Abstract
A model of the Earth's ionosphere and plasmasphere is used to investigate the effects of an imposed westward plasma drift of maximum velocity 2kms −1. A closed subauroral tube of plasma is considered and the velocity spike persists for 10 min. Ion-neutral frictional heating causes rapid elevation of the F-region O + temperature. The F-layer O + concentration is decreased due to increased O + loss rate and rapid ion flows both upward and downward from the F-region. The upward flux of O + through the topside ionosphere can reach 5 × 10 9cm −2s −1; when the velocity spike ceases there is a return flow of O + that tends to replenish the F-layer. Most of the features revealed by the model for the F-region and topside ionosphere are in accord with observations of subauroral ion drifts. Downward flows that are predicted to be persistently present around the 300 km altitude level appear to agree with observations only occasionally; suggestions are made to resolve this discrepancy.
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