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Beni T, Borselli D, Bonechi L, Lombardi L, Gonzi S, Melelli L, Turchetti MA, Fanò L, D'Alessandro R, Gigli G, Casagli N. Laser scanner and UAV digital photogrammetry as support tools for cosmic-ray muon radiography applications: an archaeological case study from Italy. Sci Rep 2023; 13:19983. [PMID: 37968324 PMCID: PMC10651839 DOI: 10.1038/s41598-023-46661-4] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/26/2023] [Accepted: 11/03/2023] [Indexed: 11/17/2023] Open
Abstract
The use of light detection and ranging technologies, i.e. terrestrial laser scanner (TLS), airborne laser scanner (ALS) and mobile laser scanner (MLS), together with the unmanned aerial vehicles digital photogrammetry (UAV-DP) and satellite data are proving to be fundamental tools to carry out reliable muographic measurement campaigns. The main purpose of this paper is to propose a workflow to correctly plan and exploit these types of data for muon radiography aims. To this end, a real case study is presented: searching for hidden tombs in the Etruscan necropolis of Palazzone (Umbria, Italy). A high-resolution digital elevation model (DEM) and three-dimensional models of the ground surface/sub-surface of the study area were created by merging data obtained using different survey methods to achieve the most accurate three-dimensional environment. Indeed, the simulated muon flux transmission used to infer relative transmission values, and the estimated density distribution, depends on the reliability of the three-dimensional reconstructed ground surface model. The aim of this study is to provide knowledge on the use of TLS and UAV-DP data and GPS-acquired points within the transmission-based muography process and how these data could improve or worsen the muon imaging results. Moreover, this study confirmed that muography applications require a multidisciplinary approach.
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Affiliation(s)
- Tommaso Beni
- Department of Earth Sciences, University of Florence, Via Giorgio La Pira 4, 50121, Florence, Italy.
| | - Diletta Borselli
- National Institute for Nuclear Physics INFN, Division of Florence, Via Bruno Rossi 1, 50019, Sesto Fiorentino, Italy
- Department of Physics and Geology, University of Perugia, Via Alessandro Pascoli, 06123, Perugia, Italy
| | - Lorenzo Bonechi
- National Institute for Nuclear Physics INFN, Division of Florence, Via Bruno Rossi 1, 50019, Sesto Fiorentino, Italy
| | - Luca Lombardi
- Department of Earth Sciences, University of Florence, Via Giorgio La Pira 4, 50121, Florence, Italy
| | - Sandro Gonzi
- National Institute for Nuclear Physics INFN, Division of Florence, Via Bruno Rossi 1, 50019, Sesto Fiorentino, Italy
- Department of Physics and Astronomy, University of Florence, Via Giovanni Sansone 1, 50019, Sesto Fiorentino, Italy
| | - Laura Melelli
- Department of Physics and Geology, University of Perugia, Via Alessandro Pascoli, 06123, Perugia, Italy
| | - Maria Angela Turchetti
- Ministry of Culture Regional Directorate of Museum Umbria, Necropolis of Palazzone, Perugia, Italy
| | - Livio Fanò
- Department of Physics and Geology, University of Perugia, Via Alessandro Pascoli, 06123, Perugia, Italy
- National Institute for Nuclear Physics INFN, Division of Perugia, Via Alessandro Pascoli, 06123, Perugia, Italy
| | - Raffaello D'Alessandro
- National Institute for Nuclear Physics INFN, Division of Florence, Via Bruno Rossi 1, 50019, Sesto Fiorentino, Italy
- Department of Physics and Astronomy, University of Florence, Via Giovanni Sansone 1, 50019, Sesto Fiorentino, Italy
| | - Giovanni Gigli
- Department of Earth Sciences, University of Florence, Via Giorgio La Pira 4, 50121, Florence, Italy
| | - Nicola Casagli
- Department of Earth Sciences, University of Florence, Via Giorgio La Pira 4, 50121, Florence, Italy
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2
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Tanaka HK, Gallo G, Gluyas J, Kamoshida O, Lo Presti D, Shimizu T, Steigerwald S, Takano K, Yang Y, Yokota Y. First navigation with wireless muometric navigation system (MuWNS) in indoor and underground environments. iScience 2023; 26:107000. [PMID: 37534132 PMCID: PMC10391674 DOI: 10.1016/j.isci.2023.107000] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/22/2022] [Revised: 04/20/2023] [Accepted: 05/24/2023] [Indexed: 08/04/2023] Open
Abstract
Navigation in indoor and underground environments has been extensively studied to realize automation of home, hospital, office, factory and mining services, and various techniques have been proposed for its implementation. By utilizing the relativistic and penetrative nature of cosmic-ray muons, a completely new wireless navigation technique called wireless muometric navigation system (MuWNS) was developed. This paper shows the results of the world's first physical demonstration of MuWNS used on the basement floor inside a building to navigate (a person) in an area where global navigation satellite system (GNSS)/ global positioning system (GPS) signals cannot reach. The resultant navigation accuracy was comparable or better than the positioning accuracy attainable with single-point GNSS/GPS positioning in urban areas. With further improvements in stability of local clocks used for timing, it is anticipated that MuWNS can be adapted to improve autonomous mobile robot navigation and positioning as well as other underground and underwater practical applications.
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Affiliation(s)
- Hiroyuki K.M. Tanaka
- The University of Tokyo, Tokyo, Japan
- International Virtual Muography Institute (VMI), Global, Tokyo, Japan
| | - Giuseppe Gallo
- International Virtual Muography Institute (VMI), Global, Tokyo, Japan
- University of Catania, Catania, Italy
| | - Jon Gluyas
- International Virtual Muography Institute (VMI), Global, Tokyo, Japan
- Durham University, Durham, UK
| | - Osamu Kamoshida
- International Virtual Muography Institute (VMI), Global, Tokyo, Japan
- NEC Corporation, Tokyo, Japan
| | - Domenico Lo Presti
- International Virtual Muography Institute (VMI), Global, Tokyo, Japan
- University of Catania, Catania, Italy
| | - Takashi Shimizu
- International Virtual Muography Institute (VMI), Global, Tokyo, Japan
- Technoland Corporation, Tokyo, Japan
| | - Sara Steigerwald
- International Virtual Muography Institute (VMI), Global, Tokyo, Japan
| | | | | | - Yusuke Yokota
- The University of Tokyo, Tokyo, Japan
- International Virtual Muography Institute (VMI), Global, Tokyo, Japan
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3
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Tanaka HK, Cerretto G, Gnesi I. First experimental results of the cosmic time synchronizer for a wireless, precise, and perpetual time synchronization system. iScience 2023; 26:106595. [PMID: 37192970 PMCID: PMC10182294 DOI: 10.1016/j.isci.2023.106595] [Citation(s) in RCA: 2] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/01/2022] [Revised: 01/15/2023] [Accepted: 04/04/2023] [Indexed: 05/18/2023] Open
Abstract
In 2022, the idea of the cosmic time synchronizer (CTS) was proposed for a precise wireless synchronization of local clocks (<100 ns). Because CTS does not require critical timing information traffic among CTS sensors, the technique can be considered robust against jamming and spoofing. In this work, a small-scale CTS sensor network has been developed and tested for the first time. Good time synchronization performances were obtained for a short-haul configuration (30-35 ns (SD, 1 σ), over 50-60 m). Based on the results of this work, CTS could be potentially conceived as a 'self-adjusting' system, offering high level continuous (perpetual) performances, to be considered either as a backup chain for GPS disciplined oscillators (GPS DO), a standalone standard for frequency and time interval measurements, or as a tool for the dissemination of reference time scales to final users, with improved characteristics in terms of robustness and reliability.
