North-south asymmetries in the thermosphere during the last maximum of the solar cycle

Physics

Scientific paper

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Annual Variations, Ionospheric Disturbances, Ionospheric Temperature, Latitude, Solar Cycles, Thermosphere, Atmospheric Density, Atmospheric Heat Budget, Atom Concentration, Ionospheric Composition, Northern Hemisphere, Southern Hemisphere, Wind (Meteorology)

Scientific paper

A large volume of data (temperatures, densities, concentrations, winds) has been accumulated showing that in addition to seasonal changes in the thermosphere, annual variations are present and have a component that is a function of latitude. It appears that the helium concentrations have much larger variations in the southern hemisphere than in the northern hemisphere; the same holds true for the exospheric temperatures deduced from Ogo 6 data. The bulge of density tends to stay over the southern hemisphere, whereas winds show a tendency to blow northward across the equator. More energy seems to be available for the thermosphere in the southern hemisphere during the equinoxes; this may be the result of an asymmetry in the geomagnetic field or an asymmetrical dissipation of tidal waves induced by an asymmetrical worldwide ozone distribution.

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