Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.210..109y&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 210, no. 1-2, p. 109-111 (IAU Colloquium 134)
Astronomy and Astrophysics
Astrophysics
Accretion Disks, Black Holes (Astronomy), Field Strength, Magnetic Fields, Magnetohydrodynamic Flow, Astrophysics, Nonlinearity, Plasma Waves, Stellar Rotation
Scientific paper
The paper is an investigation of the magnetohydrodynamics (MHD) of the quasi-radial accretion onto a rotating black hole. It is demonstrated that the nonlinear effects in the accretion flow accelerate the rate of expansion of the Alfven mode. The accretion flow becomes unstable at the weak strength of magnetic field which is about one-thirtieth of the expected value by the linear theory.
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