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Energy cascade and scaling in supersonic isothermal turbulence

Published online by Cambridge University Press:  22 July 2013

Alexei G. Kritsuk*
Affiliation:
Department of Physics and Center for Astrophysics and Space Sciences, University of California, San Diego, MC 0424, 9500 Gilman Drive, La Jolla, CA 92093-0424, USA
Rick Wagner
Affiliation:
San Diego Supercomputer Center, University of California, San Diego, MC 0505, 10100 Hopkins Drive, La Jolla, CA 92093-0505, USA
Michael L. Norman
Affiliation:
Department of Physics and Center for Astrophysics and Space Sciences, University of California, San Diego, MC 0424, 9500 Gilman Drive, La Jolla, CA 92093-0424, USA San Diego Supercomputer Center, University of California, San Diego, MC 0505, 10100 Hopkins Drive, La Jolla, CA 92093-0505, USA
*
Email address for correspondence: akritsuk@ucsd.edu

Abstract

Supersonic turbulence plays an important role in a number of extreme astrophysical and terrestrial environments, yet its understanding remains rudimentary. We use data from a three-dimensional simulation of supersonic isothermal turbulence to reconstruct an exact fourth-order relation derived analytically from the Navier–Stokes equations (Galtier & Banerjee, Phys. Rev. Lett., vol. 107, 2011, p. 134501). Our analysis supports a Kolmogorov-like inertial energy cascade in supersonic turbulence previously discussed on a phenomenological level. We show that two compressible analogues of the four-fifths law exist describing fifth- and fourth-order correlations, but only the fourth-order relation remains ‘universal’ in a wide range of Mach numbers from incompressible to highly compressible regimes. A new approximate relation valid in the strongly supersonic regime is derived and verified. We also briefly discuss the origin of bottleneck bumps in simulations of compressible turbulence.

Type
Rapids
Copyright
©2013 Cambridge University Press 

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