Theory and observations of electromagnetic ion cyclotron waves in Saturn's inner magnetosphere

Physics

Scientific paper

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Electromagnetic Radiation, Ion Cyclotron Radiation, Planetary Magnetospheres, Plasma Waves, Satellite Observation, Saturn Atmosphere, Planetary Magnetic Fields, Voyager 1 Spacecraft, Saturn, Magnetosphere, Theoretical Studies, Electromagnetic Properties, Ions, Cyclotron Waves, Spacecraft Observations, Voyager 1 Mission, Magnetic Field, Excitation, Oxygen, Pickup, Spectra, Hypotheses, Thermal Properties, Anisotropy, Pioneer 11 Mission, Satellites, Dione, Tethys, Plasma Torus, Waves, Particles, Interaction, C

Scientific paper

High-resolution Voyager 1 magnetic field observations of Saturn's inner magnetosphere are examined for the presence of ULF waves. Quasi-circular left-hand polarized transverse oscillations are found in the near-equatorial region of 5-7 Rs with a wave period about 10 s and peak amplitude of about 2 nT. The wave is identified as the electromagnetic oxygen cyclotron mode occurring at a frequency just below the O(+) ion cyclotron frequency. A theoretical model of wave excitation based on gyroresonant coupling through a temperature anisotropy of O(+) pickup ions is developed which accounts for the principal features of the wave spectrum. It is hypothesized that wave-particle interactions provide a level of scattering commensurate with the weak pitch angle diffusion regime but nonetheless one that regulates and maintains a constant thermal anisotropy of ions along the magnetic field. Arguments are also presented that O(+) was the dominant thermal ion of the Dione-Tethys plasma torus at the time of the Pioneer 11 encounter the year previous to the Voyager 1 measurements.

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