On the convective instability of the cometary ionosphere

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Brunt-Vaisala Frequency, Cometary Atmospheres, Convection, Halley'S Comet, Ionospheres, Magnetohydrodynamic Stability, Ionopause, Lorentz Force, Magnetic Field Configurations, Temperature Gradients, Comets, Ionosphere, Convection, Stability, Plasma, Motion, Ionopause, Distribution, Production Rate, Analysis, Calculations, Perturbation, Halley, Techniques, Parameters, Centrifugal Force, Momentum, Density, Velocity, Wavelength

Scientific paper

The stability analysis of a cometary ionosphere by Ershkovich et al. (1989) is extended to include the effects of plasma motion. In the local inertial frame of reference moving with the plasma we arrived at the same instability criterion, but the Brunt-Vaisala frequency which governs the convective instability now involves the centrifugal force which has a destabilizing effect. As a result, the unstable layer becomes broader, expanding to greater distances from the ionopause. An increase of the comet production rate is shown to stabilize the ionosphere whereas an increase of the ion-neutral momentum exchange rate has a destabilizing effect. The cometary ionopause is shown to undergo the convective instability. The apparent stability of the Halley ionopause is due to the fact that perturbations are convected well downstream with the plasma bulk velocity before growing substantially. Thus we arrive at the conclusion that the cometary ionopause cannot be at rest.

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