Polarization of high latitude ionospheric turbulence as determined by analysis of data from the OVI-17 satellite

Physics

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Electric Fields, Ionospheric Propagation, Polar Regions, Polarization Characteristics, Satellite Observation, Turbulence Effects, Atmospheric Turbulence, Data Acquisition, Data Reduction, Magnetospheric Instability, Plasma Turbulence

Scientific paper

High-latitude low-frequency electric field data from the OVI-17 satellite have been extensively analyzed by Kelley and Mozer (1972). In the present paper, some of these data are further scrutinized in the light of new data provided by the S3-3 satellite. It is shown that, in contrast to the original analysis, high-latitude magnetospheric turbulence has an electric field component that is predominantly perpendicular to the magnetic field and that there is no inconsistency between magnetospheric and ionospheric data.

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