Spatial irregularities in Jupiter's upper ionosphere observed by Voyager radio occultations

Physics

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Ionospheric Electron Density, Jupiter Atmosphere, Planetary Ionospheres, Radio Occultation, Spatial Distribution, Voyager 1 Spacecraft, Angular Distribution, Anisotropic Media, Density Distribution, Least Squares Method, Planetary Magnetic Fields, Radio Transmission, Voyager 2 Spacecraft, Jupiter, Ionosphere, Observations, Voyager, Occultations, Experiments, Voyager 1, Voyager 2, Radio Waves, Spectra, Amplitude, Phases, Data, Wavelengths, Scattering, Parameters, Analysis, Electrons, Density, Altitude, Latit

Scientific paper

Radio scintillations (at 3.6 and 13 cm) produced by scattering from ionospheric irregularities during the Voyager occultations are interpreted using a weak-scattering theory. Least squares solutions for ionospheric parameters derived from the observed fluctuation spectra yield estimates of (1) the axial ratio, (2) angular orientation of the anisotropic irregularities, (3) the power law exponent of the spatial spectrum of irregularities, and (4) the magnitude of the spatial variations in electron density. It is shown that the measured angular orientation of the anisotropic irregularities indicates magnetic field direction and may provide a basis for refining Jovian magnetic field models.

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