中文版 | English
Title

3D density imaging of cosmic-ray muography with adjustable angular resolutions

Author
Corresponding AuthorWu, Chenyan
DOI
Publication Years
2022-08-15
Conference Name
2nd International Meeting for Applied Geoscience and Energy, IMAGE 2022
ISSN
1052-3812
EISSN
1949-4645
Source Title
Volume
2022-August
Pages
2035-2039
Conference Date
August 28, 2022 - September 1, 2022
Conference Place
Houston, TX, United states
Publisher
Abstract
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.
SUSTech Authorship
First ; Corresponding
Language
English
Indexed By
Funding Project
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.
EI Accession Number
20230413445722
EI Keywords
Charged particles ; Cosmology ; Landforms ; Opacity ; Particle spectrometers ; Plates (structural components)
ESI Classification Code
Structural Members and Shapes:408.2 ; Geology:481.1 ; Space Physics:657 ; Extraterrestrial Physics and Stellar Phenomena:657.2 ; Light/Optics:741.1
Data Source
EV Compendex
Citation statistics
Cited Times [WOS]:0
Document TypeConference paper
Identifierhttp://kc.sustech.edu.cn/handle/2SGJ60CL/519764
DepartmentDepartment of Earth and Space Sciences
Affiliation
Department of Earth and Space Sciences, Southern University of Science and Technology, China
First Author AffilicationDepartment of Earth and Space Sciences
Corresponding Author AffilicationDepartment of Earth and Space Sciences
First Author's First AffilicationDepartment of Earth and Space Sciences
Recommended Citation
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.
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Export to Excel
Export to Csv
Altmetrics Score
Google Scholar
Similar articles in Google Scholar
[Wu, Chenyan]'s Articles
[Yang, Dikun]'s Articles
[Chen, Zhongchang]'s Articles
Baidu Scholar
Similar articles in Baidu Scholar
[Wu, Chenyan]'s Articles
[Yang, Dikun]'s Articles
[Chen, Zhongchang]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Wu, Chenyan]'s Articles
[Yang, Dikun]'s Articles
[Chen, Zhongchang]'s Articles
Terms of Use
No data!
Social Bookmark/Share
No comment.

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.