Orbital stability of ensembles of particles in regions of magnetic reconnection in Earth's magneto-tail
Author:
Affiliation:
1. Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6, A-8042 Graz, Austria
2. Institute of Astrophysics, University of Vienna, Türkenschanzstrasse 17, A-1180 Wien, Austria
Funder
Austrian Science Fund
Publisher
AIP Publishing
Subject
Condensed Matter Physics
Link
http://aip.scitation.org/doi/pdf/10.1063/1.5093392
Reference39 articles.
1. Particle Interactions with Single or Multiple 3D Solar Reconnecting Current Sheets
2. Lyapunov Characteristic Exponents for smooth dynamical systems and for hamiltonian systems; a method for computing all of them. Part 1: Theory
3. Electron distribution functions in the electron diffusion region of magnetic reconnection: Physics behind the fine structures
4. Catalog of fine-structured electron velocity distribution functions – Part 1: Antiparallel magnetic-field reconnection (Geospace Environmental Modeling case)
5. Regular and chaotic charged particle motion in magnetotaillike field reversals: 1. Basic theory of trapped motion
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