This paper proposes temporal scaling laws of the density-weighted energy spectrum for compressible turbulence in terms of dissipation rate, frequency and the Mach number. The study adopts the incomplete similarity theory in the scaling analysis of compressible turbulence motion. The investigation shows that the temporal Eulerian and Lagrangian energy spectra approach the -5/3 and -2 power laws when the Mach number M tends to reach unity and infinity, respectively.
机构:
Department of Mechanical Engineering,Cape Peninsula University of TechnologyDepartment of Mechanical Engineering,Cape Peninsula University of Technology
机构:
Univ Calif San Diego, Dept Phys, Ctr Astrophys & Space Sci, 9500 Gilman Dr, La Jolla, CA 92093 USA
St Petersburg State Univ, Sobolev Astron Inst, St Petersburg, RussiaUniv Calif San Diego, Dept Phys, Ctr Astrophys & Space Sci, 9500 Gilman Dr, La Jolla, CA 92093 USA
Kritsuk, Alexel G.
Padoan, Paolo
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Univ Calif San Diego, Dept Phys, Ctr Astrophys & Space Sci, 9500 Gilman Dr, La Jolla, CA 92093 USAUniv Calif San Diego, Dept Phys, Ctr Astrophys & Space Sci, 9500 Gilman Dr, La Jolla, CA 92093 USA
Padoan, Paolo
Wagner, Rick
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Univ Calif San Diego, Dept Phys, Ctr Astrophys & Space Sci, 9500 Gilman Dr, La Jolla, CA 92093 USAUniv Calif San Diego, Dept Phys, Ctr Astrophys & Space Sci, 9500 Gilman Dr, La Jolla, CA 92093 USA
Wagner, Rick
Norman, Michael L.
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Univ Calif San Diego, Dept Phys, Ctr Astrophys & Space Sci, 9500 Gilman Dr, La Jolla, CA 92093 USAUniv Calif San Diego, Dept Phys, Ctr Astrophys & Space Sci, 9500 Gilman Dr, La Jolla, CA 92093 USA
Norman, Michael L.
TURBULENCE AND NONLINEAR PROCESSES IN ASTROPHYSICAL PLASMAS,
2007,
932
: 393
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