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Affiliation(s)
- Hiroyuki K.M. Tanaka
- University of Tokyo, Tokyo, Japan
- International Virtual Muography Institute, Global, Tokyo, Japan
- Corresponding author
| | - Giancarlo Cerretto
- International Virtual Muography Institute, Global, Tokyo, Japan
- Quantum Metrology and Nanotechnologies Division, Istituto Nazionale di Ricerca Metrologica, Torino, Italy
| | - Ivan Gnesi
- International Virtual Muography Institute, Global, Tokyo, Japan
- Fermi Research Center (CREF), Rome, Italy
- European Center for Nuclear Research (CERN), Geneva, Switzerland
- Istituto Nazionale di Fisica Nucleare, Frascati National Labs - Cosenza Group - Cosenza, Frascati, Italy
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4
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Tioukov V, Morishima K, Leggieri C, Capriuoli F, Kitagawa N, Kuno M, Manabe Y, Nishio A, Alexandrov A, Gentile V, Iuliano A, De Lellis G. Hidden chamber discovery in the underground Hellenistic necropolis of Neapolis by muography. Sci Rep 2023; 13:5438. [PMID: 37012348 PMCID: PMC10070482 DOI: 10.1038/s41598-023-32626-0] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/11/2022] [Accepted: 03/30/2023] [Indexed: 04/05/2023] Open
Abstract
We report in this paper the muography of an archaeological site located in the highly populated "Sanità" district in the center of Naples, ten meters below the current street level. Several detectors capable of detecting muons - high energy charged particles produced by cosmic rays in the upper layers of atmosphere - were installed underground at the depth of 18 m, to measure the muon flux over several weeks. By measuring the differential flux with our detectors in a wide angular range, we have produced a radiographic image of the upper layers. Despite the architectural complexity of the site, we have clearly observed the known structures as well as a few unknown ones. One of the observed new structures is compatible with the existence of a hidden, currently inaccessible, burial chamber.
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Affiliation(s)
- Valeri Tioukov
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Naples, Italy.
| | | | - Carlo Leggieri
- Associazione Celanapoli, via Santa Maria Antesaecula 129, Naples, Italy
| | | | - Nobuko Kitagawa
- Nagoya University, Furo-cho, Chikusa-ku, Aichi, Nagoya, 464-8602, Japan
| | - Mitsuaki Kuno
- Nagoya University, Furo-cho, Chikusa-ku, Aichi, Nagoya, 464-8602, Japan
| | - Yuta Manabe
- Nagoya University, Furo-cho, Chikusa-ku, Aichi, Nagoya, 464-8602, Japan
| | - Akira Nishio
- Nagoya University, Furo-cho, Chikusa-ku, Aichi, Nagoya, 464-8602, Japan
| | - Andrey Alexandrov
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Naples, Italy
- Dipartimento di Fisica "E. Pancini", Università degli Studi di Napoli "Federico II", Naples, Italy
| | - Valerio Gentile
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Naples, Italy
- Dipartimento di Fisica "E. Pancini", Università degli Studi di Napoli "Federico II", Naples, Italy
| | - Antonio Iuliano
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Naples, Italy
- Dipartimento di Fisica "E. Pancini", Università degli Studi di Napoli "Federico II", Naples, Italy
| | - Giovanni De Lellis
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Naples, Italy
- Dipartimento di Fisica "E. Pancini", Università degli Studi di Napoli "Federico II", Naples, Italy
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5
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Tanaka HK. Cosmic coding and transfer for ultra high security near-field communications. iScience 2023; 26:105897. [PMID: 36718362 PMCID: PMC9883181 DOI: 10.1016/j.isci.2022.105897] [Citation(s) in RCA: 4] [Impact Index Per Article: 4.0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/04/2022] [Revised: 11/30/2022] [Accepted: 12/22/2022] [Indexed: 01/06/2023] Open
Abstract
By using true random number (TRN) generators, encoding with the highest security can be realized. However, a completely secure strategy to transfer these TRNs has not yet been devised. Quantum key distribution (QKD) has attempted to establish secure key distribution methodology of this kind; however, several quantum cracking strategies have been predicted and experimentally demonstrated. In this work, COSMOCAT was invented as a solution for next-generation ultrahigh security near-field communications. With COSMOCAT, TRNs are generated from naturally occurring and ubiquitous cosmic-ray muons and the generated cosmic keys are distributed by these muons with an unprecedented level of security. The successful results of this experiment indicate that our prototype and the new key-generation-and-distribution standard can be utilized for practical encoding and near-field data transfer at rates of 10-100 Mbps. It is anticipated that COSMOCAT will be one of key techniques for future high security, near-field communication management.
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Affiliation(s)
- Hiroyuki K.M. Tanaka
- University of Tokyo, Tokyo, Japan,International Virtual Muography Institute (VMI), Global, Tokyo, Japan,Corresponding author
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6
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Tanaka HKM, Gluyas J, Holma M, Joutsenvaara J, Kuusiniemi P, Leone G, Lo Presti D, Matsushima J, Oláh L, Steigerwald S, Thompson LF, Usoskin I, Poluianov S, Varga D, Yokota Y. Atmospheric muography for imaging and monitoring tropic cyclones. Sci Rep 2022; 12:16710. [PMID: 36202852 PMCID: PMC9537288 DOI: 10.1038/s41598-022-20039-4] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/05/2022] [Accepted: 09/07/2022] [Indexed: 12/04/2022] Open
Abstract
Large-scale solid bodies on Earth such as volcanoes and man-made pyramids have been visualized with solid earth muography, and the recently invented technique, acqueous muography, has already demonstrated its capability to visualize ocean tides and tsunami. In this work, atmospheric muography, a technique to visualize and monitor the vertical profile of tropic cyclones (TCs) is presented for the first time. The density distribution and time-dependent behavior of several TCs which had approached Kagoshima, Japan, has been investigated with muography. The resultant time-sequential images captured their warm cores, and their movements were consistent with the TC trails and barometric pressure variations observed at meteorological stations. By combining multidirectional muographic images with barometric data, we anticipate that muography will become a useful tool to monitor the three-dimensional density distribution of a targeted mesoscale convective system.
