The Venusian atmosphere is in a state of superrotation where prevailingwestward winds move much faster than the planet's rotation. Venus is coveredwith thick clouds that extend from about 45 to 70 km altitude, but thermalradiation emitted from the lower atmosphere and the surface on the planet'snightside escapes to space at narrow spectral windows of the near-infrared. Theradiation can be used to estimate winds by tracking the silhouettes of cloudsin the lower and middle cloud regions below about 57 km in altitude. Estimatesof wind speeds have ranged from 50 to 70 m/s at low to mid-latitudes, eithernearly constant across latitudes or with winds peaking at mid-latitudes. Herewe report the detection of winds at low latitude exceeding 80 m/s using IR2camera images from the Akatsuki orbiter taken during July and August 2016. Theangular speed around the planetary rotation axis peaks near the equator, whichwe suggest is consistent with an equatorial jet, a feature that has not beenobserved previously in the Venusian atmosphere. The mechanism producing the jetremains unclear. Our observations reveal variability in the zonal flow in thelower and middle cloud region that may provide clues to the dynamics of Venus'satmospheric superrotation.
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机译:金星的大气层处于超旋转状态,盛行的西风的移动速度比行星的旋转快得多。金星上覆盖着厚约45至70 km的厚云层,但低层大气和行星夜间表面发出的热辐射逃逸到近红外狭窄光谱窗口处的空间。通过跟踪海拔低于约57公里的中低层云区的轮廓,辐射可用于估算风。在中低纬度地区,风速的估计范围为50至70 m / s,在整个纬度范围内几乎恒定,或者在中纬度地区风速达到峰值。在此,我们报告了使用2016年7月至2016年8月期间从赤月轨道飞行器拍摄的IR2摄像机图像检测到的低纬度风超过80 m / s的情况。行星旋转轴的角速度在赤道附近达到峰值,这与赤道射流相一致。金星大气中以前没有观察到的功能。产生喷射的机制尚不清楚。我们的观察结果揭示了下部和中部云区域纬向流的变化,这可能为金星大气超旋转的动力学提供线索。
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