
Turbulence and laminar structures: can they co‐exist?
Author(s) -
Canuto V. M.
Publication year - 2000
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.2000.03786.x
Subject(s) - physics , turbulence , laminar flow , schwarzschild radius , reynolds number , classical mechanics , statistical physics , theoretical physics , astrophysics , mechanics , gravitation
Schwarzschild first suggested that the laminar structures observed in the high Reynolds number Re UL ν ≈O (10 12 ) solar photosphere are the result of turbulence rather than a proof of its absence. He reasoned that, since turbulence generates large turbulent viscosities ν t ≫ ν , the ‘effective’ Reynolds number Re UL ν t ≈O(1). Schwarzschild's argument is, however, incomplete, for it assumes that the entire role of the non‐linear interactions is to ‘enhance’ viscosity. While this is not true in general, we present a proof of how and why it may occur, thus completing Schwarzschild's argument. We further discuss the fact that the same non‐local turbulence models reproduce Large Eddy Simulation (LES) data for a variety of flows pertaining to astrophysics, geophysics and laboratory situations (in a fraction of the time).