A Computational Model for Ion and Electron Energization during Macroscale Magnetic Reconnection
arXiv:2401.14500 · doi:10.1063/5.0199679
Abstract
A set of equations are developed that extend the macroscale magnetic reconnection simulation model kglobal to include particle ions. The extension from earlier versions of kglobal, which included only particle electrons, requires the inclusion of the inertia of particle ions in the fluid momentum equation, which was not required in the electron-only model. The new equations will facilitate the exploration of the simultaneous non-thermal energization of ions and electrons during magnetic reconnection in macroscale systems. Numerical tests of the propagation of Alfvén waves in a plasma with anisotropic electron and ion pressure are presented to benchmark the new model.
10 pages, 2 figures
References in corpus (11)
- Global Energetics of Thirty-Eight Large Solar Eruptive Events
- Two-scale structure of the electron dissipation region during collisionless magnetic reconnection
- Microwave and Hard X-Ray Observations of the 2017 September 10 Solar Limb Flare
- Electron Acceleration during Macroscale Magnetic Reconnection
- Kappa Distribution Model for Hard X-Ray Coronal Sources of Solar Flares
- Formation of Power-law Electron Energy Spectra in Three-dimensional Low- Magnetic Reconnection
- Stochastic Acceleration in Turbulent Electric Fields Generated by 3-D Reconnection
- A computational model for exploring particle acceleration during reconnection in macro-scale systems
- Hybrid Vlasov-MHD models: Hamiltonian vs. non-Hamiltonian
- Variability of the Reconnection Guide Field in Solar Flares
- Large-Scale Parallel Electric Fields and Return Currents in a Global Simulation Model
Cited by in corpus (4)
- Simultaneous Proton and Electron Energization during Macroscale Magnetic Reconnection
- Magnetic reconnection-driven energization of protons up to 400 keV at the near-Sun heliospheric current sheet
- The Maximum Particle Energy Gain During Magnetic Reconnection
- Probing Proton versus Electron Heating and Energization during Magnetic Reconnection