Stability of the Io Plasma Torus/atmosphere Interaction
نویسندگان
چکیده
The stability of the Io plasma toms-atmosphere interaction is examined. A simple plasma deflection model describes how transients in the plasma flux and the content of the atmosphere affect the ionospheric conductance, limiting the plasma bombardment and, hence, the supply of atmospheric species to the toms. The supply of the toms is seen to be determined by the thermal structure of the plasma, namely, the amount of low energy plasma producing atmospheric erosion vs. that which produces ionization, so that the toms supply rate is not simply proportional to the torus ion density.
منابع مشابه
Electromagnetic interaction between Jupiter’s ionosphere and the Io Plasma torus
The electromagnetic interaction between Jupiter and Io has been studied extensively since the discovery of Io-controlled decametric radio emissions (DAMs). A variety of mechanisms for electromagnetic disturbances have been considered including a unipolar inductor, the excitation of large-amplitude Alfvén waves, the generation of electrostatic electric fields parallel to the ambient magnetic fie...
متن کاملPlasma Ion Heating of an SO<sub>2</sub> Atmosphere on Io
The Jovian plasma ion heating of any column, in the appendix a radial column. The atmospheric gas over Io is shown to be important temperature, T, is determined by the heat flow for determining the temperature structure and the described by the conductivity, K, location of the exobase and for limiting diffusive separation i Io's atmosphere. This is used (KdT/dz) -•i(z' )F(z' )dz' + (z)dz' (1) a...
متن کاملMonte Carlo Modeling of Io's [oi] Aurora in Eclipse
Introduction: Io generates an aurora with different features from Earth's aurora. For example, on Io the 630 nm [OI] aurora is concentrated around the equator whereas on Earth the aurora is mainly around the poles. Observations of Io just after entering Jupi-ter's shadow by Trauger et al. [1] and Retherford et al. [2] showed several bright regions of [OI] 630 nm emission. Several features of th...
متن کاملThe Structure of Io's Thermal Corona and Implications for Atmospheric Escape
We investigate the escape of species from Io's atmosphere using a steady-state model of Io's exospheric corona and its interaction with the Io plasma torus. The corona is assumed to be spherically symmetric with the radial density and compositional structure determined by the gas kinetic temperature, critical level radius, and mixing ratios of the component species. Thermal and nonthermal escap...
متن کاملSputtering of Sulfur by Kiloelectronvolt Ions: Application to the Magnetospheric Plasma Interaction with Io
Measurements of total yields, temperature dependences, mass spectra, and energy spectra of molecules sputtered from condensed sulfur (Ss) at low temperatures by keV ions are reported and results are given for Jovian plasma ion bombardment of !o. A change in the reflectance of the sulfur, which can be removed by annealing, is produced by the most penetrating ions and may be connected with the da...
متن کامل