Gravity wave momentum fluxes of 10-30 m² s⁻² and drag of 0.003-0.03 m s⁻² were estimated from Akatsuki radio occultation temperature data across 40-95 km altitudes on Venus.
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M-GITM simulations show gravity waves are critical for aphelion thermospheric polar warming but the model underestimates the observed polar-to-low-latitude temperature difference.
citing papers explorer
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Variation of Venusian Gravity Wave Absolute Momentum Fluxes and Drag as Retrieved from the Akatsuki Mission
Gravity wave momentum fluxes of 10-30 m² s⁻² and drag of 0.003-0.03 m s⁻² were estimated from Akatsuki radio occultation temperature data across 40-95 km altitudes on Venus.
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Mars Thermospheric Polar Warming at Aphelion: Dynamical Processes Studied Using M-GITM
M-GITM simulations show gravity waves are critical for aphelion thermospheric polar warming but the model underestimates the observed polar-to-low-latitude temperature difference.