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Observations and Analysis of the Mid-Latitude Atmospheric Electric Field During Geomagnetic Activity

机译:Observations and Analysis of the Mid-Latitude Atmospheric Electric Field During Geomagnetic Activity

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摘要

In this study, the diurnal and seasonal variation curves of atmospheric electric field are obtained, based on the extensive observations at Mohe station (Geographical coordinates: 22.357°E, 53.482°N and geomagnetic coordinates: 195.5°E, 48.8°N) of the Chinese Meridian Project. The results show that the diurnal variation of conforms to the “Carnegie” pattern, and the value of E_z in winter is higher than the summer. The coupling effect of the solar wind–magnetosphere with the atmospheric electric field is established. In total, 15 cases of magnetic storms are selected while Mohe is under fair weather condition throughout the storm period. The analyzed results reveal that E_z exhibits the same characteristics during the 15 storms, that is, E_z decreases sharply and changes simultaneously with the interplanetary magnetic field (IMF) component and solar wind proton number density. When the IMF–B_z shifts to south, E_z presents a large decrease with magnitudes of about 100 V/m–600 V/m.
机译:在这项研究中,昼夜和季节变化曲线的大气电场,基于大量的观察邻蒙古站(地理坐标:22.357°E,53.482°N和地磁坐标系:195.5°E,48.8°N)中国子午线的项目。结果表明,昼夜变化符合“卡耐基”模式和价值E_z在冬季高于夏季。太阳能wind-magnetosphere的耦合效应大气电场建立。风暴而选择邻蒙古是在公平的在风暴期间的天气条件。分析结果表明,E_z展品相同特征15风暴期间,是E_z急剧减少,变化同时与行星际磁场字段(IMF)组件和太阳风质子数密度。E_z呈现大量减少的大小约100 V / m - 600 V / m。

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