Magnetic flux tubes above the surface of accretion disks - Effect of the Coriolis force

Details Magnetic flux tubes above the surface of accretion disks - Effect of the Coriolis force Magnetic flux tubes above the surface of accretion disks - Effect of the Coriolis force

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993astl...19..184m&link_type=abstract

Astronomy Letters, Vol. 19, p. 184-187; Pis'ma v Astronomicheskij Zhurnal (ISSN 0320-0108), vol. 19, no. 5, p. 473-480. In Russ

Astronomy and Astrophysics

Astronomy

Coriolis Effect, Magnetic Field Reconnection, Magnetic Flux, Plasma Dynamics, Stellar Magnetic Fields, Accretion Disks, Angular Velocity, Momentum Transfer

Scientific paper

The study determines a 3D stationary configuration of a magnetic flux tube characterized by the presence of a special point in which two different sectors of the tube come into contact. The calculation takes into account the Coriolis force, which acts on the tube with a moving plasma. The Coriolis forces is comparable in magnitude to the buoyancy force or exceeds it, and is directed perpendicularly to it. The dissipative separation from the disk and the rising of these closed magnetic flux tubes with a circulating plasma inside result in the effective transfer of the angular momentum from an accretion disk to the ambient hot halo.

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