Transition to kinetic turbulence at proton scales driven by large-amplitude Kinetic Alfv\`en fluctuations

TL;DR

This study uses hybrid Vlasov-Maxwell simulations to explore how large-amplitude kinetic Alfvén waves in inhomogeneous space plasmas lead to proton distribution distortions and turbulence at proton scales.

Contribution

It demonstrates the transition from linear to turbulent regimes driven by KAW fluctuations in inhomogeneous magnetic backgrounds using detailed numerical simulations.

Findings

Proton distribution functions develop significant non-Maxwellian features.

KAW fluctuations induce a transition to turbulence at proton scales.

Magnetic shear influences the kinetic dynamics and turbulence development.

Abstract

Space plasmas are dominated by the presence of large-amplitude waves, large-scale inhomogeneities, kinetic effects and turbulence. Beside the homogeneous turbulence, generation of small scale fluctuations can take place also in other realistic configurations, namely, when perturbations superpose to an inhomogeneous background magnetic field. When an Alfv\'en wave propagates in a medium where the Alfv\'en speed varies in a direction transverse to the mean field, it undergoes phase-mixing, which progressively bends wavefronts, generating small scales in the transverse direction. As soon as transverse scales get of the order of the proton inertial length $d_p$, kinetic Alfv\'en waves (KAWs) are naturally generated. KAWs belong to the branch of Alfv\'en waves and propagate nearly perpendicular to the ambient magnetic field, at scales close to $d_p$. Many numerical, observational and theoretical works have suggested that these fluctuations may play a determinant role in the development of the solar-wind turbulent cascade. In the present paper, the generation of large amplitude KAW fluctuations in inhomogeneous background and their effect on the protons have been investigated by means of hybrid Vlasov-Maxwell direct numerical simulations. Imposing a pressure balanced magnetic shear, the kinetic dynamics of protons has been investigated by varying both the magnetic configuration and the amplitude of the initial perturbations. Of interest here is the transition from quasi-linear to turbulent regimes, focusing, in particular, on the development of important non-Maxwellian features in the proton distribution function driven by KAW fluctuations.