A three-component model for the formation of the chromospheric Caii K line
- 1 November 1970
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 15 (1) , 139-147
- https://doi.org/10.1007/bf00149480
Abstract
No abstract availableKeywords
This publication has 7 references indexed in Scilit:
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- Ca II resonance lines in non-homogeneous chromospheresSolar Physics, 1969
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- A measurement of the solar H and K profilesSolar Physics, 1968
- The solar H and K lines of ionized calciumSolar Physics, 1968
- The Structure of the Solar Chromosphere: I. Identification of Spicules on the DiskMonthly Notices of the Royal Astronomical Society, 1965
- The Double Reversal in the Cores of the Fraunhofer H and K Lines.The Astrophysical Journal, 1959