On the compressibility effect in test particle acceleration by magnetohydrodynamic turbulence

TL;DR

This study investigates how compressibility influences test particle acceleration in MHD turbulence, revealing that compressibility enhances proton energization via perpendicular electric fields, while electrons remain largely unaffected unless electron pressure effects are included.

Contribution

The paper demonstrates the specific impact of compressibility on proton acceleration and highlights the importance of electron pressure in electron energization within turbulent MHD fields.

Findings

Compressibility increases proton acceleration efficiency.

Electrons show minimal effect from compressibility unless electron pressure is considered.

Electron pressure gradient significantly contributes to electron energization.

Abstract

The effect of compressibility in charged particle energization by magnetohydrodynamic (MHD) fields is studiedin the context of test particle simulations. This problem is relevant to the solar wind and the solar corona due to the compressible nature of the flow in those astrophysical scenarios. We consider turbulent electromagnetic fields obtained from direct numerical simulations of the MHD equations with a strong background magnetic field. In order to explore the flow compressibilty effect over the particle dynamics we performed different numerical experiments: an incompressible case, and two weak compressible cases with Mach number M = 0.1 and M = 0.25. We analyze the behavior of protons and electrons in those turbulent fields, which are well known to form aligned current sheets in the direction of the guide magnetic field. What we call protons and electrons are test particles with scales comparable to (for protons) and much smaller than (for electrons) the dissipative scale of MHD turbulence, maintaining the correct mass ratio me /mi. For these test particles we show that compressibility enhances the efficiency of proton acceleration, and that the energization is caused by perpendicular electric fields generated between currents sheets. On the other hand, electrons remain magnetized and display an almost adiabatic motion, with no effect of compressibility observed. Another set of numerical experiments takes into account two fluid modifications, namely electric field due to Hall effect and electron pressure gradient. We show that the electron pressure has an important contribution to electron acceleration allowing highly parallel energization. In contrast, no significant effect of these additional terms is observed for the protons.