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2011年5月26日北京上空TeSL与Es、大气风场的同时观测
引用本文:荀宇畅,杨国韬,王继红,杜丽芳,焦菁,王泽龙,程学武,王赤. 2011年5月26日北京上空TeSL与Es、大气风场的同时观测[J]. 地球物理学报, 2017, 60(11): 4390-4397. DOI: 10.6038/cjg20171126
作者姓名:荀宇畅  杨国韬  王继红  杜丽芳  焦菁  王泽龙  程学武  王赤
作者单位:1. 中国科学院国家空间科学中心空间天气学国家重点实验室, 北京 100190;2. 中国科学院武汉物理与数学研究所波谱与原子分子物理国家重点实验室, 武汉 430071;3. 中国科学院大学地球科学学院, 北京 100049
基金项目:国家自然科学基金(41474130,41264006,41627804),国家自然科学基金青年科学基金项目(41604130),国家国际科技合作专项(2014DFA20770),中国科学院国家空间科学中心重点培育项目,中国科学院空间科学中心空间天气学国家重点实验室专项资助.
摘    要:本文报道了北京延庆(116.0°E,40.5°N)钠荧光激光雷达在2011年5月26日夜间观测到的一例低热层钠层(lower thermospheric-enhanced sodium layer,TeSL)事例,从数据采集开始到观测结束,该低热层钠层持续存在且不断增强,峰值密度从250 cm-3增加至1500 cm-3,峰值高度却从111 km逐渐下降到100 km.同一时间相距28 km的测高仪也观测到了出现在106~117 km的Es层,平均强度4.5 MHz;对流星雷达设备观测到的75~100 km的纬向风风速进行拟合,得到100~125 km的风速,风剪切节点从122 km下降到108 km.Es层和纬向风剪切节点的演化趋势与TeSL事件呈现出极好的相关性.我们计算了离子垂直速度及辐射复合反应的生成率,对钠原子的出现高度和密度做出解释,推测风剪切汇聚的Na+与Es层中的电子中和,是形成当日TeSL的主要机制.

关 键 词:激光雷达  低热层钠层  Es层  大气风场  
收稿时间:2016-12-06

Simultaneous measurements of TeSL,Es layer and atmospheric wind in Beijing,China (116.0°E, 40.5°N) on 26 May 2011
XUN Yu-Chang,YANG Guo-Tao,WANG Ji-Hong,DU Li-Fang,JIAO Jing,WANG Ze-Long,CHENG Xue-Wu,WANG Chi. Simultaneous measurements of TeSL,Es layer and atmospheric wind in Beijing,China (116.0°E, 40.5°N) on 26 May 2011[J]. Chinese Journal of Geophysics, 2017, 60(11): 4390-4397. DOI: 10.6038/cjg20171126
Authors:XUN Yu-Chang  YANG Guo-Tao  WANG Ji-Hong  DU Li-Fang  JIAO Jing  WANG Ze-Long  CHENG Xue-Wu  WANG Chi
Affiliation:1. State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China;2. Wuhan Institute of Physics and Mathematics, Chinese Academy of Sciences, Wuhan 430071, China;3. College of Earth Science, University of Chinese Academy of Sciences, Beijing 100049, China
Abstract:We report a lower thermospheric-enhanced sodium layer (TeSL) case observed at Yanqing station in Beijing, China (116.0°E,40.5°N) on 26 May 2011. From starting to collect data to the end of the observation, the density of lower thermospheric sodium layer was constantly enhanced. Its peak density increased from 250 cm-3 to 1500 cm-3. However, its peak height decreased from 111 km to 100 km gradually. At the same time, an ionosonde away from 28 km detected a Es layer in 106 km to 117 km, The average intensity of the Es layer was 4.5 MHz. According to the observational data of meteor radar, we fitted zonal wind over 100 km, and found the wind shear node decreased from 122 km to 108 km. The evolution trend of the Es layer and zonal wind were similar to the TeSL.We calculated vertical velocity of ions and the production rate of radiative recombination, and explained the density and height of the sodium atoms. We speculate the Na+ converged by wind shear mechanism. Furthermore, the thermospheric sodium layers are neutralized from converged Na+ layers.
Keywords:Lidar  TeSL  Es layer  Atmospheric wind
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