雷暴地面增强(TGEs)的时空结构

Q2 Physics and Astronomy Physics Open Pub Date : 2023-12-19 DOI:10.1016/j.physo.2023.100202
A. Chilingarian, D. Pokhsraryan, F. Zagumennov, M. Zazyan
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引用次数: 0

摘要

我们利用阿拉加茨岛上的粒子探测器网络分析了雷暴地面增强(TGE)的结构。我们利用 2023 年 5 月 23 日发生的有记录以来最大的 TGE 事件,在纳秒时间尺度上对粒子到达时间序列进行了统计分析。我们的研究结果证实,TGE 是多个失控电子雪崩的混合物,它们独立到达并提供稳定的粒子流。电子加速器由出现在雷云下部的偶极子驱动,向地球表面发射大量电子和伽马射线,并持续数分钟。实验结果得到了强大气电场中电子倍增和加速模拟的支持。我们将 TGEs 与地面伽马闪光(TGFs)进行了比较,后者是由轨道上的伽马射线探测器观测到的短暂爆发,被认为与大气放电有关。
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Space-temporal structure of the thunderstorm ground enhancements (TGEs)

We analyzed the structure of the Thunderstorm Ground Enhancement (TGE) using a particle detector network on Aragats. We performed a statistical analysis of the particle arrival time series on a nanosecond time scale using the largest TGE event on record, which occurred on May 23, 2023. Our findings confirm that the TGE is a mixture of multiple runaway electron avalanches that arrive independently and provide stable particle flux. The electron accelerator, operated by the dipole that emerges in the lower part of the thundercloud, sends copious electrons and gamma rays toward the Earth's surface that sustains for minutes. The experimental results are supported by simulations of electron multiplication and acceleration in strong atmospheric electric fields. We compare TGEs and Terrestrial Gamma Flashes (TGFs), which are brief bursts observed by gamma-ray detectors in orbit and are thought to be associated with atmospheric discharges.

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来源期刊
Physics Open
Physics Open Physics and Astronomy-Physics and Astronomy (all)
CiteScore
3.20
自引率
0.00%
发文量
19
审稿时长
9 weeks
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