Anomalous scaling of passive scalars in rotating flows

Abstract

We present results of direct numerical simulations of passive scalar advection and diffusion in turbulent rotating flows. Scaling laws and the development of anisotropy are studied in spectral space, and in real space using an axisymmetric decomposition of velocity and passive scalar structure functions. The passive scalar is more anisotropic than the velocity field, and its power spectrum follows a spectral law consistent with $\sim k_{\perp }^{-3/2}$. This scaling is explained with phenomenological arguments that consider the effect of rotation. Intermittency is characterized using scaling exponents and probability density functions of velocity and passive scalar increments. In the presence of rotation, intermittency in the velocity field decreases more noticeably than in the passive scalar. The scaling exponents show good agreement with Kraichnan's prediction for passive scalar intermittency in two-dimensions, after correcting for the observed scaling of the second order exponent.

10 pages, 15 figures

References in corpus (3)

• Helicity cascades in rotating turbulence
• Scaling and energy transfer in rotating turbulence
• On the decrease of intermittency in decaying rotating turbulence

Cited by in corpus (4)

• Anisotropy and non-universality in scaling laws of the large scale energy spectrum in rotating turbulence
• Intermittency in Hall-magnetohydrodynamics with a strong guide field
• Incommensurate magnetic order in rare earth and transition metal compounds with local moments
• Passive scalars: mixing, diffusion and intermittency in helical and non-helical rotating turbulence