The Huygens probe recorded atmospheric temperatures during its parachute descent through the atmosphere of Titan. A careful analysis of these data reveals for the first time spectacular but hitherto-unreported small-scale variations in stratospheric temperatures that we interpret as gravity waves, consistent with detection of such waves at higher altitudes by other means. The structures have a vertical wavelength of 3-8. km and a peak-peak amplitude of ~2. K that is roughly constant over altitudes from ~140. km, where measurements began, to ~60. km. This altitude, below which no significant temperature waves are seen, coincides with a local maximum in the zonal wind profile, and is close to where the Brunt-Väisälä frequency is highest. It seems possible that the zonal wind field influences the vertical gravity wave propagation. © 2013 Elsevier Inc.
Gravity waves in Titan's lower stratosphere from Huygens probe in situ temperature measurements
Ferri F.
2014
Abstract
The Huygens probe recorded atmospheric temperatures during its parachute descent through the atmosphere of Titan. A careful analysis of these data reveals for the first time spectacular but hitherto-unreported small-scale variations in stratospheric temperatures that we interpret as gravity waves, consistent with detection of such waves at higher altitudes by other means. The structures have a vertical wavelength of 3-8. km and a peak-peak amplitude of ~2. K that is roughly constant over altitudes from ~140. km, where measurements began, to ~60. km. This altitude, below which no significant temperature waves are seen, coincides with a local maximum in the zonal wind profile, and is close to where the Brunt-Väisälä frequency is highest. It seems possible that the zonal wind field influences the vertical gravity wave propagation. © 2013 Elsevier Inc.
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