WE PROPOSE TO ASSESS THE MORPHOLOGY AND EVOLUTION OF HOT ION INJECTION EVENTS INTO SATURN S INNER MAGNETOSPHERE. IN PARTICULAR WE WILL EXAMINE THE ENERGY-DEPENDENT AZIMUTHAL DRIFT OF HOT (>1 KEV) IONS AFTER THEY HAVE RAPIDLY MOVED RADIALLY INWARD DURING RAYLEIGH-TAYLOR LIKE INSTABILITIES COMMONLY CALLED
$469,499FY2021National Aeronautics and Space AdministrationNASA
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