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Further evidence for downflow in the solar atmosphere

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Abstract

Downflow velocities of the higher atmospheric layers of the Sun are derived from wavelength measurements of the Mg ii core absorption.

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References

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Authors and Affiliations

  1. Max Planck Institut für Radioastronomie, Bonn, F.R.G.

    A. Greve

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  1. A. Greve
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Greve, A. Further evidence for downflow in the solar atmosphere. Sol Phys 58, 287–289 (1978). https://doi.org/10.1007/BF00157273

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  • DOI: https://doi.org/10.1007/BF00157273

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