Inference of the angular velocity of plasma in the Jovian magnetosphere from the sweepback of magnetic field

Physics

Scientific paper

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Angular Velocity, Jupiter Atmosphere, Planetary Magnetic Fields, Planetary Magnetospheres, Plasma Dynamics, Current Sheets, Lines Of Force, Voyager 1 Spacecraft, Voyager 2 Spacecraft, Jupiter, Magnetosphere, Plasma Sheet, Corotation, Plasma, Calculations, Magnetic Field, Particles, Torque, Techniques, Nightside, Distance, Flow, Spacecraft Observations, Voyager Missions, Comparisons, Velocity

Scientific paper

The averaged angular velocity of plasma from magnetic observations is evaluated using plasma outflow rate as a parameter. New techniques are developed to calculate the normal and azimuthal components of the magnetic field in and near to the plasma sheet in a plasma sheet coordinate system. The revised field components differ substantially from the quantities used in previous analyses. With the revised field values, it appears that during the Voyager 2 flyby for an outflow rate of 2.5 x 10 exp 29 amu/s, the observed magnetic torque may be sufficient to keep the plasma in corotation to radial distances of 50 Rj in the postmidnight quadrant.

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