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ANALYSIS OF CLAP SOUNDS RECORDED DURING THE SEPTEMBER 9-10 2011 GEOMAGNETIC STORM

机译:2011年9月9日至10日录制的拍摄声音分析

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Strong geomagnetic storms accompanied with bright and lively aurora may produce audible sounds perceivable at ground level. However, the physical origin of these emissions is not yet known. In order to understand the phenomenon, sound recordings with simultaneous electric or magnetic field measurements have been performed at different locations in Finland during geomagnetic storms since 2000. One such measurement was performed on September 9, 2011 near the village of Fiskars in southern Finland. The main goal was to test out new instruments and to demonstrate the measurement procedure to a colleague from the University of Graz, Austria. Signals were stored in WAV format using a Zoom H4n four-channel audio recorder. One stereo signal was recorded from the internal microphones of the Zoom unit while the second stereo signal consisted of an audio signal from a separate B&K low-noise measuring microphone mounted at the focal point of a parabolic reflector. The latter signal was recorded on one channel while the other channel consisted of a VLF antenna signal. The total duration of the recording was 130.6 minutes and covered a time interval approximately from 19 to 21 UTC. Twenty-one short sound events, clearly discernible from the background noise, were detected afterwards in the recording. The best ten were selected for closer analysis. These were the loudest events (claps) and exhibited relatively high mutual cross-correlations and a low background noise. Three of these events were detected with all three microphones. This is the first time during our studies when similar sound events were recorded simultaneously with multiple microphones during a geomagnetic storm. Knowing the separation distance of the microphones (B&K vs. Zoom) it was possible to estimate the direction of the sound source. The synchronously recorded VLF signal provided data to estimate the distances of the sound sources assuming that a certain magnetic field event is associated with a certain sound event. Three independent methods to estimate distance to the sound sources yielded an average value of 70 meters. This outcome, together with the direction estimate, indicates that the average altitude of the sound sources measured from ground was only 60-70 meters.
机译:强大的地磁风暴伴随着明亮而活泼的极光可能会产生在地面上可感知的声音。但是,这些排放的物理来源尚不清楚。为了理解现象,自2000年以来,在芬兰的不同位置,在芬兰的不同地点进行了具有同时电场或磁场测量的响应。2011年9月9日在芬兰南部的Fiskars村进行了一个这样的测量。主要目标是测试新仪器,并展示来自奥地利格拉茨大学的同事的测量程序。使用Zoom H4N四通道音频记录器在WAV格式中存储信号。从变焦单元的内部麦克风记录一个立体声信号,而第二立体声信号由来自安装在抛物线反射器的焦点的单独的B&k低噪声测量麦克风的音频信号组成。后一个信号被记录在一个通道上,而另一个信道由VLF天线信号组成。记录的总持续时间为130.6分钟,覆盖约19到21 UTC的时间间隔。在录制中,在后台噪声中检测到二十一条短声事件,清晰可辨别。最好的十个被选中以进行更密切的分析。这些是最响亮的事件(CLAPS),并且表现出相对高的相互互相关和低背景噪声。用所有三个麦克风检测到其中三个事件。这是在我们在地磁风暴期间与多个麦克风同时记录类似的声音事件时第一次。知道麦克风的分离距离(B&k与变焦)可以估计声源的方向。同步录制的VLF信号提供了数据来估计声源的距离,假设某个磁场事件与某个声音事件相关联。三种独立的方法来估计与声源的距离产生的平均值为70米。这种结果与方向估计表明,从地面测量的声源的平均海拔仅为60-70米。

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