Atmospheric Gamma-ray Observations at the Telescope Array Detector

Atmospheric Gamma-ray Observations at the Telescope Array Detector
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望远镜阵列探测器的大气伽马射线观测

DOI:
10.1088/1742-6596/2398/1/012008
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发表时间:
2022
期刊:
Journal of Physics: Conference Series
影响因子:
--
通讯作者:
Abbasi, R.
Abbasi, R.
中科院分区:
--
文献类型:
--
作者:
Abbasi, R.

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此前在AtmoHead-2018上,我们报告了望远镜阵列表面探测器(TASD)、闪电测绘阵列(LMA)、SERIC传感器和宽带干涉仪对与闪电重合的粒子簇射的联合观测。其中包括持续时间约不到10微秒的高能阵雨,地面足迹直径为3-6公里,起源于向下的闪电先导的前一至两毫秒,并与先导内部的强电流过程重合。闪烁体波形和模拟研究证实,这些流星雨必须主要由伽马辐射组成。
Previously in AtmoHead-2018, we reported joint observations by Telescope Array Surface Detector (TASD), Lightning Mapping Array (LMA), sferic sensor and broadband interferometer of particle showers coincident with lightning. These consisted of energetic showers of approximately less than 10 microsecond duration with footprints on the ground of 3-6 kilometers in diameter, originating in the first one to two milliseconds of downward lightning leaders and coincident with high-current processes within the leaders. Scintillator waveform and simulation studies confirmed that these showers must consist primarily of gamma radiation.
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