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Abstract
While satellite-based global navigation systems have become essential tools in our daily lives, their effectiveness is often hampered by the fact that the signals cannot be accessed in underground, indoor, or underwater environments. Recently, a novel navigation system has been invented to address this issue by utilizing the characteristics of the ubiquitous and highly penetrative cosmic-ray muons. This technique, muometric navigation, does not require active signal generation and enables positioning in the aforementioned environments within a reference coordinate defined by the three-dimensional positions of multiple detectors. In its first phase of development, these reference detectors had to be connected to the receivers via a wired configuration to guarantee precise time synchronization. This work describes more versatile, wireless muometric navigation system (MuWNS), which was designed in conjunction with a cost-effective, crystal-oscillator-based grandmaster clock and a performance evaluation is reported for shallow underground/indoor, deep underground and undersea environments. It was confirmed that MuWNS offers a navigation quality almost equivalent to aboveground GPS-based handheld navigation by determining the distance between the reference frame and the receivers within a precision range between 1 and 10 m.
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Abstract
Sub-hourly to seasonal and interannual oceanographic phenomena can be better understood with high special resolution and high frequency tidal observations. However, while current tidal measurements can provide sufficiently high observational density in terms of time, the observational density in terms of space is low mainly due to the high expense of constructing tide gauge stations. In this work, we designed a novel tide monitoring technique with muography that could be operated in near-shore basements (or similar structures on land below sea level) and found that more practical, stable, robust and cost-effective high-spatiotemporal-density tide measurements are possible. Although the time resolution, sensitivity, and the distance between the detectors and the shorelines are tradeoffs, hourly and annual sensitivity (ability to detect the tide height variations) of less than 10 cm and 1 mm can be statistically attained, respectively. It is anticipated that the current muographic technique could be applied as an alternative, cost-effective and convenient dense tidal monitor network strategy in coastal areas worldwide.
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9
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Periodic sea-level oscillation in Tokyo Bay detected with the Tokyo-Bay seafloor hyper-kilometric submarine deep detector (TS-HKMSDD). Sci Rep 2022; 12:6097. [PMID: 35414679 PMCID: PMC9005544 DOI: 10.1038/s41598-022-10078-2] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/11/2021] [Accepted: 03/23/2022] [Indexed: 11/26/2022] Open
Abstract
Meteorological-tsunami-like (or meteotsunami-like) periodic oscillation was muographically detected with the Tokyo-Bay Seafloor Hyper-Kilometric Submarine Deep Detector (TS-HKMSDD) deployed in the underwater highway called the Trans-Tokyo Bay Expressway or Tokyo Bay Aqua-Line (TBAL). It was detected right after the arrival of the 2021 Typhoon-16 that passed through the region 400 km south of the bay. The measured oscillation period and decay time were respectively 3 h and 10 h. These measurements were found to be consistent with previous tide gauge measurements. Meteotsunamis are known to take place in bays and lakes, and the temporal and spatial characteristics of meteotsunamis are similar to seismic tsunamis. However, their generation and propagation mechanisms are not well understood. The current result indicates that a combination of muography and trans-bay or trans-lake underwater tunnels will offer an additional tool to measure meteotsunamis at locations where tide gauges are unavailable.
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10
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Miyadera H, Morris CL. Muon scattering tomography: review. APPLIED OPTICS 2022; 61:C154-C161. [PMID: 35201040 DOI: 10.1364/ao.445806] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/15/2021] [Accepted: 01/13/2022] [Indexed: 06/14/2023]
Abstract
Cosmic-ray muon scattering tomography has gathered attention in the security and nuclear industries in the last 10 years. Muon scattering tomography is capable of identifying atomic numbers of objects, is highly sensitivity to high-atomic-number materials such as uranium, and is very useful for detecting them in a background of low-atomic-number material. The principle, detectors, and applications of muon tomography are presented, as well as its future aspect.
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11
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Cimmino L. Principles and Perspectives of Radiographic Imaging with Muons. J Imaging 2021; 7:253. [PMID: 34940720 PMCID: PMC8708377 DOI: 10.3390/jimaging7120253] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/18/2021] [Revised: 11/22/2021] [Accepted: 11/25/2021] [Indexed: 11/16/2022] Open
Abstract
Radiographic imaging with muons, also called Muography, is based on the measurement of the absorption of muons, generated by the interaction of cosmic rays with the earth's atmosphere, in matter. Muons are elementary particles with high penetrating power, a characteristic that makes them capable of crossing bodies of dimensions of the order of hundreds of meters. The interior of bodies the size of a pyramid or a volcano can be seen directly with the use of this technique, which can rely on highly segmented muon trackers. Since the muon flux is distributed in energy over a wide spectrum that depends on the direction of incidence, the main difference with radiography made with X-rays is in the source. The source of muons is not tunable, neither in energy nor in direction; to improve the signal-to-noise ratio, muography requires large instrumentation, long time data acquisition and high background rejection capacity. Here, we present the principles of the Muography, illustrating how radiographic images can be obtained, starting from the measurement of the attenuation of the muon flux through an object. It will then be discussed how recent technologies regarding artificial intelligence can give an impulse to this methodology in order to improve its results.
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Affiliation(s)
- Luigi Cimmino
- Department of Physics, University of Naples Federico II, 80126 Napoli, Italy;
- Division of Naples, Italian National Institute for Nuclear Physics, 80126 Roma, Italy
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12
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First results of undersea muography with the Tokyo-Bay Seafloor Hyper-Kilometric Submarine Deep Detector. Sci Rep 2021; 11:19485. [PMID: 34593861 PMCID: PMC8484265 DOI: 10.1038/s41598-021-98559-8] [Citation(s) in RCA: 8] [Impact Index Per Article: 2.7] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/20/2021] [Accepted: 09/03/2021] [Indexed: 02/08/2023] Open
Abstract
Tidal measurements are of great significance since they may provide us with essential data to apply towards protection of coastal communities and sea traffic. Currently, tide gauge stations and laser altimetry are commonly used for these measurements. On the other hand, muography sensors can be located underneath the seafloor inside an undersea tunnel where electric and telecommunication infrastructures are more readily available. In this work, the world's first under-seafloor particle detector array called the Tokyo-bay Seafloor Hyper-Kilometric Submarine Deep Detector (TS-HKMSDD) was deployed underneath the Tokyo-Bay seafloor for conducting submarine muography. The resultant 80-day consecutive time-sequential muographic data were converted to the tidal levels based on the parameters determined from the first-day astronomical tide height (ATH) data. The standard deviation between ATH and muographic results for the rest of a 79-day measurement period was 12.85 cm. We anticipate that if the length of the TS-HKMSDD is extended from 100 m to a full-scale as large as 9.6 km to provide continuous tidal information along the tunnel, this muography application will become an established standard, demonstrating its effectiveness as practical tide monitor for this heavy traffic waterway in Tokyo and in other important sea traffic areas worldwide.
