Abstract The Astroneu Extensive Air Shower (EAS) array comprises autonomous detection stations; each station consisting of 3 large scintillator detectors and one or more Radio Frequency (RF) antennas. The scintillator detectors of a station are able to detect showers with a low energy threshold of 20 − 30 TeV, at a rate of 10 − 20 showers per hour depending on the station geometrical layout. The RF antennas are used to detect very high energy EAS (E > 1017eV) through their radio wave emission. This work focuses in reconstructing and studying showers that have been detected synchronously by the scintillator detectors of two distant Astroneu stations. The performance of the array to detect and reconstruct the direction of such high energy (E > 5 · 1015eV) showers is evaluated by comparing the experimental measurements to the predictions of a detail Monte Carlo (MC) simulation.

中文翻译：

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通过 Astroneu 广泛的空气淋浴阵列检测高能淋浴

摘要 Astroneu Extensive Air Shower (EAS) 阵列包括自主探测站；每个站由 3 个大型闪烁体探测器和一个或多个射频 (RF) 天线组成。一个站的闪烁体探测器能够以每小时 10 - 20 个阵雨的速度检测 20 - 30 TeV 低能量阈值的阵雨，具体取决于站的几何布局。射频天线用于通过其无线电波发射检测非常高能量的 EAS (E > 1017eV)。这项工作的重点是重建和研究由两个遥远的 Astroneu 站的闪烁体探测器同步探测到的流星雨。阵列检测和重建这种高能量方向的性能 (E >