The radial-azimuthal instability of an isothermal magnetized accretion disk.

Details The radial-azimuthal instability of an isothermal magnetized accretion disk. The radial-azimuthal instability of an isothermal magnetized accretion disk.

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cotph..30..269y&link_type=abstract

Commun. Theor. Phys., Vol. 30, No. 2, p. 269 - 274

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Accretion Disks: Instabilities

Scientific paper

The radial-azimuthal instability of an isothermal magnetized accretion disk is examined. The authors find that the azimuthal perturbation enhances the instability of the magneto-acoustic and non-axisymmetric modes. The magnetic field induces and enhances the instability of magneto-acoustic modes, but stabilizes the non-axisymmetric modes in the outer disk. The viscous modes are always stable. The instability of magneto-acoustic modes are dominant in this disk.

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