Linear force-free magnetic fields for solar extrapolation and interpretation

Details Linear force-free magnetic fields for solar extrapolation and interpretation Linear force-free magnetic fields for solar extrapolation and interpretation

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apjs...69..323g&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 69, Feb. 1989, p. 323-348. Research supported by USAF.

Physics

91

Force-Free Magnetic Fields, Magnetohydrodynamics, Solar Activity, Solar Atmosphere, Solar Magnetic Field, Current Density, Field Theory (Physics), Nonlinear Equations, Photosphere

Scientific paper

This paper discusses the interconnection of the various linear force-free magnetic field formulations, the specific phenomenological and topological parameters of these formulations, and their usefulness. Particularly, the limitations and usefulness of linear force-free fields are discussed. Specific field configurations are related to magnetographic interpretation. The relationship of the integral and Fourier procedures is shown explicitly. The physical interpretation of linear force-free fields is shown by analytic models and from the Marshall Space Flight Center solar vector magnetograms.

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