Convergence Study of the Magnetorotational Instability in a Shearing Box With a Mean Field

Details Convergence Study of the Magnetorotational Instability in a Shearing Box With a Mean Field Convergence Study of the Magnetorotational Instability in a Shearing Box With a Mean Field

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sf2a.conf..107s&link_type=abstract

SF2A-2006: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: D. Barret, F. Casoli, G.

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

For more than a decade the so-called shearing box model has been used to study the fundamental dynamics of accretion discs. Such an approach is particularly useful when numerical simulations at high resolutions are needed. However, it is often difficult to know how reliable a numerically obtained quantity is, especially if the underlying flow is turbulent. Here we present some results from a resolution study, which is designed to address this issue directly.

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