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13
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Cimmino L, Ambrosino F, Anastasio A, D'Errico M, Masone V, Roscilli L, Saracino G. A new cylindrical borehole detector for radiographic imaging with muons. Sci Rep 2021; 11:17425. [PMID: 34465834 PMCID: PMC8408154 DOI: 10.1038/s41598-021-96247-1] [Citation(s) in RCA: 4] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/27/2021] [Accepted: 08/05/2021] [Indexed: 11/20/2022] Open
Abstract
Muon radiography is a methodology which enables measuring the mass distribution within large objects. It exploits the abundant flux of cosmic muons and uses detectors with different technologies depending on the application. As the sensitive surface and geometric acceptance are two fundamental parameters for increasing the collection of muons, the optimization of the detectors is very significant. Here we show a potentially innovative detector of size and shape suitable to be inserted inside a borehole, that optimizes the sensitive area and maximizes the angular acceptance thanks to its cylindrical geometry obtained using plastic arc-shaped scintillators. Good spatial resolution is obtained with a reasonable number of channels. The dimensions of the detector make it ideal for use in 25 cm diameter wells. Detailed simulations based on Monte Carlo methods show great cavity detection capability. The detector has been tested in the laboratory, achieving overall excellent performance.
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Affiliation(s)
- L Cimmino
- Department of Physics, University of Naples "Federico II", Naples , Italy.
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Naples, Italy.
| | - F Ambrosino
- Department of Physics, University of Naples "Federico II", Naples , Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Naples, Italy
| | - A Anastasio
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Naples, Italy
| | - M D'Errico
- Department of Physics, University of Naples "Federico II", Naples , Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Naples, Italy
| | - V Masone
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Naples, Italy
| | - L Roscilli
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Naples, Italy
| | - G Saracino
- Department of Physics, University of Naples "Federico II", Naples , Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Naples, Italy
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14
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Tanaka HKM. Muometric positioning system (μPS) with cosmic muons as a new underwater and underground positioning technique. Sci Rep 2020; 10:18896. [PMID: 33144620 PMCID: PMC7609578 DOI: 10.1038/s41598-020-75843-7] [Citation(s) in RCA: 10] [Impact Index Per Article: 2.5] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/03/2019] [Accepted: 10/13/2020] [Indexed: 11/21/2022] Open
Abstract
Thus far, underwater and underground positioning techniques have been limited to those using classical waves (sound waves, electromagnetic waves or their combination). However, the positioning accuracy is strongly affected by the conditions of media they propagate (temperature, salinity, density, elastic constants, opacity, etc.). In this work, we developed a precise and entirely new three-dimensional positioning technique with cosmic muons. This muonic technique is totally unaffected by the media condition and can be universally implemented anywhere on the globe without a signal transmitter. Results of our laboratory-based experiments and simulations showed that, for example, plate-tectonics-driven seafloor motion and magma-driven seamount deformation can be detected with the μPS.
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Affiliation(s)
- Hiroyuki K M Tanaka
- Earthquake Research Institute, The University of Tokyo, 1-1-1 Yayoi, Bunkyo, Tokyo, 113-0032, Japan. .,International Muography Research Organization (MUOGRAPHIX), The University of Tokyo, 1-1-1 Yayoi, Bunkyo, Tokyo, 113-0032, Japan.
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15
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Proof-of-Principle of a Cherenkov-Tag Detector Prototype. SENSORS 2020; 20:s20123437. [PMID: 32570725 PMCID: PMC7349058 DOI: 10.3390/s20123437] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Subscribe] [Scholar Register] [Received: 05/21/2020] [Revised: 06/13/2020] [Accepted: 06/16/2020] [Indexed: 11/17/2022]
Abstract
In a recent paper, the authors discussed the feasibility study of an innovative technique based on the directionality of Cherenkov light produced in a transparent material to improve the signal to noise ratio in muon imaging applications. In particular, the method was proposed to help in the correct identification of incoming muons direction. After the first study by means of Monte Carlo simulations with Geant4, the first reduced scale prototype of such a detector was built and tested at the Department of Physics and Astronomy "E. Majorana" of the University of Catania (Italy). The characterization technique is based on muon tracking by means of the prototype in coincidence with two scintillating tiles. The results of this preliminary test confirm the validity of the technique and stressed the importance to enhance the Cherenkov photons production to get a signal well distinguishable with respect to sensors and electronic noise.
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16
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Lo Presti D, Gallo G, Bonanno DL, Bongiovanni DG, Longhitano F, Reito S. Feasibility Study of a New Cherenkov Detector for Improving Volcano Muography. SENSORS 2019; 19:s19051183. [PMID: 30857136 PMCID: PMC6427707 DOI: 10.3390/s19051183] [Citation(s) in RCA: 8] [Impact Index Per Article: 1.6] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Subscribe] [Scholar Register] [Received: 01/18/2019] [Revised: 03/01/2019] [Accepted: 03/05/2019] [Indexed: 11/16/2022]
Abstract
Muography is an expanding technique for internal structure investigation of large volume object, such as pyramids, volcanoes and also underground cavities. It is based on the attenuation of muon flux through the target in a way similar to the attenuation of X-ray flux through the human body for standard radiography. Muon imaging have to face with high background level, especially compared with the tiny near horizontal muon flux. In this paper the authors propose an innovative technique based on the measurement of Cherenkov radiation by Silicon photo-multipliers arrays to be integrated in a standard telescope for muography applications. Its feasibility study was accomplished by means of Geant4 simulations for the measurement of the directionality of cosmic-ray muons. This technique could be particularly useful for the suppression of background noise due to back-scattered particles whose incoming direction is likely to be wrongly reconstructed. The results obtained during the validation study of the technique principle confirm the ability to distinguish the arrival direction of muons with an efficiency higher than 98% above 1 GeV. In addition, a preliminary study on the tracking performance of the presented technique was introduced.
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Affiliation(s)
- Domenico Lo Presti
- Department of Physics and Astronomy "E. Maiorana", University of Catania, Via S. Sofia 64, 95123 Catania, Italy.
- National Institute for Nuclear Physics (INFN), Sezione di Catania, Via S. Sofia 64, 95123 Catania, Italy.
| | - Giuseppe Gallo
- Department of Physics and Astronomy "E. Maiorana", University of Catania, Via S. Sofia 64, 95123 Catania, Italy.
- National Institute for Nuclear Physics (INFN), Laboratori Nazionali del Sud, Via S. Sofia 62, 95123 Catania, Italy.
| | - Danilo L Bonanno
- National Institute for Nuclear Physics (INFN), Sezione di Catania, Via S. Sofia 64, 95123 Catania, Italy.
| | - Daniele G Bongiovanni
- National Institute for Nuclear Physics (INFN), Laboratori Nazionali del Sud, Via S. Sofia 62, 95123 Catania, Italy.
| | - Fabio Longhitano
- National Institute for Nuclear Physics (INFN), Sezione di Catania, Via S. Sofia 64, 95123 Catania, Italy.
| | - Santo Reito
- National Institute for Nuclear Physics (INFN), Sezione di Catania, Via S. Sofia 64, 95123 Catania, Italy.
