We use direct numerical simulations to compute turbulent transport
coefficients for passive scalars in turbulent rotating flows. Effective
diffusion coefficients in the directions parallel and perpendicular to the
rotations axis are obtained by studying the diffusion of an imposed initial
profile for the passive scalar, and calculated by measuring the scalar average
concentration and average spatial flux as a function of time. The Rossby and
Schmidt numbers are varied to quantify their effect on the effective diffusion.
It is find that rotation reduces scalar diffusivity in the perpendicular
direction. The perpendicular diffusion can be estimated from mixing length
arguments using the characteristic velocities and lengths perpendicular to the
rotation axis. Deviations are observed for small Schmidt numbers, for which
turbulent transport decreases and molecular diffusion becomes more significant.Comment: 10 pages, 13 figures. Slightly modified version to address referees'
comment