Magnetic Reconnection
Magnetic reconnection is a plasma process that dissipates the energy stored in magnetic field into plasma kinetic energy, through a rearrangement of magnetic field topology, resulting in particles heating and acceleration.
It is thought to play an important role in numerous astrophysical sources like gamma-ray bursts and jets from active galactic nuclei (AGN). Magnetic reconnection and shock acceleration are usually invoked among the possible mechanisms to produce particle non-thermal spectra.