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Structure of the Solar Chromosphere. Basic Computations and Summary of the Results

  • Vernazza J
  • Avrett E
  • Loeser R
The Astrophysical Journal (1973) 184 605
DOI: 10.1086/152353
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Abstract

A procedure is demonstrated that is used to compute a one-component model of the solar atmosphere, including in that model the photosphere, chromosphere, and chromosphere-corona transition zone. In particular, the equations are described that are solved in order to determine this theoretical model.

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Vernazza, J. E., Avrett, E. H., & Loeser, R. (1973). Structure of the Solar Chromosphere. Basic Computations and Summary of the Results. The Astrophysical Journal, 184, 605. https://doi.org/10.1086/152353

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