C. Beck, R. Rezaei, K. G. Puschmann
Abstract
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Context. The Ca ii H line is one of the strongest lines in the solar spectrum, and it provides continuous information on the solar atmosphere from the photosphere to the lower chromosphere.
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Context. The Ca ii H line is one of the strongest lines in the solar spectrum, and it provides continuous information on the solar atmosphere from the photosphere to the lower chromosphere.
Key concepts: Chromosphere, Spectral line, Photosphere, Physics, Radiative transfer, Inversion (geology), Astrophysics, Line (geometry)