On the theory of rotating magnetic stars. Part 1.

Details On the theory of rotating magnetic stars. Part 1. On the theory of rotating magnetic stars. Part 1.

Jan 1954

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1954cokon..32....1c&link_type=abstract

Communications of the Konkoly Observatory, No. 32 (Vol. III, 11), p. 1-9 (1954).

Computer Science

Magnetic Stars, Stars: Rotation

Scientific paper

The kinetical equations of stars considered as conducting gases may he written under very general conditions. These equations not only permit the consideration of axial rotation and of meridional currents but they also offer an utterly general structure for the magnetic field. Together with the component of the magnetic field parallel to the meridional plane (mentioned in the following as "meridional component"), the component perpendicular to the meridional plane (phi-component) may be introduced as well. The introduction of the latter may be only necessitated by the general hydro- and electrodynamical conditions.

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