Computer Science – Numerical Analysis
Scientific paper
Mar 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...254..376b&link_type=abstract
Astrophysical Journal, Part 1, vol. 254, Mar. 1, 1982, p. 376-390.
Computer Science
Numerical Analysis
16
Earth Magnetosphere, Electrostatic Waves, Jupiter Atmosphere, Plasma Resonance, Plasma Temperature, Wave Dispersion, Hydrogen Plasma, Line Spectra, Nonuniform Plasmas, Numerical Analysis, Plasma Composition
Scientific paper
Dispersion properties of electrostatic waves in a multi-ion plasma are examined, with an analysis that incorporates the effects of finite temperature, finite parallel wavenumber, and wave growth/damping in a systematic development of equations. Numerical solutions and analytic formulas are given for an ion plasma consisting of H(+), O(+), and S(+) for application to Jupiter's magnetosphere. It is demonstrated how observations of plasma resonance lines may be used as a diagnostic of ion composition in magnetospheric plasma. This potential use of high-sensitivity/high-resolution plasma wave instrumentation may provide information necessary to resolve issues concerning the origin of plasmas in the earth's neighborhood.
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