Partially coherent scattering models for the formation of the chromospheric Ca ii K line
- 1 October 1974
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 38 (2) , 367-376
- https://doi.org/10.1007/bf00155074
Abstract
No abstract availableKeywords
This publication has 17 references indexed in Scilit:
- Multi-component models for the formation of the chromospheric Caii K lineSolar Physics, 1972
- Shock Waves and the Interpretation of the Chromospheric Calcium K-linePublications of the Astronomical Society of Australia, 1971
- Emission cores in H and K linesSolar Physics, 1970
- Ca II resonance lines in non-homogeneous chromospheresSolar Physics, 1969
- Emission cores in H and K linesSolar Physics, 1968
- Emission cores in H and K linesSolar Physics, 1968
- Improved Boundary Conditions for the Feautrier MethodThe Astrophysical Journal, 1967
- Non-Coherent Scattering: I. The Redistribution Function with Doppler BroadeningMonthly Notices of the Royal Astronomical Society, 1962
- Noncoherent Scattering due to Collisions. I. Zanstra's Ratio of Coherent to Uncorrelated Noncoherent Scattering.The Astrophysical Journal, 1955
- On the Weakening of the Polarisation Effect by Collision DampingMonthly Notices of the Royal Astronomical Society, 1941