Frequency power spectra of global quantities in magnetoconvection
arXiv:2103.04834 · doi:10.3390/fluids6040163
Abstract
We present the results of direct numerical simulations of power spectral densities for kinetic energy, convective entropy and heat flux for unsteady Rayleigh-Bénard magnetoconvection in the frequency space. For larger values of frequency, the power spectral densities for all the global quantities vary with frequency as . The scaling exponent is independent of Rayleigh number, Chandrasekhar's number and thermal Prandtl number.
5 pages, 3 figures