Three-dimensional magnetostatic models of the large-scale corona

Details Three-dimensional magnetostatic models of the large-scale corona Three-dimensional magnetostatic models of the large-scale corona

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nascp2442..275b&link_type=abstract

In NASA. Goddard Space Flight Center Coronal and Prominence Plasmas p 275-278 (SEE N87-20871 13-92)

Mathematics

Equilibrium Equations, Magnetostatic Fields, Photosphere, Solar Corona, Solar Flux Density, Thomson Scattering, Three Dimensional Models, Coronagraphs, Electric Current, Solar Magnetic Field, Solar Rotation, Synoptic Measurement

Scientific paper

A special class of magnetostatic equilibria is described, which are mathematically simple and yet sufficiently versatile so as to fit any arbitrary normal magnetic flux prescribed at the photosphere. With these solutions, the corona can be modeled with precisely the same mathematically simple procedure as has previously been done with potential fields. The magnetostatic model predicts, in addition to the coronal magnetic field, the three dimensional coronal density which can be compared with coronagraph observations.

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