Theoretical study of the high-latitude ionosphere's response to multicell convection patterns

Physics

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Convective Flow, F Region, Ionospheric Ion Density, Space Plasmas, Electron Precipitation, Interplanetary Magnetic Fields, Magnetohydrodynamic Flow, Oxygen Ions, Polar Caps, Three Dimensional Models

Scientific paper

A time-dependent three-dimensional model of the high-latitude ionosphere is used to study the characteristic ionospheric signatures associated with two-, three-, and four-cell plasma convection patterns. It is found that, for two-cell convection, the antisunward flow of plasma from the dayside into the polar cap acts to maintain the densities in this region in winter. For four-cell convection, the two additional convection cells in the polar cap are in darkness most of the time, and the resulting O(+) decay acts to produce twin polar holes that are separated by a sun-aligned ridge of enhanced ionization due to theta-auroral precipitation. For three-cell convection, only one polar hole forms in the total electron density, and an additional O(+) depletion region develops near noon. In this region there are strong electric fields, high ion temperatures, and an enhanced rate of O(+) - NO(+) conversion.

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