Determination of constant-alpha force-free magnetic fields above the photosphere using three-component boundary conditions

Details Determination of constant-alpha force-free magnetic fields above the photosphere using three-component boundary conditions Determination of constant-alpha force-free magnetic fields above the photosphere using three-component boundary conditions

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...216..265c&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 216, no. 1-2, June 1989, p. 265-277.

Statistics

Computation

14

Boundary Conditions, Force-Free Magnetic Fields, Magnetic Field Configurations, Magnetohydrodynamics, Photosphere, Solar Magnetic Field, Chromosphere, Computational Astrophysics, Electric Current, Solar Corona

Scientific paper

The constant-α, force-free magnetic field equations are
numerically integrated for the case in which all three field components
are specified at the photo sphere and used as boundary conditions.
Test-cases successfully compare the numerical results with exact
analytical values.

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