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作 者:熊波[1] 张燕革[1] 艾勇[1] 张虹[1] 刘珏[1]
出 处:《空间科学学报》2013年第6期629-636,共8页Chinese Journal of Space Science
基 金:国家高技术研究发展计划项目资助
摘 要:极光亚暴是地球空间基本的能量输入、耦合及耗散过程,其对低热层大气中性风的影响不容忽视,对这一问题进行深入研究具有重要意义.2010年11月,中国北极黄河站(78.92°N,11.93°E)安装了一台自主研制的全天空法布里-珀罗干涉仪(FPI)并开始进行正常观测,为中国首次获得了极光亚暴期间的FPI观测数据.根据2012年越冬期间的观测情况,对2012年11月12—14日及12月09—11日两个极光亚暴事件期间的数据进行处理,计算得到了5级干涉环对应的风场.亚暴期间风场变化与地磁活动变化的对比分析表明,风速的剧烈变化可能是由地磁活动剧烈扰动造成的.针对2012年11月13日00:00 UT—02:00 UT和2012年12月10日05:00 UT—07:30 UT的亚暴事件,将全天空相机拍摄到的极光图像与FPI干涉图像对应的视线风场进行对比分析.结果表明在极光活动中,视线风速加强的方向与极光弧的方向垂直,而在极光弧的平行方向,风速相对较小.Auroral substorm is a basic energy input, coupling and dissipation process. Complex auroral substorm effects are not to be neglected for the thermospheric neutral wind effects, and has important significance on its in-depth study. A self-developed Ml-sky Fabry-Perot Interferometer (FPI) has been deployed by Chinese Arctic Yellow River Station (78.92°N, 11.93°E) at Ny-Alesund, Svalbard in November 2010, and formal observation has been carried out, which obtained FPI mea- sured data for the first time in domestic. This paper briefly introduces the observations during winter in 2012. Two auroral substorm events on November 12--14, 2012 and December 9-11, 2012 were selected for data processing, and wind fields corresponded to 5 interference rings were calculated. The comparison and analysis between1 wind field and geomagnetic activity variations during the pe- riods of auroral substorms indicated that the dramatic change of wind speed may be caused by a violent disturbance of geomagnetic activity. Contrastive analyses between auroral images by an all sky camera and FPI interference fringes corresponding line of sight wind field during November 13, 2012, 00:00 UT--02:00 UT and December 10, 2012, 05:00 UT--07:30UT suggest that the enhanced direction is perpendicular to the aur,~ra arc, and it weakens in the direction paralleled with the arc.
关 键 词:极光亚暴 法布里珀罗干涉仪 热层中性风 地磁活动
分 类 号:P353.7[天文地球—空间物理学]
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