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NASA NTRS · 19910063744

Neutral line chaos and phase space structure

Abstract

Phase space structure and chaos near a neutral line are studied with numerical surface-of-section (SOS) techniques and analytic methods. Results are presented for a linear neutral line model with zero crosstail electric field. It was found that particle motion can be divided into three regimes dependening on the value of the conserved canonical momentum, Py, and the conserved Hamiltonian, h. The phase space structure, using Poincare SOS plots, is highly sensitive to bn = Bn/B0 variations, but not to h variations. It is verified that the slow motion preserves the action, Jz, as evaluated by Sonnerup (1971), when the period of the fast motion is smaller than the time scale of the slow motion. Results show that the phase space structure and particle chaos depend sensitively upon Py and bn, but are independent of h.

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BibTeXRIS

Burkhart, Grant R., Speiser, Theodore W., Martin, Richard F., Jr., Dusenbery, Paul B.. 1991-08-01. Neutral line chaos and phase space structure. https://ntrs.nasa.gov/citations/19910063744

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