Pharasi Hirdesh K, Kumar Krishna, Bhattacharjee Jayanta K
Department of Physics, Indian Institute of Technology, Kharagpur 721 302, India.
Harish-Chandra Research Institute, Allahabad 211 019, India.
Phys Rev E Stat Nonlin Soft Matter Phys. 2014 Oct;90(4):041004. doi: 10.1103/PhysRevE.90.041004. Epub 2014 Oct 31.
The frequency spectra of the entropy and kinetic energy along with the power spectrum of the thermal flux are computed from direct numerical simulations for turbulent Rayleigh-Bénard convection with uniform rotation about a vertical axis in low-Prandtl-number fluids (Pr<0.6). Simulations are done for convective Rossby numbers Ro≥0.2. The temporal fluctuations of these global quantities show two scaling regimes: (i) ω(-2) at higher frequencies for all values of Ro and (ii) ω(-γ1) at intermediate frequencies with γ1≈4 for Ro>1, while 4<γ1<6.6 for 0.2≤Ro<1.