探测大面积空气淋点的全覆盖方法

Giuseppe Di Sciascio
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引用次数: 0

摘要

利用全覆盖方法的阵雨阵列具有高分割的读数,可以以前所未有的分辨率和细节对大气阵雨的前部进行成像。栅格距离决定了能量阈值(检测器之间的间隙会损失小能量簇)和簇采样的质量。因此,需要这种实验解决方案来检测阈值在100 GeV范围内的阵雨。ARGO-YBJ实验采用了全覆盖方法。在这篇文章中,我们将总结这种技术的优点,并讨论在新的宽视场检测器中的可能应用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The full coverage approach to the detection of Extensive Air Showers
A shower array exploiting the full coverage approach with a high segmentation of the readout allow to image the front of atmospheric showers with unprecedented resolution and detail. The grid distance determines the energy threshold (small energy showers are lost in the gap between detectors) and the quality of the shower sampling. Therefore, this experimental solution is needed to detect showers with a threshold in the 100 GeV range. The full coverage approach has been exploited in the ARGO-YBJ experiment. In this contribution we will summarise the advantages of this technique and discuss possible applications in new wide field of view detectors.
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