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Model Calculations of the Photospheric Layers of Solar Magnetic Fluxtubes

  • Oskar Steiner
  • J. O. Stenflo
Part of the International Astronomical Union book series (IAUS, volume 138)

Abstract

Multi-dimensional radiative energy transport is coupled self-consistently to magnetohydrostatic solutions for fluxtubes with rotational symmetry. It is shown that the photospheric layers of plage and network fluxtubes are heated by radiation by as much as 300 K at equal geometrical height. The amount of heating depends on the density reduction within the tube. The results are compared with observational data and the most recent semi-empirical model.

Keywords

Current Sheet Radiative Transfer Equation Solar Photosphere Thin Current Sheet Heavy Solid Line 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© International Astronomical Union 1990

Authors and Affiliations

  • Oskar Steiner
    • 1
  • J. O. Stenflo
    • 1
  1. 1.Institut für AstronomieETH-ZentrumZurichSwitzerland

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