Influence of Venus topography on the zonal wind and UV albedo at cloud top level: The role of stationary gravity waves.

Jean-Loup Bertaux (1) , Igor V. Khatunstsev (2) , Alain Hauchecorne (3) , Wojciech J. Markiewicz (4) , Emmanuel Marcq (1) , Sébastien Lebonnois (5) , Marina Patsaeva (2) , Alexander Turin (2) , Anna Fedorova (2)

1 PLANETO - LATMOS
2 IKI - Space Research Institute of the Russian Academy of Sciences
3 STRATO - LATMOS
4 MPS - Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research
5 LMD - Laboratoire de Météorologie Dynamique (UMR 8539)

Based on the analysis of UV images (at 365 nm) of Venus cloud top (altitude 67 ± 2 km) collected with VMC (Venus Monitoring Camera) on board Venus Express (VEX), it is found that the zonal wind speed south of the equator (from 5°S to 15°S) shows a conspicuous variation (from -101 to -83 m/s) with geographic longitude of Venus, correlated with the underlying relief of Aphrodite Terra. We interpret this pattern as the result of stationary gravity waves produced at ground level by the up lift of air when the horizontal wind encounters a mountain slope. These waves can propagate up to the cloud top level, break there and transfer their momentum to the zonal flow. Such upward propagation of gravity waves and influence on the wind speed vertical profile was shown to play an important role in the middle atmosphere of the Earth by Lindzen [1981], but is not reproduced in the current GCM of Venus atmosphere from LMD. In the equatorial regions, the UV albedo at 365 nm varies also with longitude. We argue that this variation may be simply explained by the divergence of the horizontal wind field. In the longitude region (from 60° to -10°) where the horizontal wind speed is increasing in magnitude (stretch), it triggers air upwelling which brings the UV absorber at cloud top level and decreases the albedo, and vice-versa when the wind is decreasing in magnitude (compression). This picture is fully consistent with the classical view of Venus meridional circulation, with upwelling at equator revealed by horizontal air motions away from equator: the longitude effect is only an additional but important modulation of this effect. This interpretation is comforted by a recent map of cloud top H2O [Fedorova et al., 2015], showing that near the equator the lower UV albedo longitude region is correlated with increased H2O. We argue that H2O enhancement is the sign of upwelling, suggesting that the UV absorber is also brought to cloud top by upwelling.

Mots clés: Venus; zonal wind; gravity waves; Venus Express; VMC; superrotation

Domaines: Planétologie et astrophysique de la terre [astro-ph.EP]; Océan, Atmosphère

Jean-Loup Bertaux, Igor V. Khatunstsev, Alain Hauchecorne, Wojciech J. Markiewicz, Emmanuel Marcq, et al.. Influence of Venus topography on the zonal wind and UV albedo at cloud top level: The role of stationary gravity waves.. Journal of Geophysical Research. Planets, 2016, 121 (6), pp.1087-1101. ⟨10.1002/2015JE004958⟩. ⟨insu-01328045⟩