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17
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Hussein EM. Imaging with naturally occurring radiation. Appl Radiat Isot 2019; 145:223-239. [DOI: 10.1016/j.apradiso.2018.12.006] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/22/2018] [Revised: 10/30/2018] [Accepted: 12/04/2018] [Indexed: 10/27/2022]
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18
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Abstract
Muography (or muon radiography) is a technique that exploits the penetration capability of muons, elementary particles similar to electrons but with a mass about 200 times larger. High energy muons are naturally produced in the interactions of cosmic rays with the Earth atmosphere. The measurement of their absorption in matter allows the imaging of the inner structure of large bodies. The technological developments in the detection of elementary particles have opened the way to its application in various fields, such as archaeology, studies of geological structures, civil engineering and security issues. We have developed a new approach to the three-dimensional muography of underground structures, capable of directly localising hidden cavities and of reconstructing their shape in space. Our measurements at Mt. Echia, the site of the earliest settlement of the city of Naples in the 8th century BC, have led us to the discovery of a hidden underground cavity, whose existence was not evident with the usual two-dimensional muography graphs. We demonstrate here that our original approach definitely enhances muography discovery potential, especially in case of complex underground systems.
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19
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Muon Radiography of Ancient Mines: The San Silvestro Archaeo-Mining Park (Campiglia Marittima, Tuscany). UNIVERSE 2019. [DOI: 10.3390/universe5010034] [Citation(s) in RCA: 11] [Impact Index Per Article: 2.2] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
Abstract
Muon absorption radiography is an imaging technique based on the measurement of the absorption of cosmic ray muons. This technique has recently been used successfully to investigate the presence of unknown cavities in the Bourbon Gallery in Naples and in the Chephren Pyramid at Cairo. The MIMA detector (Muon Imaging for Mining and Archaeology) is a prototype muon tracker for muon radiography for application in the fields of archaelogy and mining. It is made of three pairs of X-Y planes each consisting of 21 scintillator bars with a silicon photomultiplier readout. The detector is compact, robust, easily transportable, and has a low power consumption: all of which makes the detector ideal for measurements in confined and isolated environments. With this detector, a measurement from inside the Temperino mine in the San Silvestro archaeo-mining park in Tuscany was performed. The park includes about 25 km of mining tunnels arranged on several levels that have been exploited from the Etruscan time. The measured muon absorption was compared to the simulated one, obtained from the information provided by 3D laser scanner measurements and cartographic maps of the mountain above the mine, in order to obtain information about the average density of the rock. This allowed one to confirm the presence of a partially accessible exploitation opening and provided some hints regarding the presence of a high-density body within the rock.
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20
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Saracino G, Ambrosino F, Bonechi L, Cimmino L, D'Alessandro R, D'Errico M, Noli P, Scognamiglio L, Strolin P. Applications of muon absorption radiography to the fields of archaeology and civil engineering. PHILOSOPHICAL TRANSACTIONS. SERIES A, MATHEMATICAL, PHYSICAL, AND ENGINEERING SCIENCES 2018; 377:rsta.2018.0057. [PMID: 30530534 PMCID: PMC6335300 DOI: 10.1098/rsta.2018.0057] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Accepted: 10/12/2018] [Indexed: 06/09/2023]
Abstract
Muon radiography, also known as muography, is an imaging technique that provides information on the mass density distribution inside large objects. Muons are naturally produced in the interactions of cosmic rays in the Earth's atmosphere. The physical process exploited by muography is the attenuation of the muon flux, that depends on the thickness and density of matter that muons cross in the course of their trajectory. A particle detector with tracking capability allows the measurement of the muons flux as a function of the muon direction. The comparison of the measured muon flux with the expected one gives information on the distribution of the density of matter, in particular, on the presence of cavities. In this article, the measurement performed at Mt. Echia in Naples (Saracino 2017 Sci. Rep. 7, 1181. (doi:10.1038/s41598-017-01277-3)), will be discussed as a practical example of the possible application of muography in archaeology and civil engineering.This article is part of the Theo Murphy meeting issue 'Cosmic-ray muography'.
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Affiliation(s)
- G Saracino
- Università degli studi di Napoli Federico II, Naples, Italy
- INFN sezione di Napoli, Naples, Italy
| | - F Ambrosino
- Università degli studi di Napoli Federico II, Naples, Italy
- INFN sezione di Napoli, Naples, Italy
| | - L Bonechi
- INFN sezione di Firenze, Sesto Fiorentino, Italy
| | - L Cimmino
- INFN sezione di Napoli, Naples, Italy
| | - R D'Alessandro
- INFN sezione di Firenze, Sesto Fiorentino, Italy
- Università di Firenze, Sesto Fiorentino, Italy
| | | | - P Noli
- INFN sezione di Napoli, Naples, Italy
| | | | - P Strolin
- Università degli studi di Napoli Federico II, Naples, Italy
- INFN sezione di Napoli, Naples, Italy
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21
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Oláh L, Tanaka HKM, Hamar G, Varga D. Investigation of the limits of high-definition muography for observation of Mt Sakurajima. PHILOSOPHICAL TRANSACTIONS. SERIES A, MATHEMATICAL, PHYSICAL, AND ENGINEERING SCIENCES 2018; 377:20180135. [PMID: 30530543 PMCID: PMC6335296 DOI: 10.1098/rsta.2018.0135] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Accepted: 11/01/2018] [Indexed: 06/09/2023]
Abstract
A multi-wire proportional chamber-based muo- graphy observatory is under development for the monitoring of the internal structure of Mt Sakurajima in Kyushu, Japan. We investigated the limits of large-scale and high-definition muography. We adjusted the parameters of a modified Gaisser model and found that the spectral index of γ = - 2.64 and normalization factor of C = 0.66 reproduce more accurately the measured fluxes than the original parameters at large thickness. A thickness and zenith angle-dependent correction is suggested to the measured muon flux due to the energy cut which is introduced to suppress the background particles. The multiple scattering of muons was simulated across the standard rock and sea-level atmosphere up to the distance of 5 km. We found that multiple scattering decreases from 10 mrad to 4 mrad across the rock due to the decrease in the steepness of muon spectra. The multiple scattering falls down to about 2 mrad after the object in the atmosphere due to the increase in observed arrival zenith angles. The 2 m2 sized multi-wire proportional chamber-based Muographic Observation System (MMOS) was operating between February and June 2018. Three tracking systems operated reliably with tracking efficiencies of above 95%. The muon flux has been measured correctly down to 10-3 m-2 sr-1 s-1 The average density map of Mt Sakurajima has been measured with angular resolution of 12 mrad × 12 mrad (spatial resolution of 34 m × 34 m from the distance of 2.8 km). The average density values were found between 1.4 and 2 g cm-3, except at the crater regions where lower densities were observed.This article is part of the Theo Murphy meeting issue 'Cosmic-ray muography'.
