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The Ionospheric Response to the Annular Solar Eclipse on 26th January 2009

机译:2009年1月26日对环形日食的电离层反应

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The paper examines the ionspheric responses to the annular solar eclipse on 26th January 2009 over Southern Atlantic, Australia and Indian Ocean. The solar eclipse event took place during quiet solar and magnetic activities with maximum Kp and Dst indices are 3 and -32 nT. The external contacts of penumbra U1 and U4 occurred at 06:02:39 UT in the South Atlantic and 09:54:44 UT in the Celebes Sea. The GPS Total Electron Content (TEC) measurements obtained from 5 GPS stations belonging to International GNSS Service (IGS) network over India, Australia, and Antarctica have been employed in the analysis. 5 stations had been selected to conduct this study. They are Syowa in Antarctica, Windhoek in Namibia, Indian Institute of Science in India, Ceduna and Kerguelen Islands in Australia. The observations showed clear depletion in the TEC level from about 0.4 to 20% during the eclipse period.
机译:本文审查了2009年1月26日在南大西洋,澳大利亚和印度洋的环形日食对环形日食的反应。太阳日食事件发生在安静的太阳能和磁性活动期间,最大KP和DST指数为3和-32 NT。 Penumbra U1和U4的外部联系人在南大西洋和09:54:44 UT在Celebes Sea中发生的06:02:39。在分析中,从属于国际GNSS服务(IGS)网络的5个GPS站获得的GPS全电子含量(TEC)测量已经在分析中受雇。选择了5个站进行这项研究。他们是南极洲的南极洲的Syowa,印度印度科学研究所,Ceduna和Kerguelen岛屿在澳大利亚。观察结果表明,在Eclipse期间,TEC水平的清除耗竭量为约0.4至20%。

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