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Magnetohydrodynamic Turbulence in Accretion Discs
Published online by Cambridge University Press: 25 May 2016
Abstract
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We present results from numerical simulations of magneto-hydrodynamic 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.
- Type
- Part I: Talks
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- Copyright
- Copyright © Astronomical Society of the Pacific 2000
References
Torkelsson, U., Ogilvie, G. I., Brandenburg, A., Pringle, J. E., Nordlund, Å., & Stein, R. F.
2000, MNRAS, submitted.Google Scholar