Magnetic shear instability for accretion tori of constant specific angular momentum

Details Magnetic shear instability for accretion tori of constant specific angular momentum Magnetic shear instability for accretion tori of constant specific angular momentum

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..431...65p&link_type=abstract

Accretion processes in astrophysical systems: Some like it hot! - eigth astrophysics conference. AIP Conference Proceedings, Vo

Astronomy and Astrophysics

Astrophysics

Accretion And Accretion Disks, Magnetohydrodynamics And Plasmas

Scientific paper

The global linear stability of a thick accretion disc with a torus shape versus the magnetic shear instability is studied through numerical simulations. The model consists of a torus disc with constant specific angular momentum embedded in a vertical, uniform, external magnetic field. The effects of density and temperature stratification are included via the anelastic approximation.

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