{"title":"First results of terrestrial gamma-ray flash observed by Insight-HXMT","authors":"Qibin Yi, Yi Zhao, Shaolin Xiong, Xuejuan Yang, Ce Cai, Shuo Xiao, Gang Li, Gaopeng Lu, Hongbo Zhang, Fanchao Lyu, Wei Xu, Xiaobo Li, Chengkui Li, Mingyu Ge, Haisheng Zhao, Wangchen Xue, Jiacong Liu, Chao Zheng, Yanqiu Zhang, Chenwei Wang, Wenjun Tan, Shenglun Xie, Yue Huang, Zhi Chang, Congzhan Liu, Fangjun Lu, Liming Song, Yupeng Xu, Zhen Zhang, Shuangnan Zhang, Tipei Li","doi":"10.1007/s11433-024-2599-4","DOIUrl":null,"url":null,"abstract":"<div><p>As China’s first X-ray astronomy satellite, the hard X-ray modulation telescope (Insight-HXMT) carries three sets of X-ray telescopes. The high energy X-ray telescope (<i>Insight</i>-HXMT/HE) could serve as an all-sky gamma-ray monitor with a detection area of up to 5000 cm<sup>2</sup> and energy range from about 200 keV to 3 MeV. These characteristics, together with the high orbital inclination angle (43°) of the satellite, make the HE very suitable for detecting terrestrial gamma-ray flashes (TGFs). In this work, we implemented a dedicated TGF search algorithm for Insight-HXMT/HE, and identified 282 bright TGFs in its first four years of operation. We made a systematic study on the properties of these TGFs, including trigger time, duration, intensity, as well as the lightning association. We found that TGFs detected in mid-latitude regions (30° to 43°) are rare and they do not exhibit significantly different properties compared with TGFs in low-latitude (within 30°). Interestingly, the hardness ratio of TGF measured by <i>Insight</i>-HXMT/HE seems to be independent of the TGF duration, which differs from previous studies. These results show that, despite the dedicated design for astronomical observation, <i>Insight</i>-HXMT/HE is a versatile instrument to study energetic radiation phenomena from the Earth.</p></div>","PeriodicalId":774,"journal":{"name":"Science China Physics, Mechanics & Astronomy","volume":"68 5","pages":""},"PeriodicalIF":6.4000,"publicationDate":"2025-03-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Science China Physics, Mechanics & Astronomy","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s11433-024-2599-4","RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0
Abstract
As China’s first X-ray astronomy satellite, the hard X-ray modulation telescope (Insight-HXMT) carries three sets of X-ray telescopes. The high energy X-ray telescope (Insight-HXMT/HE) could serve as an all-sky gamma-ray monitor with a detection area of up to 5000 cm2 and energy range from about 200 keV to 3 MeV. These characteristics, together with the high orbital inclination angle (43°) of the satellite, make the HE very suitable for detecting terrestrial gamma-ray flashes (TGFs). In this work, we implemented a dedicated TGF search algorithm for Insight-HXMT/HE, and identified 282 bright TGFs in its first four years of operation. We made a systematic study on the properties of these TGFs, including trigger time, duration, intensity, as well as the lightning association. We found that TGFs detected in mid-latitude regions (30° to 43°) are rare and they do not exhibit significantly different properties compared with TGFs in low-latitude (within 30°). Interestingly, the hardness ratio of TGF measured by Insight-HXMT/HE seems to be independent of the TGF duration, which differs from previous studies. These results show that, despite the dedicated design for astronomical observation, Insight-HXMT/HE is a versatile instrument to study energetic radiation phenomena from the Earth.
期刊介绍:
Science China Physics, Mechanics & Astronomy, an academic journal cosponsored by the Chinese Academy of Sciences and the National Natural Science Foundation of China, and published by Science China Press, is committed to publishing high-quality, original results in both basic and applied research.
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