Abstract
The analysis of three Ca ii K-spectra with spatial resolution of ∼1″ is described and its results presented. The comparison of the observed single peak line profiles with model computation leads to some conclusions regarding the non-uniform large-scale velocity fields in the chromosphere.
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Mitteilungen aus dem Fraunhofer Institut No. 128.
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Grossmann-Doerth, U., Kneer, F. & Uexküll, M.v. Properties of the solar Ca ii K-Line at high spatial resolution. Sol Phys 37, 85–97 (1974). https://doi.org/10.1007/BF00157846
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DOI: https://doi.org/10.1007/BF00157846