The solar H and K lines of ionized calcium
- 1 January 1968
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 3 (1) , 164-180
- https://doi.org/10.1007/bf00154252
Abstract
No abstract availableKeywords
This publication has 13 references indexed in Scilit:
- Velocity Fields in the Solar Atmosphere. III. Large-Scale Motions, the Chromospheric Network, and Magnetic Fields.The Astrophysical Journal, 1964
- The Origin of the Emission Reversals in the Fraunhofer h- and K-LinesThe Astrophysical Journal, 1964
- Observational Study of Macroscopic Inhomogeneities in the Solar Atmosphere.IV. Velocity and Intensity Fluctuations Observed in the K Line.The Astrophysical Journal, 1963
- A New Model of the ChromosphereProceedings of the Japan Academy, 1963
- The Elimination of Scattered Light in Solar SpectrographsApplied Optics, 1962
- The Source Function in a Non-Equilibrium Atmosphere. V. Character of the Selfreversed Emission FO CA^{+} H and K.The Astrophysical Journal, 1960
- Observations of Solar Magnetic Fields in Plage Regions.The Astrophysical Journal, 1959
- Observations of Solar Magnitic Fields.The Astrophysical Journal, 1959
- The Double Reversal in the Cores of the Fraunhofer H and K Lines.The Astrophysical Journal, 1959
- The Sun's Magnetic Field, 1952-1954.The Astrophysical Journal, 1955