Numerical Measurements of the Spectrum in Strong Magnetohydrodynamic Turbulence

ORAL

Abstract

We discuss the results of an extensive set of direct numerical simulations of forced, incompressible, strong MHD turbulence with a strong guide field. Our aim is to resolve the controversy regarding the power law exponent of the field perpendicular energy spectrum. The two main theoretical predictions, -3/2 and -5/3, have both received some support from numerical simulations carried out by different groups, however, the design of those calculations also differ. Our simulations have a resolution of $512^3$ mesh points, a strong guide field, an anisotropic simulation domain, and implement a broad range of large-scale forcing routines. Our findings indicate that the spectrum of well developed, strong incompressible MHD turbulence with a strong guide field has the exponent -3/2.

Authors

  • J. Mason

    University of Chicago

  • F. Cattaneo

    University of Chicago/ Argonne National Laboratory, University of Chicago, University of Chicago / Argonne National Laboratory

  • Stanislav Boldyrev

    Department of Physics, University of Wisconsin-Madison, University of Wisconsin, University of Wisconsin-Madison, University of Wisconsin, Madison, UW-Madison