A composite stellar model of geostrophic flows. II

Details A composite stellar model of geostrophic flows. II A composite stellar model of geostrophic flows. II

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.143...63s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 143, no. 1, April 1988, p. 63-71. Research supported by the Council of Sci

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Geostrophic Wind, Interstellar Matter, Solar Cycles, Space Plasmas, Stellar Models, Thermonuclear Reactions, Computational Astrophysics, Magnetic Field Configurations, Solar Magnetic Field, Solar System

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Mathematical relationships governing highly conducting electromagneto-geostrophic flows are discussed, and the geometry of magnetic field lines is examined. The following cases are considered: (1) J = 0 in the entire region of the flow, (2) the Jacobian (J) not equal to 0 in the entire region of the flow, and (3) J = 0 in one part of the region and J not equal to 0 in the remaining region. It is shown that the common magnetic field line patterns for the cases of J equal to 0 and J not equal to 0 are concentric circles and that the third case (3) cannot exist.

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