Ballooning Instability in the Jovian Magnetosphere

Details Ballooning Instability in the Jovian Magnetosphere Ballooning Instability in the Jovian Magnetosphere

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..649..285d&link_type=abstract

DUSTY PLASMAS IN THE NEW MILLENNIUM: Third Conference on the Physics of Dusty Plasmas. AIP Conference Proceedings, Volume 649,

Physics

Dusty Or Complex Plasmas, Plasma Crystals, Macroinstabilities, Jupiter, Magnetohydrodynamic And Fluid Equation

Scientific paper

The ballooning instability arising due to the curvature of the magnetic field in the Jovian magnetosphere and co-rotational motion of plasma particles with the planet, is investigated in this problem. The MHD equation for the system of electrons, ions and dust grains appropriate to the situation are considered. The stability condition for the ballooning mode is derived using the energy principle. The effect of dust particles is studied in destabilizing the mode.

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