Physics
Scientific paper
Sep 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jgr....93.9584g&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 93, Sept. 1, 1988, p. 9584-9596. DOE-supported research.
Physics
48
Comets, Computerized Simulation, Ion Density (Concentration), Magnetohydrodynamic Stability, Ion Injection, Oxygen Ions, Particle Acceleration, Solar Protons, Solar Wind
Scientific paper
This paper presents a one-dimensional electromagnetic hybrid computer simulation of distant cometary environments, in which protons and oxygen ions are injected continuously at the same time. It is demonstrated that, when, instead of a single component, both protons and oxygen ions are injected, the faster growing shorter-wavelength proton-proton right-hand resonant instability dominates the early time physics, leading to linear temporal growth of the fluctuating magnetic field energy density and pitch angle scattering of the protons (but causing no significant response by the nonresonant oxygen ions). At later times, as the injected oxygen ions accumulate sufficient density, the oxygen-proton right-hand resonant instability emerges, exhibiting exponential temporal growth to a relatively large peak amplitude, phase bunching, and magnetically trapping the oxygen ions. At times after peak amplitude, the oxygen-proton fluctuations stochastically accelerate some of the injected protons.
Gary Peter S.
Madland Christian D.
Omidi Nojan
Winske Dan
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