Magnetohydrodynamic Turbulence in Accretion Discs

Details Magnetohydrodynamic Turbulence in Accretion Discs Magnetohydrodynamic Turbulence in Accretion Discs

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000iaus..195..241t&link_type=abstract

Highly Energetic Physical Processes and Mechanisms for Emission from Astrophysical Plasmas, Proceedings of IAU Symposium #195, h

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present results from numerical simulations of magnetohydrodynamic
turbulence in accretion discs. Our simulations show that the turbulent
stresses that drive the accretion are less stratified than the matter;
thus, the surface layers are more strongly heated than the interior of
the disc.

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