Particle acceleration in three-dimensional reconnection regions: A new test particle approach
- 1 November 1999
- journal article
- conference paper
- Published by AIP Publishing in Physics of Plasmas
- Vol. 6 (11) , 4318-4327
- https://doi.org/10.1063/1.873696
Abstract
Magnetic Reconnection is an efficient and fast acceleration mechanism by means of direct electric field acceleration parallel to the magnetic field. Thus, acceleration of particles in reconnection regions is a very important topic in plasma astrophysics. In this paper we show that the conventional analytical models and numerical test particle investigations can be misleading concerning the energy distribution of the accelerated particles, since they oversimplify the electric field structure by the assumption that the field is homogeneous. These investigations of the acceleration of charged test particles are extended by considering three-dimensional field configurations characterized by localized field-aligned electric fields. Moreover, effects of radiative losses are discussed. The comparison between homogeneous and inhomogeneous electric field acceleration in reconnection regions shows dramatic differences concerning both, the maximum particle energy and the form of the energy distribution.All Related Versions
This publication has 27 references indexed in Scilit:
- The magnetic structure ofB≠ 0-reconnectionPhysica Scripta, 1998
- Substorm ion injections: Geosynchronous observations and test particle orbits in three‐dimensional dynamic MHD fieldsJournal of Geophysical Research, 1997
- Particle Acceleration in Reconnecting Current Sheets with a Nonzero Magnetic FieldThe Astrophysical Journal, 1996
- Heating and acceleration atX-point reconnectionPhysica Scripta, 1996
- Nonlinear magnetic reconnection with collisionless dissipationPhysics of Plasmas, 1995
- Cross‐tail current, field‐aligned current, and ByJournal of Geophysical Research, 1994
- On the sources of interplanetary shocks at 0.72 AUJournal of Geophysical Research, 1994
- 3D resistive MHD computations of magnetospheric physicsComputer Physics Communications, 1990
- Particle acceleration by astrophysical shocksThe Astrophysical Journal, 1978
- Theoretical models of magnetic field line mergingReviews of Geophysics, 1975