论文标题

火星尘埃风暴和重力波:将水传输到高层

Martian Dust Storms and Gravity Waves: Disentangling Water Transport to the Upper Atmosphere

论文作者

Shaposhnikov, Dmitry S., Medvedev, Alexander S., Rodin, Alexander V., Yiğit, Erdal, Hartogh, Paul

论文摘要

Max Planck Institute Martian通用循环模型的模拟28年和34年揭示了水“泵”机制的细节以及重力波(GW)强迫的作用。水的向上循环的向上分支向上大气中:在春分期间,在低纬度中,在溶解度期间在南极。分子扩散在中间气氛中和跨间隙中的水运输中起很少作用。 GWS调节全球尘埃飞机期间的循环和温度,从而改变了运输的时间和强度。在春分处,它们有助于在中间大气中的极性变暖区域中积聚水,然后在赤道上方上升。随着e骨暴风雨的衰变,GWS倾向于加速热层中水的减少。 GWS延迟了在解决方案风暴期间运输的发作,并将上层大气中的全球平均水降低10-25%。

Simulations with the Max Planck Institute Martian general circulation model for Martian years 28 and 34 reveal details of the water "pump" mechanism and the role of gravity wave (GW) forcing. Water is advected to the upper atmosphere mainly by upward branches of the meridional circulation: in low latitudes during equinoxes and over the south pole during solstices. Molecular diffusion plays little role in water transport in the middle atmosphere and across the mesopause. GWs modulate the circulation and temperature during global dust storms, thus changing the timing and intensity of the transport. At equinoxes, they facilitate water accumulation in the polar warming regions in the middle atmosphere followed by stronger upwelling over the equator. As equinoctial storms decay, GWs tend to accelerate the reduction of water in the thermosphere. GWs delay the onset of the transport during solstitial storms and change the globally averaged amount of water in the upper atmosphere by 10-25%.

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