Geophysical fluid flows are predominantly turbulent and often strongly affected by the Earth's rotation, as well as by stable density stratification. Using direct numerical simulations of forced Boussinesq equations, we study the influence of these effects on the motion of fluid particles. We perform a detailed study of Lagrangian statistics of acceleration, velocity, and related quantities, focusing on cases where the frequencies associated with rotation and stratification (RaS), f and N, respectively, are held at a fixed ratio N/f = 5. The simulations are performed in a periodic domain, at Reynolds number Re approximate to 4000, and Froude number Fr in the range 0.03 less than or similar to Fr less than or similar to 0.2 (with Rossby number Ro = 5Fr). As the intensity of RaS increases, a sharp transition is observed between a regime dominated by eddies to a regime dominated by waves, which corresponds to Fr less than or similar to 0.07. For the given runs, this transition to a wave-dominated regime can also be seemingly described by simply comparing the timescales 1/N and tau(eta), the latter being the Kolmogorov timescale based on the mean kinetic energy dissipation. Due to the known anisotropy induced by RaS, we consider separately the motion in the horizontal and vertical directions. In the regime N tau(eta) 1, they behave very differently, experiencing the direct influence of the imposed rotation and stratification. On the other hand, the Lagrangian velocity statistics exhibit visible anisotropy for all runs; nevertheless the degree of anisotropy becomes very strong in the regime N tau(eta) > 1. We observe that in the regime N tau(eta ) 1, with no clear diffusive behavior. In contrast, the displacements in the vertical direction are always reduced. This inhibition is extremely strong in the N tau(eta )> 1 regime, leading to a scenario where particles almost appear to be trapped in horizontal planes.
