AbstractCurrent knowledge of solar tides in the middle and upper atmospheres of Mars and Venus is summarized, including Sun-synchronous tides on both planets; nonmigrating tides on Mars due to radiative/topographic interactions near the surface; and acceleration/deceleration of the zonal mean flows on Mars and Venus due to tidal interactions.
Tides in the middle and upper atmospheres of Mars and Venus
Advances in Space Research ; 33 , 2 ; 125-131
2003-05-23
7 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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