首页> 外文期刊>Journal of geophysical research. Planets >Influence of Venus topography on the zonal wind and UV albedo at cloud top level: The role of stationary gravity waves
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Influence of Venus topography on the zonal wind and UV albedo at cloud top level: The role of stationary gravity waves

机译:金星地形对云顶层的纬向风和紫外线反照率的影响:静止重力波的作用

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Based on the analysis of UV images (at 365 nm) of Venus cloud top (altitude 67 ± 2 km) collected with 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 -83m/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 uplift 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. (Laboratoire de Météorologie Dynamique) In the equatorial regions, the UV albedo at 365nm 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 H_2O, showing that near the equator the lower UV albedo longitude region is correlated with increased H_2O. We argue that H_2O enhancement is the sign of upwelling, suggesting that the UV absorber is also brought to cloud top by upwelling.
机译:根据对金星快车(VEX)上的金星监控摄像机收集的金星云顶(海拔67±2 km)的紫外线图像(365 nm)的分析,发现赤道以南的纬向风速(来自5°S到15°S)显示金星的地理经度存在明显的变化(从-101到-83m / s),与阿芙罗狄蒂Terra的下伏相关。我们将这种模式解释为当水平风遇到山坡时,由于空气的抬升在地面产生的静止重力波的结果。这些波可以传播到云的最高层,在那里破裂,并将其动量传递到纬向流。 Lindzen(1981)已证明,重力波的这种向上传播和对风速垂直剖面的影响在地球的中层大气中起着重要作用,但在LMD的当前金星大气的GCM中并未重现。 (Laboratoire deMétéorologieDynamique)在赤道地区,365nm的紫外线反照率也随经度而变化。我们认为这种变化可以简单地用水平风场的发散来解释。在水平风速在幅度上增加(拉伸)的经度区域(从60°到-10°),它触发空气上升,使紫外线吸收剂达到云层的最高水平,反之则使风向降低,反之亦然。大小降低(压缩)。这幅图与金星子午环流的经典观点完全一致,赤道上的上升是由远离赤道的水平空气运动揭示的:经度效应只是对该效应的附加但重要的调制。最近的云顶H_2O映射使这种解释得到了安慰,该图表明在赤道附近较低的UV反照率经度区域与H_2O的增加相关。我们认为H_2O的增强是上升流的迹象,表明紫外线吸收剂也通过上升流而带到云顶。

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