The solar abundance of calcium and collision broadening of Ca i- and Ca ii-Fraunhofer lines by hydrogen
- 1 July 1972
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 25 (1) , 14-29
- https://doi.org/10.1007/bf00155741
Abstract
No abstract availableKeywords
This publication has 31 references indexed in Scilit:
- How well do we know “Cosmic” abundances?Geochimica et Cosmochimica Acta, 1971
- Measurements of atomic lifetimes for neutral and ionized magnesium and calciumJournal of Quantitative Spectroscopy and Radiative Transfer, 1970
- Experimente mit Erdalkaliatomen in metastabilen ZuständenThe European Physical Journal A, 1969
- The Abundances of the Elements in the Solar Photosphere--V: The Alkaline Earths Mg, Ca, Sr, BaMonthly Notices of the Royal Astronomical Society, 1968
- Atomic Oscillator Strengths-III. Alkali-Like SpectraMonthly Notices of the Royal Astronomical Society, 1968
- Lifetimes of 41P1, 41D2, 51D2, 43F4 levels of calcium excited by electron impactsPhysics Letters A, 1967
- The Distinction Between - and Macroturbulence in the Solar Photosphere Using Line ProfilesThe Astrophysical Journal, 1967
- Interpretation of collision broadening and shift in atomic spectraProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1967
- Faint Lines in the Arc Spectrum of Iron (Fe I).Journal of Research of the National Bureau of Standards Section A: Physics and Chemistry, 1961
- Physik der SternatmosphärenPublished by Springer Nature ,1955