Transport from chaotic orbits in the geomagnetic tail

Details Transport from chaotic orbits in the geomagnetic tail Transport from chaotic orbits in the geomagnetic tail

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991georl..18.1583h&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 18, Aug. 1991, p. 1583-1586.

Physics

11

Geomagnetic Tail, Space Plasmas, Transport Properties, Chaos, Cyclotron Radiation, Stochastic Processes, Trapped Particles

Scientific paper

The rapid change in direction and magnitude of the magnetic field vector in crossing the quasi-neutral sheet in the geomagnetic tail leads to deterministic Hamiltonian chaos. The finite correlation times in the single particle orbits due to the continuum of orbital frequencies leads to well-defined collisionless transport coefficients. The transport coefficients are derived for plasma trapped in the quasi-neutral sheet.

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