Contribution and response functions for Caii lines in different atmospheric models
- 1 September 1991
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 135 (1) , 1-13
- https://doi.org/10.1007/bf00146695
Abstract
No abstract availableKeywords
This publication has 10 references indexed in Scilit:
- Changes of the chromosphere model during ?umbral flashes?Solar Physics, 1989
- Formation of chromospheric lines in cool dwarf starsThe Astrophysical Journal, 1987
- On the effect of temperature fluctuations on line intensitiesJournal of Quantitative Spectroscopy and Radiative Transfer, 1983
- A model of a sunspot chromosphere based on OSO 8 observationsThe Astrophysical Journal Supplement Series, 1982
- Structure of the solar chromosphere. III - Models of the EUV brightness components of the quiet-sunThe Astrophysical Journal Supplement Series, 1981
- Solar atmospheric dynamics. I - Formation of optically thick chromospheric linesThe Astrophysical Journal, 1980
- The line response function of stellar atmospheres and the effective depth of line formationSolar Physics, 1975
- Physical properties of solar chromospheric plagesSolar Physics, 1974
- Computation and observation of Zeeman multiplet polarization in Fraunhofer linesSolar Physics, 1974
- Emission cores in H and K linesSolar Physics, 1970