Exploring magnetohydrodynamic turbulence on the computer

Details Exploring magnetohydrodynamic turbulence on the computer Exploring magnetohydrodynamic turbulence on the computer

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..431...69t&link_type=abstract

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

Astronomy and Astrophysics

Astrophysics

Magnetohydrodynamics And Plasmas, Accretion And Accretion Disks

Scientific paper

Although numerical simulations have established magnetohydrodynamic turbulence as a possible candidate for the angular momentum transport mechanism in accretion discs there is still a need for a deeper understanding of the physics of the shear-induced turbulence. There are two complementary pathways to this goal, to analyze the results of a simulation at depth or to start from a simple state, whose evolution can be understood by semi-analytical methods and `extrapolate' to the turbulent state that we want to understand. We will show examples of these two approaches.

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