ON THE LAGRANGIAN NATURE OF THE TURBULENCE ENERGY CASCADE

The spatial and temporal evolution of turbulence kinetic energy at dif ferent scales is studied using direct numerical simulations of isotrop ic turbulence. To explicitly follow the energy during the cascade proc ess in physical space, a Lagrangian correlation coefficient between lo cal kinetic energy at different scales is computed. This correlation i s found to peak only after a Lagrangian time delay that is an increasi ng function of the scale separation. It is shown that a characteristic length reduction of a factor of 2 is achieved approximately after the local eddy-turnover time scale. The results show that the view of spa tially localized eddy structures transferring their kinetic energy to smaller scales appears to be, on average, quite realistic.