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Tropospheres of Earth, Mars and Venus are, as a rule, stably stratified. At the same time, turbulence exists, creating constant composition of the atmospheres up to altitudes of 100-150 km. This turbulence is formed mainly via breaking of buoyancy waves (i.e. internal gravity waves), moving from the surface upwards in the atmosphere of a planet. Under such conditions, an anomalous downward turbulent...
We use the previous radio-occulation data and quasi-2D MHD model for the dayside of the planet to construct a global isodensity and plasma scale height distributions and large scale inhomogeneities in the Martian topside ionosphere. This semiempirical global electron density distribution is used for comparison of plasma scale heights and scale heights of the neutral atmosphere (Mars-GRAM - model)...
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