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Affiliation(s)
- László Oláh
- Earthquake Research Institute, University of Tokyo, 1-1-1 Yayoi, Bunkyo, Tokyo 113-0032, Japan
| | - Hiroyuki K M Tanaka
- Earthquake Research Institute, University of Tokyo, 1-1-1 Yayoi, Bunkyo, Tokyo 113-0032, Japan
| | - Gergő Hamar
- Wigner Research Centre for Physics of the Hungarian Academy of Sciences, 29-33 Konkoly-Thege Miklós Str., Budapest H-1121, Hungary
| | - Dezső Varga
- Wigner Research Centre for Physics of the Hungarian Academy of Sciences, 29-33 Konkoly-Thege Miklós Str., Budapest H-1121, Hungary
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22
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Vanini S, Calvini P, Checchia P, Rigoni Garola A, Klinger J, Zumerle G, Bonomi G, Donzella A, Zenoni A. Muography of different structures using muon scattering and absorption algorithms. PHILOSOPHICAL TRANSACTIONS. SERIES A, MATHEMATICAL, PHYSICAL, AND ENGINEERING SCIENCES 2018; 377:20180051. [PMID: 30530531 PMCID: PMC6335307 DOI: 10.1098/rsta.2018.0051] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Accepted: 10/12/2018] [Indexed: 06/09/2023]
Abstract
In recent decades, muon imaging has found a plethora of applications in many fields. This technique succeeds to infer the density distribution of big inaccessible structures where conventional techniques cannot be used. The requirements of different applications demand specific implementations of image reconstruction algorithms for either multiple scattering or absorption-transmission data analysis, as well as noise-suppression filters and muon momentum estimators. This paper presents successful results of image reconstruction techniques applied to simulated data of some representative applications. In addition to well-known reconstruction methods, a novel approach, the so-called μCT, is proposed for the inspection of spent nuclear fuel canisters. Results obtained based on both μCT and the maximum-likelihood expectation maximization reconstruction algorithms are presented.This article is part of the Theo Murphy meeting issue 'Cosmic-ray muography'.
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Affiliation(s)
- S Vanini
- Department of Physics and Astronomy "Galileo Galilei", University of Padova, via Marzolo 8, 35131 Padova, Italy
| | - P Calvini
- Department of Physics, University of Genova, Via Dodecaneso 33, 16146 Genova, Italy
| | - P Checchia
- INFN Sezione di Padova, via Marzolo 8, 35131 Padova, Italy
| | - A Rigoni Garola
- CNR, Consorzio RFX, Corso Stati Uniti 4, 35127 Padova, Italy
| | - J Klinger
- INFN Sezione di Padova, via Marzolo 8, 35131 Padova, Italy
| | - G Zumerle
- Department of Physics and Astronomy "Galileo Galilei", University of Padova, via Marzolo 8, 35131 Padova, Italy
| | - G Bonomi
- Department DIMI, University of Brescia, via Branze 38, 25123 Brescia, Italy
| | - A Donzella
- Department DIMI, University of Brescia, via Branze 38, 25123 Brescia, Italy
| | - A Zenoni
- Department DIMI, University of Brescia, via Branze 38, 25123 Brescia, Italy
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23
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Wuyckens S, Giammanco A, Cortina Gil E, Demin P. A portable muon telescope based on small and gas-tight resistive plate chambers. PHILOSOPHICAL TRANSACTIONS. SERIES A, MATHEMATICAL, PHYSICAL, AND ENGINEERING SCIENCES 2018; 377:rsta.2018.0139. [PMID: 30530546 PMCID: PMC6335295 DOI: 10.1098/rsta.2018.0139] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Accepted: 10/09/2018] [Indexed: 06/09/2023]
Abstract
We report on the first steps in the development of a small-size muon telescope based on glass resistive plate chambers with small active area (16 × 16 cm2). The long-term goal of this project is to focus on applications of muography where the telescope may have to be operated underground and/or inside small rooms, and in challenging logistic situations. Driving principles in our design are therefore compact size, light weight, gas tightness and robustness. The first data-taking experiences have been encouraging, and we elaborate on the lessons learnt and future directions for development.This article is part of the Theo Murphy meeting issue 'Cosmic-ray muography'.
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Affiliation(s)
- Sophie Wuyckens
- Centre for Cosmology, Particle Physics and Phenomenology, Université catholique de Louvain, Louvain-la-Neuve 1348, Belgium
| | - Andrea Giammanco
- Centre for Cosmology, Particle Physics and Phenomenology, Université catholique de Louvain, Louvain-la-Neuve 1348, Belgium
| | - Eduardo Cortina Gil
- Centre for Cosmology, Particle Physics and Phenomenology, Université catholique de Louvain, Louvain-la-Neuve 1348, Belgium
| | - Pavel Demin
- Centre for Cosmology, Particle Physics and Phenomenology, Université catholique de Louvain, Louvain-la-Neuve 1348, Belgium
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24
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Yang G, Clarkson T, Gardner S, Ireland D, Kaiser R, Mahon D, Jebali RA, Shearer C, Ryan M. Novel muon imaging techniques. PHILOSOPHICAL TRANSACTIONS. SERIES A, MATHEMATICAL, PHYSICAL, AND ENGINEERING SCIENCES 2018; 377:rsta.2018.0062. [PMID: 30530538 PMCID: PMC6335303 DOI: 10.1098/rsta.2018.0062] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Accepted: 09/27/2018] [Indexed: 06/09/2023]
Abstract
Owing to the high penetrating power of high-energy cosmic ray muons, muon imaging techniques can be used to image large bulky objects, especially objects with heavy shielding. Muon imaging systems work just like CT scanners in the medical imaging field-that is, they can reveal information inside of a target. There are two forms of muon imaging techniques: muon absorption imaging and muon multiple scattering imaging. The former is based on the flux attenuation of muons, and the latter is based on the multiple scattering of muons in matter. The muon absorption imaging technique is capable of imaging very large objects such as volcanoes and large buildings, and also smaller objects like spent fuel casks; the muon multiple scattering imaging technique is best suited to inspect smaller objects such as nuclear waste containers. Muon imaging techniques can be applied in a broad variety of fields, i.e. from measuring the magma thickness of volcanoes to searching for secret cavities in pyramids, and from monitoring the borders of countries checking for special nuclear materials to monitoring the spent fuel casks for nuclear safeguards applications. In this paper, the principles of muon imaging are reviewed. Image reconstruction algorithms such as Filtered Back Projection and Maximum Likelihood Expectation Maximization are discussed. The capability of muon imaging techniques is demonstrated through a Geant4 simulation study for imaging a nuclear spent fuel cask.This article is part of the Theo Murphy meeting issue 'Cosmic-ray muography'.
