Direct kinetic Alfvén wave energy cascade in the presence of imbalance

T. Passot (1) , P.L. Sulem (1) , D. Laveder (1)

1 LAGRANGE - Joseph Louis LAGRANGE

A two-field Hamiltonian gyrofluid model for kinetic Alfvén waves retaining ion finite Larmor radius corrections and parallel magnetic field fluctuations is used to study direct turbulent cascades from the magnetohydrodynamic to the sub-ion scales. For moderate energy imbalance and weak enough magnetic fluctuations, the spectrum of the transverse magnetic field and that of the most energetic wave display a steep transition zone near the ion scale, while the parallel transfer (and thus the parallel dissipation) remains weak. In this regime, the perpendicular flux of generalized cross-helicity displays a significant decay past the ion scale, while the perpendicular energy flux remains almost constant. A phenomenological model suggests that the interactions between co-propagative waves present at the sub-ion scales can play a central role in the development of a transition zone in the presence of a helicity barrier.

Domains: Solar and Stellar Astrophysics [astro-ph.SR]; Plasmas

T. Passot, P.L. Sulem, D. Laveder. Direct kinetic Alfvén wave energy cascade in the presence of imbalance. Journal of Plasma Physics, 2022, 88 (3), pp.905880312. ⟨10.1017/S0022377822000472⟩. ⟨hal-03694468⟩