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Localization of VLF ionospheric exit point by comparison of multipoint ground-based observation with full-wave analysis

机译:通过多点地面观测与全波分析的比较,对VLF电离层出口点进行定位

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摘要

In order to estimate the dynamic structure of the VLF ionospheric exit point, we conducted multipoint ground-based observation of the natural VLF emissions at three unmanned sites: West Ongul (69°01' S, 39°30' E), Skallen (69°40' S, 39°24' E), and H100 (69°18' S, 41°19' E) around Japanese Syowa station, Antarctica, during a whole year of 2006. In this observation, we developed three sets of unmanned autonomous observation systems for natural VLF emissions. Each observation system consists of two crossed vertical loop antennas to pick-up North-South (NS) and East-West (EW) magnetic components, a multi-channel analyzer, and a data logger. The intensity and polarization of NS and EW magnetic components are obtained in 4 spaced frequency (0.5,1.0, 2.0, and 6.0 kHz) channels by the multi-channel analyzer.rnThe VLF emissions observed at the three sites exhibit an interesting difference in the wave intensity as well as the polarization that allows important information about the locations of their ionospheric exit point to be determined. Firstly, to find the distinct exit point, we have theoretically calculated the spatial distributions of the wave intensity and the polarization on the Earth for VLF whistler mode waves coming down from the magnetized ionosphere, by using the full-wave analysis. Then, we have compared the calculated results with the observed data, to evaluate the possible locations of the ionospheric exit point for the auroral hiss events.rnAs an example, the direction of the estimated ionospheric exit point for the auroral hiss event at 31 March 2006 was found to be consistent with a bright aurora region. However, in this case, the estimated ionospheric exit point was located a few hundred kilometers equatorward of the associated aurora. This would suggest that the ray paths for the auroral hiss could be different from the directions of the geomagnetic field lines for auroral precipitation.
机译:为了估算VLF电离层出口点的动态结构,我们对三个无人驾驶地点的自然VLF排放进行了多点地面观测:西昂古尔(69°01'S,39°30'E),Skallen(69 2006年全年,在南极洲日本Syowa站周围的40°S,39°24'E和H100(69°18'S,41°19'E)周围。用于自然甚低频排放的无人自主观测系统。每个观测系统都包括两个交叉的垂直环形天线以拾取南北(NS)和东西(EW)磁性元件,一个多通道分析仪和一个数据记录器。通过多通道分析仪在4个间隔的频率(0.5、1.0、2.0和6.0 kHz)通道中获得了NS和EW磁性成分的强度和极化.rn在三个位置观察到的VLF发射在波中表现出有趣的差异强度以及极化可以确定有关其电离层出口点位置的重要信息。首先,为了找到明显的出射点,我们通过全波分析,从理论上计算了来自磁化电离层的VLF惠斯勒模式波的波强度和极化在地球上的空间分布。然后,我们将计算结果与观测数据进行了比较,以评估极光嘶嘶事件的电离层出口点的可能位置.rn例如,2006年3月31日极光嘶嘶事件的估计电离层出口点的方向被发现与明亮的极光区域一致。但是,在这种情况下,估计的电离层出口点位于相关极光的赤道面几百公里处。这表明极光嘶嘶声的射线路径可能不同于极光降水的地磁场线的方向。

著录项

  • 来源
    《Polar science》 |2008年第4期|p.237-249|共13页
  • 作者单位

    Graduate School of Natural Science & Technology, Kanazawa University, Kakuma-machi, Kanazawa 920-1192, Japan;

    rnGraduate School of Natural Science & Technology, Kanazawa University, Kakuma-machi, Kanazawa 920-1192, Japan;

    rnKanazawa University, Kakuma-machi, Kanazawa 920-1192, Japan;

    rnGraduate School of Natural Science & Technology, Kanazawa University, Kakuma-machi, Kanazawa 920-1192, Japan;

    rnNational Institute of Polar Research, 1-9-10 Kaga, ltabashi-ku, Tokyo 173-8515, Japan;

    rnNational Institute of Polar Research, 1-9-10 Kaga, ltabashi-ku, Tokyo 173-8515, Japan;

    rnNational Institute of Polar Research, 1-9-10 Kaga, ltabashi-ku, Tokyo 173-8515, Japan;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    unmanned observation; natural VLF emissions; lonospheric exit point; full-wave analysis; antarctica;

    机译:无人观察VLF自然排放;球形出口点;全波分析;南极洲;

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