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Affiliation(s)
- Guangliang Yang
- School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK
- Lynkeos Technology Ltd., University of Glasgow, Glasgow G12 8QQ, UK
| | - Tony Clarkson
- School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK
- Lynkeos Technology Ltd., University of Glasgow, Glasgow G12 8QQ, UK
| | - Simon Gardner
- School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK
- Lynkeos Technology Ltd., University of Glasgow, Glasgow G12 8QQ, UK
| | - David Ireland
- School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK
- Lynkeos Technology Ltd., University of Glasgow, Glasgow G12 8QQ, UK
| | - Ralf Kaiser
- School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK
- Lynkeos Technology Ltd., University of Glasgow, Glasgow G12 8QQ, UK
| | - David Mahon
- School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK
- Lynkeos Technology Ltd., University of Glasgow, Glasgow G12 8QQ, UK
| | - Ramsey Al Jebali
- School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK
- Lynkeos Technology Ltd., University of Glasgow, Glasgow G12 8QQ, UK
| | - Craig Shearer
- National Nuclear Laboratory, Central Laboratory, Sellafield, Seascale, Cumbria CA20 1PG, UK
| | - Matthew Ryan
- National Nuclear Laboratory, Central Laboratory, Sellafield, Seascale, Cumbria CA20 1PG, UK
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25
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Bonechi L, Baccani G, Bongi M, Brocchini D, Casagli N, Ciaranfi R, Cimmino L, Ciulli V, D'Alessandro R, Del Ventisette C, Dini A, Gigli G, Gonzi S, Guideri S, Lombardi L, Melon B, Mori N, Nocentini M, Noli P, Saracino G, Viliani L. Tests of a novel imaging algorithm to localize hidden objects or cavities with muon radiography. PHILOSOPHICAL TRANSACTIONS. SERIES A, MATHEMATICAL, PHYSICAL, AND ENGINEERING SCIENCES 2018; 377:rsta.2018.0063. [PMID: 30530539 PMCID: PMC6335299 DOI: 10.1098/rsta.2018.0063] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Accepted: 10/19/2018] [Indexed: 06/09/2023]
Abstract
A novel algorithm developed within muon radiography to localize objects or cavities hidden inside large material volumes was recently proposed by some of the authors (Bonechi et al. 2015 J. Instrum. 10, P02003 (doi:10.1088/1748-0221/10/02/P02003)). The algorithm, based on muon back projection, helps to estimate the three-dimensional position and the transverse extension of detected objects without the need for measurements from different points of view, which would be required to make a triangulation. This algorithm can now be tested owing to the availability of real data collected both in laboratory tests and from real-world measurements. The methodology and some test results are presented in this paper.This article is part of the Theo Murphy meeting issue 'Cosmic-ray muography'.
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Affiliation(s)
- L Bonechi
- INFN Firenze, Via B. Rossi 3, 50019 Sesto F.no (Firenze), Italy
- Università di Firenze, Dipartimento di Fisica e Astronomia, Via G. Sansone 1, 50019 Sesto F.no (Firenze), Italy
| | - G Baccani
- INFN Firenze, Via B. Rossi 3, 50019 Sesto F.no (Firenze), Italy
- Università di Firenze, Dipartimento di Fisica e Astronomia, Via G. Sansone 1, 50019 Sesto F.no (Firenze), Italy
| | - M Bongi
- INFN Firenze, Via B. Rossi 3, 50019 Sesto F.no (Firenze), Italy
- Università di Firenze, Dipartimento di Fisica e Astronomia, Via G. Sansone 1, 50019 Sesto F.no (Firenze), Italy
| | - D Brocchini
- Parchi Val di Cornia, Via Giovanni Lerario 90, 57025 Piombino (LI), Italy
| | - N Casagli
- Università di Firenze, Dipartimento di Scienze della Terra, Via La Pira 4, 50121 Firenze, Italy
| | - R Ciaranfi
- INFN Firenze, Via B. Rossi 3, 50019 Sesto F.no (Firenze), Italy
| | - L Cimmino
- Università di Napoli Federico II, Dipartimento di Fisica, Via Cinthia 21, 80126 Napoli, Italy
- INFN Napoli, Via Cinthia 21, 80126 Napoli, Italy
| | - V Ciulli
- INFN Firenze, Via B. Rossi 3, 50019 Sesto F.no (Firenze), Italy
- Università di Firenze, Dipartimento di Fisica e Astronomia, Via G. Sansone 1, 50019 Sesto F.no (Firenze), Italy
| | - R D'Alessandro
- INFN Firenze, Via B. Rossi 3, 50019 Sesto F.no (Firenze), Italy
- Università di Firenze, Dipartimento di Fisica e Astronomia, Via G. Sansone 1, 50019 Sesto F.no (Firenze), Italy
| | - C Del Ventisette
- Università di Firenze, Dipartimento di Scienze della Terra, Via La Pira 4, 50121 Firenze, Italy
| | - A Dini
- IGG-CNR, Via G. Moruzzi 1, 56124 Pisa, Italy
| | - G Gigli
- Università di Firenze, Dipartimento di Scienze della Terra, Via La Pira 4, 50121 Firenze, Italy
| | - S Gonzi
- INFN Firenze, Via B. Rossi 3, 50019 Sesto F.no (Firenze), Italy
- Università di Firenze, Dipartimento di Fisica e Astronomia, Via G. Sansone 1, 50019 Sesto F.no (Firenze), Italy
| | - S Guideri
- Parchi Val di Cornia, Via Giovanni Lerario 90, 57025 Piombino (LI), Italy
| | - L Lombardi
- Università di Firenze, Dipartimento di Scienze della Terra, Via La Pira 4, 50121 Firenze, Italy
| | - B Melon
- INFN Firenze, Via B. Rossi 3, 50019 Sesto F.no (Firenze), Italy
| | - N Mori
- INFN Firenze, Via B. Rossi 3, 50019 Sesto F.no (Firenze), Italy
- Università di Firenze, Dipartimento di Fisica e Astronomia, Via G. Sansone 1, 50019 Sesto F.no (Firenze), Italy
| | - M Nocentini
- Università di Firenze, Dipartimento di Scienze della Terra, Via La Pira 4, 50121 Firenze, Italy
| | - P Noli
- Università di Napoli Federico II, Dipartimento di Fisica, Via Cinthia 21, 80126 Napoli, Italy
- INFN Napoli, Via Cinthia 21, 80126 Napoli, Italy
| | - G Saracino
- Università di Napoli Federico II, Dipartimento di Fisica, Via Cinthia 21, 80126 Napoli, Italy
- INFN Napoli, Via Cinthia 21, 80126 Napoli, Italy
| | - L Viliani
- INFN Firenze, Via B. Rossi 3, 50019 Sesto F.no (Firenze), Italy
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26
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Bonechi L, Ambrosino F, Cimmino L, D'Alessandro R, Macedonio G, Melon B, Mori N, Noli P, Saracino G, Strolin P, Giudicepietro F, Martini M, Orazi M, Peluso R. The MURAVES project and other parallel activities on muon absorption radiography. EPJ WEB OF CONFERENCES 2018. [DOI: 10.1051/epjconf/201818202015] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
The MURAVES (MUon RAdiography of VESuvius) project is a joint activity participated by INGV, INFN and the Universities of Naples “Federico II” and Florence. The collaboration, following the experience gained within the previous INFN R&D project Mu-Ray, is currently completing the production of a robust four square meter low power consumption detector to be installed on the flank of Mount Vesuvius, an active volcano located on the western coast of Italy. The detector is supposed to collect data for at least one year, thus allowing performing a scan of the structure of the Vesuvius volcanic cone. In this work the status of the project and some parallel activities on muon radiography are presented.
