题名 | 3D density imaging of cosmic-ray muography with adjustable angular resolutions |
作者 | |
通讯作者 | Wu, Chenyan |
DOI | |
发表日期 | 2022-08-15
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会议名称 | 2nd International Meeting for Applied Geoscience and Energy, IMAGE 2022
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ISSN | 1052-3812
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EISSN | 1949-4645
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会议录名称 | |
卷号 | 2022-August
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页码 | 2035-2039
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会议日期 | August 28, 2022 - September 1, 2022
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会议地点 | Houston, TX, United states
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出版者 | |
摘要 | Using cosmic-ray muons as the probe for density structures, muography has advantages in detecting cavities and fracture zones for engineering applications in the mountainous area, because it is not disturbed by vibration and electromagnetic noise and does not require fieldwork over rough terranes. However, the conventional muon detector is bulky and often requires a long observation time to accumulate a statistically significant number of muon events. This study presents a new concept of muon detector with smaller sensor arrays and adjustable angular resolutions for improved portability and efficiency. The detector uses two 7×7-pixel plates to record the arrivals of moun particles; the size of each pixel is 5×5 cm2. The angular resolution can be adjusted by changing the plate separation. A smaller separation has a lower angular resolution of ray paths but can accumulate sufficient muon events more quickly. Firstly, the empirical formula for calculating observed muon flux is introduced. The observed flux can be simulated for the direction with a known zenith angle by calculating opacity data along the path. Then we develop a forward algorithm of opacity data simulation at variable plate separations to ensure the accuracy of flux calculation. In our example, a mountain model with a low-density fracture zone is designed. Four muon detectors are placed at the western, eastern, northern, and southern feet of the mountain. The forward flux data at the four detectors is converted into opacity data through the corresponding relationship calculated by the empirical formula for inversion. Finally, our synthetic inversions find that a smaller plate separation and a lower angular resolution can still accurately locate the fault location using mountain-foot observations, but at the cost of lower spatial resolution in the inversion model. Our numerical simulations have proven the feasibility of 3D muon tomography with adjustable angular resolutions for more efficient applications in engineering problems. © 2022 Society of Exploration Geophysicists and the American Association of Petroleum Geologists. |
学校署名 | 第一
; 通讯
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语种 | 英语
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收录类别 | |
资助项目 | This research was funded by the Featured Innovation Programs for Universities of Guangdong Province grant no. 2021KTSCX105 and Special Funds for the Cultivation of Guangdong College Students' Scientific and Technological Innovation no. pdjh2022c0015.This research was funded by the Featured Innovation Programs for Universities of Guangdong Province grant no. 2021KTSCX105 and Special Funds for the Cultivation of Guangdong College Students’ Scientific and Technological Innovation no. pdjh2022c0015.
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EI入藏号 | 20230413445722
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EI主题词 | Charged particles
; Cosmology
; Landforms
; Opacity
; Particle spectrometers
; Plates (structural components)
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EI分类号 | Structural Members and Shapes:408.2
; Geology:481.1
; Space Physics:657
; Extraterrestrial Physics and Stellar Phenomena:657.2
; Light/Optics:741.1
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来源库 | EV Compendex
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引用统计 |
被引频次[WOS]:0
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成果类型 | 会议论文 |
条目标识符 | http://sustech.caswiz.com/handle/2SGJ60CL/519764 |
专题 | 理学院_地球与空间科学系 |
作者单位 | Department of Earth and Space Sciences, Southern University of Science and Technology, China |
第一作者单位 | 地球与空间科学系 |
通讯作者单位 | 地球与空间科学系 |
第一作者的第一单位 | 地球与空间科学系 |
推荐引用方式 GB/T 7714 |
Wu, Chenyan,Yang, Dikun,Chen, Zhongchang,et al. 3D density imaging of cosmic-ray muography with adjustable angular resolutions[C]:Society of Exploration Geophysicists,2022:2035-2039.
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条目包含的文件 | 条目无相关文件。 |
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