Large scale effects on the decay of rotating helical and non-helical turbulence

Abstract

Decaying three-dimensional (3D) turbulence is studied via direct numerical simulations (DNS) for an isotropic non-rotating flow and for rotating flows with and without helicity. We analyze the cases of moderate Rossby number and large Reynolds number focusing on the behavior of the energy spectrum at large scales and studying its effect on the time evolution of the energy and integral scales for $E(k)\sim k^4$ initial conditions. In the non-rotating case we observe the classical energy decay rate $t^{-10/7}$ and a growth of the integral length proportional to $t^{2/7}$ in agreement with the prediction obtained assuming conservation of the Loitsyanski integral. In the presence of rotation we observe a decoupling in the decay of the modes perpendicular to the rotation axis from the remaining 3D modes. These slow modes show a behavior similar to that found in two-dimensional (2D) turbulence whereas the 3D modes decay as in the isotropic case. We phenomenologically explain the decay considering integral conserved quantities that depend on the large scale anisotropic spectrum. The decoupling of modes is also observed for a flow with a net amount of helicity. In this case, the 3D modes decay as an isotropic fluid with a constant, constrained integral length, and the 2D modes decay as a constrained rotating fluid with maximum helicity.

20 pages, 16 figures

References in corpus (5)

• Scale interactions and scaling laws in rotating flows at moderate Rossby numbers and large Reynolds numbers
• Helicity cascades in rotating turbulence
• Scaling and energy transfer in rotating turbulence
• Structure and decay of rotating homogeneous turbulence
• On the decrease of intermittency in decaying rotating turbulence

Cited by in corpus (5)

• Generation of gravitational waves from freely decaying turbulence
• The decay of turbulence in rotating flows
• Large scale behavior and statistical equilibria in rotating flows
• Thermalized Abrikosov lattices from decaying turbulence in rotating BECs
• The decay of Batchelor and Saffman rotating turbulence