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| | The Interaction of the Solar Wind With Venus |
 | | However, the solar wind does not directly interact with the atmosphere and current rates of loss to the solar wind are thought to play a minor role in the evolution of the terrestrial atmosphere. |
 | | At higher solar wind pressures, the ionopause moves to low altitudes, the current layer thickens, and a more direct interaction seems to occur in which currents are driven in the ionosphere by the solar wind electric field, i.e., by unipolar induction. |
 | | Region 1 is the wake, 2 the rarefaction region, 3 the magnetosheath, 4 the foreshock, and 5 the undisturbed solar wind. |
| www-ssc.igpp.ucla.edu /personnel/russell/papers/interact_solwind (18676 words) |
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