pith. sign in

arxiv: physics/0701201 · v2 · submitted 2007-01-18 · ⚛️ physics.flu-dyn · cond-mat.other

Signatures of two-dimensionalisation of 3D turbulence in presence of rotation

classification ⚛️ physics.flu-dyn cond-mat.other
keywords exponentrotationturbulencearguebeenenergyrapidlyrotating
0
0 comments X
read the original abstract

A reason has been given for the inverse energy cascade in the two-dimensionalised rapidly rotating 3D incompressible turbulence. For such system, literature shows a possibility of the exponent of wavenumber in the energy spectrum's relation to lie between -2 and -3. We argue the existence of a more strict range of -2 to -7/3 for the exponent in the case of rapidly rotating turbulence which is in accordance with the recent experiments. Also, a rigorous derivation for the two point third order structure function has been provided helping one to argue that even with slow rotation one gets, though dominated, a spectrum with the exponent -2.87, thereby hinting at the initiation of the two-dimensionalisation effect with rotation.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Spatio-Temporal Signatures of Intermittency in Helically Rotating Turbulence through Topological Data Analysis

    physics.flu-dyn 2026-05 unverdicted novelty 6.0

    TDA on vorticity magnitude and length-scale fields in helically rotating turbulence produces Wasserstein-distance heatmaps that flag spatiotemporal signatures of strong turbulent fluctuations more sensitively than con...