Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.112..287k&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 112, no. 2, May 1985, p. 287-301.
Astronomy and Astrophysics
Astrophysics
1
Self Consistent Fields, Space Plasmas, Stellar Magnetic Fields, Stellar Magnetospheres, Stellar Winds, Corotation, Inertia, Ohms Law, Plasma Drift, Pulsars
Scientific paper
Kaburaki's (1985) self-consistent solution method for three-dimensional stellar wind problems is noted to be exemplified in a nearly corotating inner magnetosphere. Drift motion around the magnetic axis, which is a manifestation of inertial effects, is determined self-consistently with the electromagnetic field, yielding explicit expressions for the energy integral in the rotating frame and for the density distribution. These expressions possess a fundamental length which is to be evaluated according to physical conditions of a magnetosphere, and which determines the asymptotic-kinetic energy of a plasma particle at infinity. The integrated Ohm's law is used to describe a force balance in the rotating frame, in the limits of weak and strong magnetic fields.
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