Stability of an isothermal disk with three-dimensional magnetic fields and radial viscous force.

Details Stability of an isothermal disk with three-dimensional magnetic fields and radial viscous force. Stability of an isothermal disk with three-dimensional magnetic fields and radial viscous force.

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cotph..33..301d&link_type=abstract

Commun. Theor. Phys., Vol. 33, No. 2, p. 301 - 308

Other

Quasars: Variability

Scientific paper

The stability of an isothermal thin disk with three-dimensional magnetic fields and radial viscous force is examined. The authors find that the radial viscous force has no influence on the stability of viscous modes. However, there is more influence on the stability of magneto-acoustic modes, which is related to the perturbation wavelength and different parts of disk. Finally, the authors use their model to explain the long-term variability of the quasar 3C 345.

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