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Automatic Detection of Omega Signals Captured by the Poynting Flux Analyzer (PFX) on Board the Akebono Satellite

机译:poynting Flux捕获的Omega信号的自动检测   akebono卫星上的分析仪(pFX)

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摘要

The Akebono satellite was launched in 1989 to observe the Earth'smagnetosphere and plasmasphere. Omega was a navigation system with 8 groundstations transmitter and had transmission pattern that repeats every 10 s. From1989 to 1997, the PFX on board the Akebono satellite received signals at 10.2kHz from these stations. Huge amounts of PFX data became valuable for studyingthe propagation characteristics of VLF waves in the ionosphere andplasmasphere. In this study, we introduce a method for automatic detection ofOmega signals from the PFX data in a systematic way, it involves identifying atransmission station, calculating the delay time, and estimating the signalintensity. We show the reliability of the automatic detection system where weable to detect the omega signal and confirmed its propagation to the oppositehemisphere along the Earth's magnetic field lines. For more than three years(39 months), we detected 43,734 and 111,049 signals in the magnetic andelectric field, respectively, and demonstrated that the proposed method ispowerful enough for the statistical analyses.
机译:1989年发射了Akebono卫星,用于观测地球的磁层和等离子层。欧米茄是具有8个地面站发射机的导航系统,其传输模式每10秒钟重复一次。从1989年到1997年,Akebono卫星上的PFX从这些电台接收了10.2kHz的信号。大量的PFX数据对于研究VLF波在电离层和等离子层中的传播特性非常有价值。在这项研究中,我们介绍了一种系统地从PFX数据自动检测Omega信号的方法,该方法涉及识别传输站,计算延迟时间并估算信号强度。我们展示了自动检测系统的可靠性,该系统可用于检测欧米茄信号并确认其沿地球磁场线传播到对半球。在三年多的时间(39个月)中,我们分别在磁场和电场中检测到43,734和111,049信号,并证明了该方法足以进行统计分析。

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