Turbulence in compressible flows

David Porter, Annick Pouquet, Igor Sytine, Paul Woodward

Research output: Contribution to journalArticlepeer-review

28 Scopus citations


Results stemming from a series of high-resolution three-dimensional computations using the PPM code [28] are reviewed, both for decaying and for driven supersonic turbulence at a r.m.s. Mach number of unity. A comparison with Navier-Stokes runs is provided for the first time in three dimensions. Scaling laws for two-point structure functions obtain, that are similar to the incompressible case, including new results for the energy transfer. Vortex sheets and filaments develop, as well as numerous shocks, with a strong density contrast.

Original languageEnglish (US)
Pages (from-to)263-270
Number of pages8
JournalPhysica A: Statistical Mechanics and its Applications
Issue number1-4
StatePublished - Jan 1 1999


  • Intermittency
  • Interstellar medium
  • Supersonic turbulence

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