Three-dimensional magnetic field configurations in the heliosphere

Details Three-dimensional magnetic field configurations in the heliosphere Three-dimensional magnetic field configurations in the heliosphere

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992jgr....9717183l&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 97, no. A11, p. 17,183-17,188.

Physics

15

Heliosphere, Magnetic Field Configurations, Magnetohydrodynamic Flow, Solar Magnetic Field, Three Dimensional Models, Galactic Cosmic Rays, Magnetohydrodynamics, Radiation Transport, Small Perturbation Flow, Solar Wind

Scientific paper

A class of steady three-dimensional MHD solar wind solutions is constructed from a given primary radial MHD wind which is spherically symmetric, and a systematic procedure is developed for calculating the second-order corrections to the first-order MHD flows. The newly developed 3D MHD wind solutions provide a new theoretical bases for constructing a broad class of magnetic field configurations in the heliosphere by incorporating the solar differential rotation and possible nonaxisymmetric flows over the sun in the presence of a warped heliospheric current sheet, and for developing numerical MHD codes.

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