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27
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Morishima K, Kuno M, Nishio A, Kitagawa N, Manabe Y, Moto M, Takasaki F, Fujii H, Satoh K, Kodama H, Hayashi K, Odaka S, Procureur S, Attié D, Bouteille S, Calvet D, Filosa C, Magnier P, Mandjavidze I, Riallot M, Marini B, Gable P, Date Y, Sugiura M, Elshayeb Y, Elnady T, Ezzy M, Guerriero E, Steiger V, Serikoff N, Mouret JB, Charlès B, Helal H, Tayoubi M. Discovery of a big void in Khufu's Pyramid by observation of cosmic-ray muons. Nature 2017; 552:386-390. [PMID: 29160306 DOI: 10.1038/nature24647] [Citation(s) in RCA: 190] [Impact Index Per Article: 27.1] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/12/2017] [Accepted: 10/24/2017] [Indexed: 11/09/2022]
Abstract
The Great Pyramid, or Khufu's Pyramid, was built on the Giza plateau in Egypt during the fourth dynasty by the pharaoh Khufu (Cheops), who reigned from 2509 bc to 2483 bc. Despite being one of the oldest and largest monuments on Earth, there is no consensus about how it was built. To understand its internal structure better, we imaged the pyramid using muons, which are by-products of cosmic rays that are only partially absorbed by stone. The resulting cosmic-ray muon radiography allows us to visualize the known and any unknown voids in the pyramid in a non-invasive way. Here we report the discovery of a large void (with a cross-section similar to that of the Grand Gallery and a minimum length of 30 metres) situated above the Grand Gallery. This constitutes the first major inner structure found in the Great Pyramid since the nineteenth century. The void, named ScanPyramids' Big Void, was first observed with nuclear emulsion films installed in the Queen's chamber, then confirmed with scintillator hodoscopes set up in the same chamber and finally re-confirmed with gas detectors outside the pyramid. This large void has therefore been detected with high confidence by three different muon detection technologies and three independent analyses. These results constitute a breakthrough for the understanding of the internal structure of Khufu's Pyramid. Although there is currently no information about the intended purpose of this void, these findings show how modern particle physics can shed new light on the world's archaeological heritage.
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Affiliation(s)
- Kunihiro Morishima
- F-lab, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8602, Japan
| | - Mitsuaki Kuno
- F-lab, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8602, Japan
| | - Akira Nishio
- F-lab, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8602, Japan
| | - Nobuko Kitagawa
- F-lab, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8602, Japan
| | - Yuta Manabe
- F-lab, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8602, Japan
| | - Masaki Moto
- F-lab, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8602, Japan
| | - Fumihiko Takasaki
- High Energy Accelerator Research Organization (KEK), 1-1 oho, Tsukuba, Ibaraki 305-0801, Japan
| | - Hirofumi Fujii
- High Energy Accelerator Research Organization (KEK), 1-1 oho, Tsukuba, Ibaraki 305-0801, Japan
| | - Kotaro Satoh
- High Energy Accelerator Research Organization (KEK), 1-1 oho, Tsukuba, Ibaraki 305-0801, Japan
| | - Hideyo Kodama
- High Energy Accelerator Research Organization (KEK), 1-1 oho, Tsukuba, Ibaraki 305-0801, Japan
| | - Kohei Hayashi
- High Energy Accelerator Research Organization (KEK), 1-1 oho, Tsukuba, Ibaraki 305-0801, Japan
| | - Shigeru Odaka
- High Energy Accelerator Research Organization (KEK), 1-1 oho, Tsukuba, Ibaraki 305-0801, Japan
| | - Sébastien Procureur
- Institut de Recherche sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris Saclay, 91191 Gif-sur-Yvette, France
| | - David Attié
- Institut de Recherche sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris Saclay, 91191 Gif-sur-Yvette, France
| | - Simon Bouteille
- Institut de Recherche sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris Saclay, 91191 Gif-sur-Yvette, France
| | - Denis Calvet
- Institut de Recherche sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris Saclay, 91191 Gif-sur-Yvette, France
| | - Christopher Filosa
- Institut de Recherche sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris Saclay, 91191 Gif-sur-Yvette, France
| | - Patrick Magnier
- Institut de Recherche sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris Saclay, 91191 Gif-sur-Yvette, France
| | - Irakli Mandjavidze
- Institut de Recherche sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris Saclay, 91191 Gif-sur-Yvette, France
| | - Marc Riallot
- Institut de Recherche sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'Energie Atomique et aux Energies Alternatives (CEA), Université Paris Saclay, 91191 Gif-sur-Yvette, France
| | | | - Pierre Gable
- Emissive, 71 rue de Provence, 75009 Paris, France
| | - Yoshikatsu Date
- NHK Enterprises, Inc. (NEP), 4-14 Kamiyama-cho, Shibuya-ku, Tokyo 150-0047, Japan
| | - Makiko Sugiura
- Suave Images, N-2 Maison de Shino, 3-30-8 Kamineguro, Meguro-Ku, Tokyo 153-0051, Japan
| | - Yasser Elshayeb
- Cairo University, 9 Al Gameya, Oula, Giza Governorate, Egypt
| | - Tamer Elnady
- Ain Shams University, Kasr el-Zaafaran, Abbasiya, Cairo, Egypt
| | - Mustapha Ezzy
- Cairo University, 9 Al Gameya, Oula, Giza Governorate, Egypt
| | | | | | | | - Jean-Baptiste Mouret
- Inria, Villers-lès-Nancy F-54600, France.,CNRS, Vandœuvre-lès-Nancy F-54500, France.,Université de Lorraine, Vandœuvre-lès-Nancy F-54500, France
| | - Bernard Charlès
- Dassault Systèmes, 10 Rue Marcel Dassault, 78140 Vélizy-Villacoublay, France
| | - Hany Helal
- HIP Institute, 50 rue de Rome, 75008 Paris, France.,Cairo University, 9 Al Gameya, Oula, Giza Governorate, Egypt
| | - Mehdi Tayoubi
- HIP Institute, 50 rue de Rome, 75008 Paris, France.,Dassault Systèmes, 10 Rue Marcel Dassault, 78140 Vélizy-Villacoublay, France
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