Analysis of Skylab/Apollo Telescope Mount S-056 observations based on a force-free magnetic field model

Astronomy and Astrophysics – Astronomy

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Apollo Telescope Mount, Force-Free Magnetic Fields, Skylab Program, Solar Atmosphere, Solar Magnetic Field, Spaceborne Astronomy, Astronomical Models, Atmospheric Models, Chromosphere, Photographic Recording, Satellite Observation, Solar Corona, Solar X-Rays, X Ray Analysis

Scientific paper

Data obtained from the S-056 X-ray experiment on Skylab/ATM have been analyzed based on the assumption that the magnetic fields in the chromosphere and lower corona are force-free. Underlying the analysis is the hypothesis that the observed X-ray filaments coincide with magnetic field lines. The photographic recording of the filaments can then be compared with the projection along the line of sight of the computed magnetic field lines of the model. Ground-based observations of the longitudinal magnetic field component complement the X-ray data and are used in the theoretical interpretation.

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