Multiscale Nature of the Dissipation Range in Gyrokinetic Simulations of Alfvenic Turbulence

Nonlinear energy transfer and dissipation in Alfven wave turbulence are analyzed in the first gyrokinetic simulation spanning all scales from the tail of the MHD range to the electron gyroradius scale. For typical solar wind parameters at 1 AU, about 30% of the nonlinear energy transfer close to the electron gyroradius scale is mediated by modes in the tail of the MHD cascade. Collisional dissipation occurs across the entire kinetic range k(perpendicular to)rho(i) greater than or similar to 1. Both mechanisms thus act on multiple coupled scales, which have to be retained for a comprehensive picture of the dissipation range in Alfvenic turbulence.