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- W4313360761 abstract "Abstract The ubiquitous turbulence in astrophysical plasmas is important for both magnetic reconnection and reconnection acceleration. We study the particle acceleration during fast 3D turbulent reconnection with reconnection-driven turbulence. Particles bounce back and forth between the reconnection-driven inflows due to the mirror reflection and convergence of strong magnetic fields. Via successive head-on collisions, the kinetic energy of the inflows is converted into accelerated particles. Turbulence not only regulates the inflow speed but also introduces various inflow obliquities with respect to the local turbulent magnetic fields. As both the energy gain and probability of the escape of particles depend on the inflow speed, the spectral index of particle energy spectrum is not universal. We find it in the range of ≈2.5–4, with the steepest spectrum expected at a strong guide field, i.e., a small angle between the total incoming magnetic field and the guide field. Without scattering diffusion needed for confining particles, the reconnection acceleration can be very efficient at a large inflow speed and a weak guide field." @default.
- W4313360761 created "2023-01-06" @default.
- W4313360761 creator A5028300061 @default.
- W4313360761 creator A5086116818 @default.
- W4313360761 date "2022-12-30" @default.
- W4313360761 modified "2023-10-18" @default.
- W4313360761 title "Turbulent Reconnection Acceleration" @default.
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- W4313360761 doi "https://doi.org/10.3847/1538-4357/aca32c" @default.
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