Turbulence and laminar structures: Can they co-exist?

7Citations
Citations of this article
8Readers
Mendeley users who have this article in their library.

Abstract

Schwarzschild first suggested that the laminar structures observed in the high Reynolds number Re = UL/v ≈ O (1012) solar photosphere are the result of turbulence rather than a proof of its absence. He reasoned that, since turbulence generates large turbulent viscosities vt ≫ v, the 'effective' Reynolds number Re = UL/vt ≈ 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).

Author supplied keywords

Cite

CITATION STYLE

APA

Canuto, V. M. (2000). Turbulence and laminar structures: Can they co-exist? Monthly Notices of the Royal Astronomical Society, 317(4), 985–988. https://doi.org/10.1046/j.1365-8711.2000.03786.x

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free