Test particle energization of heavy ions in magnetohydrodynamic turbulence
arXiv:2112.09603 · doi:10.3847/1538-4357/ac5abe
Abstract
In the present work, we study the energization and displacement of heavy ions through the use of test particles interacting with the electromagnetic fields of magnetohydrodynamic (MHD) turbulence. These fields are obtained from pseudospectral direct numerical solutions (DNSs) of the compressible three-dimensional MHD equations with a strong background magnetic field. We find particle energization to be predominantly perpendicular as the ions become heavier (lower charge-to-mass ratio) and that high displacement is detrimental for perpendicular energization. On the other hand, perpendicular displacement is unaffected by the charge-to-mass ratio, which we explain with a simple guide center model. Using Voronoi tessellation along with this model, we analyze preferential concentration and find that particles behave as tracers in the perpendicular plane, clustering in regions with . These regions also have , which is optimal for perpendicular energization, thus providing a mechanism to understand precedent results.
References in corpus (7)
- Interstellar Pickup Ion Observations to 38 AU
- Weakly Turbulent MHD Waves in Compressible Low-Beta Plasmas
- Sources of Solar Energetic Particles
- Particle Acceleration and Fractional Transport in Turbulent Reconnection
- Preferential Heating and Acceleration of Heavy Ions in Impulsive Solar Flares
- Acceleration of Particles in Imbalanced Magnetohydrodynamic Turbulence
- Weak-strong clustering transition in renewing compressible flows