Energisation of charged particles by fast magnetic reconnection
by
Dhrubaditya Mitra
→
Europe/Stockholm
122:026
122:026
Description
We study the role of turbulence in magnetic reconnection, within the
framework of magneto-hydrodynamics, using three-dimensional direct
numerical simulations. For small turbulent intensity we find that the
reconnection rate obeys Sweet-Parker scal- ing. For large enough
turbulent intensity reconnection rate departs significantly from
Sweet-Parker behaviour, becomes almost a constant as a function of the
Lundquist number. We further study energisation of test-particles in
the same setup. We find that the speed of the energised particles
obeys a Maxwellian distribution, whose vari- ance also obeys
Sweet-Parker scaling for small turbulent intensity but depends weakly
on the Lundquist number for large turbulent intensity. Furthermore,
the variance is found to increase with the strength of the
reconnecting magnetic field.