The magnetosphere of Neptune - Its response to daily rotation

Details The magnetosphere of Neptune - Its response to daily rotation The magnetosphere of Neptune - Its response to daily rotation

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990georl..17.1705v&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 17, Sept. 1990, p. 1705-1708.

Physics

12

Current Sheets, Neptune (Planet), Periodic Variations, Planetary Magnetospheres, Planetary Rotation, Free Energy, Magnetohydrodynamics, Magnetotails, Potential Energy, Thermodynamic Equilibrium, Three Dimensional Models, Two Dimensional Models

Scientific paper

The Neptunian magnetosphere periodically changes every eight hours between a pole-on magnetosphere with only one polar cusp and an earth-type magnetosphere with two polar cusps. In the pole-on configuration, the tail current sheet has an almost circular shape with plasma currents closing entirely within the magnetosphere. Eight hours later the tail current sheet assumes an almost flat shape with plasma currents touching the magnetotail boundary and closing over the tail magnetopause. Magnetic field and tail current sheet configurations have been calculated in a three-dimensional model, but the plasma- and thermodynamic conditions were investigated in a simplified two-dimensional MHD equilibrium magnetosphere. It was found that the free energy in the tail region of the two-dimensional model becomes independent of the dipole tilt angle. It is conjectured that the Neptunian magnetotail might assume quasi-static equilibrium states that make the free energy of the system independent of its daily rotation.

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