorous, Sulphur and PotassiumMonthly Notices of the Royal Astronomical Society, 1968
- The Bilderberg model of the photosphere and low chromosphereSolar Physics, 1968
- Effects of line blanketing on the solar windowsSolar Physics, 1968
- The Associative Detachment of H and H^{-}The Astrophysical Journal, 1967
- Blanketing approximations for solar modelsJournal of Quantitative Spectroscopy and Radiative Transfer, 1966
- Molecular Schrödinger Equation. IV. Results for One- and Two-Electron SystemsThe Journal of Chemical Physics, 1964
- Configuration-Interaction Study of the Ground State of the H3+ MoleculeThe Journal of Chemical Physics, 1964
- The dissociation energies of the H2, HD, and D2 moleculesJournal of Molecular Spectroscopy, 1961