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On the VHF radar echoes in the region of midnight aurora: Signs of ground echoes modulated by the ionosphere

机译:在午夜极光区域的甚高频雷达回波上:电离层调制的地面回波迹象

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摘要

We present all-sky interferometric meteor radar (MR), VHF (36.9 MHz), observations from Sodankylä Geophysical Observatory and report on the unusual echoes, which were detected at low elevation on the northern horizon, typically during substorms. These echoes have a near-zero Doppler shift, relatively low power, but with a sharp rise to the power peak, short lifetime (less than 2 s), and nonexponential decay (NED). We suggest that such auroral NED echoes are in fact ground backscatter of the MR waves which have been refracted in the ionosphere, passing through the ionosphere in the substorm region, where pulsating aurora (at a frequency higher than 1.7 Hz) occurs and causes quasiperiodic modulation of the wave propagation conditions, which leads to corresponding modulation of the amplitude of return. The MR treats such oscillating signal as meteor trails.
机译:我们介绍了全天空干涉流星雷达(MR),VHF(36.9 MHz),Sodankylä地球物理天文台的观测结果,并报告了异常回波,这些回波是在北部地平线低海拔(通常在亚暴期间)发现的。这些回波具有接近零的多普勒频移,相对较低的功率,但功率峰值急剧上升,寿命短(小于2µs)和非指数衰减(NED)。我们建议这样的极光NED回波实际上是已在电离层折射,穿过亚暴雨区中的电离层的MR波在地面的反向散射,在此发生了脉动极光(频率高于1.7 Hz)并引起了准周期调制传播条件的变化,导致对回波幅度的相应调制。 MR将这种振荡信号视为流星迹。

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  • 作者

    Kozlovsky, A.; Lester, Mark;

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  • 年度 2015
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  • 原文格式 PDF
  • 正文语种 en
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