Energetics in MRI driven turbulence

Thomas A. Gardiner, James McLellan Stone

Research output: Chapter in Book/Report/Conference proceedingConference contribution

17 Scopus citations

Abstract

In these proceedings we present recent efforts to understand the energetics of magneto-hydrodynamic (MHD) turbulence driven by the magneto-rotational instability (MRI). These studies are carried out in the local (shearing box) approximation using the Athena simulation code. Athena is a higher order Godunov algorithm based on the piecewise parabolic method (PPM), the corner transport upwind (CTU) integration algorithm, and the constrained transport (CT) algorithm for evolving the magnetic field. This algorithm is particularly suited for these studies owing to the conservation properties of a Godunov scheme and the particular implementation of the shearing box source terms used here. We present a variety of calculations which may be compared directly to previously published results and discuss them in some detail. The only significant discrepancy found between the results presented here and in the published literature involves the turbulent heating rate. We observe the presence of recurrent channel solutions in calculations involving a mean vertical magnetic field and the associated time lag between the energy injection and thermalization rate. We also present the results of a shearing box calculation which includes an optically thin radiative term with a cooling rate selected to match the turbulent heating rate. Some properties which we find uniformly present in all of the calculations presented here are compressible fluctuations, spiral waves and weak shocks. It is found that these compressible modes dominate the temporal fluctuations in the probability distribution functions for most of the thermodynamic variables; only the specific entropy is relatively immune to their effects.

Original languageEnglish (US)
Title of host publicationMAGNETIC FIELDS IN THE UNIVERSE
Subtitle of host publicationFrom Laboratory and Stars to Primordial Structures
Pages475-488
Number of pages14
DOIs
StatePublished - Sep 28 2005
EventMAGNETIC FIELDS IN THE UNIVERSE: From Laboratory and Stars to Primordial Structures - Angra dos Reis, Brazil
Duration: Nov 28 2004Dec 3 2004

Publication series

NameAIP Conference Proceedings
Volume784
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

OtherMAGNETIC FIELDS IN THE UNIVERSE: From Laboratory and Stars to Primordial Structures
CountryBrazil
CityAngra dos Reis
Period11/28/0412/3/04

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

Keywords

  • Accretion disks
  • MHD

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    Gardiner, T. A., & Stone, J. M. (2005). Energetics in MRI driven turbulence. In MAGNETIC FIELDS IN THE UNIVERSE: From Laboratory and Stars to Primordial Structures (pp. 475-488). (AIP Conference Proceedings; Vol. 784). https://doi.org/10.1063/1.2077209