A three-dimensional magnetohydrodynamic formalism for coronal helmet streamers

Details A three-dimensional magnetohydrodynamic formalism for coronal helmet streamers A three-dimensional magnetohydrodynamic formalism for coronal helmet streamers

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...404..356c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 404, no. 1, p. 356-371.

Astronomy and Astrophysics

Astrophysics

6

Magnetohydrodynamics, Solar Corona, Three Dimensional Models, Current Density, Hydrodynamic Equations, Iterative Solution, Magnetic Field Configurations, Solar Magnetic Field, Solar Wind, Two Dimensional Models

Scientific paper

A 3D MHD formulation of the steady state coronal helmet-streamer problem is presented. It includes the simple azimuthally symmetric and two-dimensional cases. The major mathematical difficulty - the correct, iterative calculation of the transverse electrical currents, which are the sources of the fields in Maxwell's equations - is eliminated by the elaboration of an algorithm connecting four different coordinate spaces.

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