Beam-generated upper hybrid noise in Jupiter's outer magnetosphere

Physics

Scientific paper

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Boundary Layer Plasmas, Electromagnetic Noise, Electron Beams, Jupiter Atmosphere, Planetary Magnetospheres, Cyclotron Resonance, Field Aligned Currents, Heat Flux, Magnetic Equator, Jupiter, Magnetosphere, Waves, Origin, Formation, Theoretical Studies, Energetic Particles, Electrons, Magnetic Fields, Plasma Sheet, Diagrams, Kinematics, Stability, Electromagnetic Properties, Radiation, Emissions, Boundaries, Spacecraft Observations, Voyager 1 Mission, Injection, Heat, Flux, Diffusion

Scientific paper

A model for generation of upper hybrid waves in Jupiter's outer magnetosphere is presented. Energetic electrons accelerated on high-latitude auroral field lines at 1 R(J) altitudes are assumed to stream outwards to the distant magnetosphere. The large decrease in the local magnetic field strength results in a highly collimated, field-aligned electron beam due to conservation of the particle's magnetic moment. As the beam travels outward it passes through the plasma sheet boundary layer region located on the edges of the plasma sheet. Because of the large field-aligned anisotropy of the beam, the distribution is unstable to the excitation of the upper hybrid waves which amplify and then undergo mode conversion at the f(p) layer to generate the Jovian continuum radiation. A novel feature of the model is the beam-anisotropic heat flux instability which drives UH waves unstable without the need for any positive slope on the electron distribution function.

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