D. E. Rees, G. J. Saliba
Abstract
The Ca II K line serves as an important tool in determining the physics of the photosphere-chromosphere region of the solar atmosphere (Cram 1983). To date detailed analyses have centred on the study of line intensity profiles.
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The Ca II K line serves as an important tool in determining the physics of the photosphere-chromosphere region of the solar atmosphere (Cram 1983). To date detailed analyses have centred on the study of line intensity profiles.
Key concepts: Chromosphere, Physics, Solar atmosphere, Photosphere, Solar physics, Line (geometry), Polarization (electrochemistry), Coronal radiative losses