Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-29T15:28:26.470Z Has data issue: false hasContentIssue false

Particle Acceleration in Collisionless Magnetic Reconnection

Published online by Cambridge University Press:  13 May 2016

P. K. Browning
Affiliation:
Dept of Physics, UMIST, PO Box 88, Manchester M60 1QD, UK
G. E. Vekstein
Affiliation:
Dept of Physics, UMIST, PO Box 88, Manchester M60 1QD, UK

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We investigate the acceleration of charged particles in the framework of collisionless reconnection. A steady reconnection scenario is considered, with a two dimensional X-point magnetic field geometry having also a uniform field component transverse to the plane of the X-point field, and an inductive electric field generating an inflow of particles. Test particle trajectories are studied, and the energy spectra of the accelerated particles are determined.

Type
Session VI: The Solar Wind and Heliosphere
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Vekstein, G.E. and Priest, E.R. 1995, Phys Plas 2, 3169.Google Scholar
Vekstein, G.E. and Browning, P.K. 1997, Phys Plas 4, 2261.CrossRefGoogle Scholar
Bruhwiler, D.L. and Zweibel, E.G. 1992, J. Geophys. Res. A97, 10825.CrossRefGoogle Scholar
Browning, P.K. and Vekstein, G.E. submitted to J. Geophys. Res.Google Scholar