Ion Acceleration During Macroscale Magnetic Reconnection
ORAL
Abstract
The recently developed computational model kglobal, which combines an MHD backbone with self-consistent guiding-center particles has previously demonstrated self-consistent simulations of electron acceleration during magnetic reconnection in a macroscale system that produced power-law energy spectra extending over multiple decades in energy. Here we report on an expansion of kglobal that demonstrates simultaneous ion and electron acceleration and power-law production. The ion power laws also extend over multiple decades of energy and exhibit spectral indices similar to the electrons. A strong guide field weakens the Fermi drive mechanism and suppresses nonthermal particle production. For a weak guide field, the total energy content of nonthermals dominates even though their respective number densities remain small.
*This work has been supported by NSF Grant Nos. PHY1805829 and PHY1500460 and the NASA Drive Science Center on Solar Flare Energy Release (SolFER), grant 80NSSC20K0627. The simulations were carried out at the National Energy Research Scientific Computing Center (NERSC).
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Presenters
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Michael M Swisdak
- University of Maryland, College Park