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Evidence for influence of the solar wind variations on atmospheric temperature in the southern polar region

机译:太阳风变化对南极地区大气温度影响的证据

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摘要

Detailed analysis of meteorological and aerological data from Vostok station (Antarctica) for 1978-1992 made it possible to conclude that dramatic changes of the troposphere temperature, observed in the southern polar region, are related to the variations of the interplanetary magnetic field (IMF). The warming is observed at ground level and cooling at h > 10 km if the IMF vertical component decreases (△B_Z < 0). The opposite deviation of the atmospheric temperatures (cooling at the ground level and warming at h > 10 km) is observed for △B_Z > 0. There is a linear relationship between the value of change in the interplanetary electric field (△E_(SW)) and ground temperature at Vostok station: the larger is the leap in the E_(SW) the stronger is the temperature deviation. The effect reaches maximum within 1 day and is damped equally quickly. The tropospheric pressure and horizontal winds respond to the E_(SW) fluctuations as well. It is suggested that the interplanetary electric field affects the katabatic system of atmospheric circulation typical of the ice dome in winter Antarctic.
机译:对1978-1992年南极Vostok站的气象和航空数据进行的详细分析,有可能得出结论,即在南极地区观测到的对流层温度的剧烈变化与行星际磁场(IMF)的变化有关。 。如果IMF垂直分量减小(△B_Z <0),则在地面观察到变暖,在h> 10 km观察到冷却。当△B_Z> 0时,观察到大气温度的相反偏差(在地平面降温和在h> 10 km处变暖)。行星际电场的变化值(△E_(SW)之间存在线性关系。 )和Vostok站的地面温度:E_(SW)的跃变越大,温度偏差就越大。效果在1天内达到最大,并且被同样迅速地衰减。对流层压力和水平风也对E_(SW)波动做出响应。建议行星际电场影响南极冬季典型的冰穹大气环流的合成系统。

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