| 基于TEROS的自然闪电X射线暴观测研究 |
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| 引用本文： | 张雄, 张阳, 李小强, 郑毅, 曹保锋, 王宇, 吕伟涛, 李鹏. 2024. 基于TEROS的自然闪电X射线暴观测研究. 地球物理学报, 67(1): 21-33, doi: 10.6038/cjg2023Q0461 |
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| 作者姓名： | 张雄 张阳 李小强 郑毅 曹保锋 王宇 吕伟涛 李鹏 |
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| 作者单位： | 1. 国民核生化灾害防护国家重点实验室, 北京 102205; 2. 中国气象科学研究院灾害天气国家重点实验室, 北京 100081; 3. 国网电力科学研究院武汉南瑞有限责任公司, 武汉 430074 |
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| 基金项目： | 中国科学院战略性先导科技专项(XDA17040503), 国防科技基础加强计划技术领域基金, 中国气象科学研究院基本科研业务费项目(2021Z011)联合资助 |
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| 摘 要： | 本文报道了国内首个自然闪电高能辐射(Lightning Energetic Radiation, LER)多点观测结果. 基于自主研发的雷暴高能辐射观测系统(Thunderstorm Energetic Radiation Observation System, TEROS), 在2021年夏季观测期成功捕获3次自然LER事件, 结合闪电定位、低频快电场变化、回击峰值电流等其他资料, 对3次事件的高能辐射特征进行研究. 分析发现: 3次LER事件均于负地闪下行先导的最后阶段被探测到, 是典型的X射线暴, 且均具有MeV能量的单光子, 最大能量超过2.2 MeV; 伴随梯级先导出现的X射线暴持续时间为数百μs, 伴随不规则直窜先导的X射线暴持续时间为数十μs, 主要与先导发展速度有关; 相应回击峰值电流最大的1次事件具有最高的单光子能量、最大的单位面积沉积总能量和最多的爆发过程数量, 随着接近回击时刻, 该事件还表现出与电场变化一致的增强趋势, 表明先导头部电场是影响高能辐射产生的重要因素; 随到达强度降低, 高能辐射信号逐渐由束流模式向单光子模式转变, 呈现出与地球伽马射线闪类似的现象学特征, 更多乃至所有的爆发过程无法被探测到, 高能辐射可能是闪电发展过程中的普遍现象.
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| 关 键 词： | 闪电高能辐射 自然闪电 X射线暴 地球伽马射线闪 闪电先导 |
| 收稿时间： | 2022-06-16 |
| 修稿时间： | 2023-02-19 |
Observations of X-ray bursts from natural lightning flashes by TEROS |
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| ZHANG Xiong, ZHANG Yang, LI XiaoQiang, ZHENG Yi, CAO BaoFeng, WANG Yu, LÜ WeiTao, LI Peng. 2024. Observations of X-ray bursts from natural lightning flashes by TEROS. Chinese Journal of Geophysics (in Chinese), 67(1): 21-33, doi: 10.6038/cjg2023Q0461 |
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| Authors: | ZHANG Xiong ZHANG Yang LI XiaoQiang ZHENG Yi CAO BaoFeng WANG Yu LÜ WeiTao LI Peng |
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| Affiliation: | 1. State Key Laboratory of NBC Protection for Civilian, Beijing 102205, China; 2. State Key Laboratory of Severe Weather, Chinese Academy of Meteorological Sciences, Beijing 100081, China; 3. Wuhan NARI Limited Liability Company, State Grid Electric Power Research Institute, Wuhan 430074, China |
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| Abstract: | This work presents the first multi-point observations of natural Lightning Energetic Radiation (LER) in China. In summer of 2021, 3 LER events were recorded by the independently-developed Thunderstorm Energetic Radiation Observation System (TEROS). Combining with the lightning location data, low-frequency fast electric field change waveforms and return stroke peak currents, the energetic radiation characteristics of the 3 events are investigated in detail. All of the 3 LER events were detected during the last stages of the downward leaders before the negative cloud-to-ground lighting return strokes, which were typical X-ray bursts having photons with energy of MeV, and the maximum energy exceeded 2.2 MeV. The durations of the 2 X-ray bursts accompanying the stepped leaders were hundreds of microseconds, while the duration of the other one accompanying the chaotic dart leader was tens of microseconds, which can be attributed to the difference of the developing speeds of various types of leaders. The X-ray burst with the largest return stroke peak current had the highest single photon energy, the largest total deposited energy per unit area and the largest number of burst process. While approaching the return stroke, the intensity of this event also showed an increasing trend consistent with the electric field change, indicating that the electric field at the leader tip is an important factor affecting the production of energetic radiation. With the decrease of the arrival intensity, the energetic radiation signals gradually changed from the beam mode to the single photon mode, showing the phenomenological characteristics similar to Terrestrial Gamma-ray Flashes (TGFs), and more or even all of the burst processes could not be detected. We suggest that energetic radiation may be a common phenomenon during the development of lightning. |
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| Keywords: | Lightning Energetic Radiation (LER) Natural lightning X-ray burst Terrestrial Gamma-ray Flashes (TGFs) Lightning leader |
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