Fletcher, L. and Petkaki, P. (1997) Particle acceleration and transport in reconnecting plasmas. Solar Physics, 172(1-2), pp. 267-270. (doi: 10.1023/A:1004992228306)
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Abstract
We model the behaviour of particles in and around X-type magnetic configurations, a possible solar flare reconnection geometry. Particles are accelerated by a time-varying electric field close to the neutral point, and followed by integrating the equations of motion. When their motion becomes adiabatic a stochastic simulation is used to model their further transport in a collisional magnetised medium.
Item Type: | Articles |
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Status: | Published |
Refereed: | Yes |
Glasgow Author(s) Enlighten ID: | Fletcher, Professor Lyndsay |
Authors: | Fletcher, L., and Petkaki, P. |
Subjects: | Q Science > QB Astronomy Q Science > QC Physics |
College/School: | College of Science and Engineering > School of Physics and Astronomy |
Research Group: | Astronomy and Astrophysics |
Journal Name: | Solar Physics |
Publisher: | Springer Verlag |
ISSN: | 0038-0938 |
ISSN (Online): | 1573-093X |
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