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Analysis of Signals from an Unique Ground-Truth Infrasound Source Observed at IMS Station IS26 in Southern Germany

机译:在德国南部的IMS站IS26观察到的来自唯一的地面对地次声源的信号的分析

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Quantitative modeling of infrasound signals and development and verification of the corresponding atmospheric propagation models requires the use of well-calibrated sources. Numerous sources have been detected by the currently installed network of about 40 of the final 60 IMS infrasound stations. Besides non-nuclear explosions such as mining and quarry blasts and atmospheric phenomena like auroras, these sources include meteorites, volcanic eruptions and supersonic aircraft including re-entering spacecraft and rocket launches. All these sources of infrasound have one feature in common, in that their source parameters are not precisely known and the quantitative interpretation of the corresponding signals is therefore somewhat ambiguous. A source considered well-calibrated has been identified producing repeated infrasound signals at the IMS infrasound station IS26 in the Bavarian forest. The source results from propulsion tests of the ARIANE-5 rocket’s main engine at a testing facility near Heilbronn, southern Germany. The test facility is at a range of 320 km and a backazimuth of ~280° from IS26. Ground-truth information was obtained for nearly 100 tests conducted in a 5-year period. Review of the available data for IS26 revealed that at least 28 of these tests show signals above the background noise level. These signals are verified based on the consistency of various signal parameters, e.g., arrival times, durations, and estimates of propagation characteristics (backazimuth, apparent velocity). Signal levels observed are a factor of 2–8 above the noise and reach values of up to 250 mPa for peak amplitudes, and a factor of 2–3 less for RMS measurements. Furthermore, only tests conducted during the months from October to April produce observable signals, indicating a significant change in infrasound propagation conditions between summer and winter months.
机译:次声信号的定量建模以及相应的大气传播模型的开发和验证需要使用校准良好的信号源。当前安装的网络中最后60个IMS次声台站中的约40个已检测到许多源。除了诸如采矿和采石场爆炸之类的非核爆炸以及极光之类的大气现象外,这些来源还包括陨石,火山喷发和超音速飞机,包括重新进入的航天器和火箭发射。所有这些次声源都有一个共同的特征,即它们的源参数无法精确得知,因此对相应信号的定量解释有些模棱两可。在巴伐利亚森林的IMS次声台站IS26,已经确定了一个经过良好校准的信号源,可产生重复的次声信号。消息来源是在德国南部海尔布隆附近的一个测试设施中对ARIANE-5火箭的主发动机进行推进测试的结果。测试设备的距离为320 km,与IS26的后方位角约为280°。在5年中进行了近100次测试,获得了真实的信息。查看IS26的可用数据后发现,这些测试中至少有28个显示出高于背景噪声水平的信号。这些信号是根据各种信号参数(例如到达时间,持续时间和传播特性(后方位角,视在速度)的估计值)的一致性进行验证的。观察到的信号电平比噪声高2-8倍,峰值幅度高达250 mPa,而RMS测量则低2-3倍。此外,只有在十月至四月的几个月中进行的测试才能产生可​​观察到的信号,表明次夏和冬季之间次声传播条件发生了重大变化。

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