Three-dimensional model calculations for the solar wind

Details Three-dimensional model calculations for the solar wind Three-dimensional model calculations for the solar wind

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977phdt.........1r&link_type=abstract

Braunschweig, Technische Universitaet, Naturwissenschaftliche Fakultaet, Doktor der Naturwissenschaften Dissertation, 1977. 176

Other

3

Digital Simulation, Dynamic Models, Solar Wind, Stellar Models, Three Dimensional Flow, Three Dimensional Models, Gas Expansion, Helios 1, Interplanetary Magnetic Fields, Photosphere, Solar Corona, Solar Magnetic Field, Solar Wind Velocity

Scientific paper

The reasons for using a three-dimensional model of the solar wind are explained. It is shown that knowledge of a certain component of the magnetic field permits the development of a single-value spherical function, so that the spherical function coefficients over the orthogonality relations can be characterized. When a certain plausible temperature curve is used in conjunction with the Spitzer-Haerm thermal conductivity in the solar wind, false values of other solar wind parameters are generated. The effects caused by the different geometries of flow tubes in the center and the boundary of a sector are described. Model calculations are examined with reference to data obtained by Helios-1.

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