A portable muon telescope for exploration geophysics in confined environments

Author(s):  
Marwa Moussawi ◽  
Samip Basnet ◽  
Eduardo Cortina Gil ◽  
Pavel Demin ◽  
Ran M. I. D. Gamage ◽  
...  
Keyword(s):  
2007 ◽  
Vol 25 ◽  
pp. 163-167 ◽  
Author(s):  
Marlos Rockenbach da Silva ◽  
Walter Demetrio Gonzalez Alarcon ◽  
Ezequiel Echer ◽  
Alisson Dal Lago ◽  
Luis Eduardo Antunes Vieira ◽  
...  

2019 ◽  
Author(s):  
Sindulfo Ayuso ◽  
José Ignacio García Tejedor ◽  
Juan Jose Blanco ◽  
Raúl Gómez Herrero ◽  
Oścar García Población ◽  
...  
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2020 ◽  
Vol 63 (6) ◽  
pp. 860-863
Author(s):  
Yu. V. Balabin ◽  
B. B. Gvozdevsky ◽  
A. V. Germanenko ◽  
E. A. Mikhalko ◽  
E. A. Maurchev ◽  
...  
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2019 ◽  
Vol 83 (5) ◽  
pp. 547-550
Author(s):  
V. G. Grigoryev ◽  
P. Yu. Gololobov ◽  
P. A. Krivoshapkin ◽  
G. F. Krymsky ◽  
V. G. Yanke
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1994 ◽  
Vol 11 (2) ◽  
pp. 170-174 ◽  
Author(s):  
D. L. Hall ◽  
J. E. Humble ◽  
M. L. Duldig

AbstractWe have deduced the yearly averaged value of the solar diurnal variation as observed by a surface muon telescope and three underground muon telescopes over the years 1957 to 1985. This has allowed us to examine the temporal variation in both the latitudinal gradient Gz and the product of the parallel mean free path and the radial gradient of galactic cosmic rays during three consecutive solar cycles. The median rigidities of the primary particles being detected by the telescopes are 50 GV in the case of the surface muon telescope and greater than 150 GV in the case of the underground muon telescopes. We have compared our results with those of a similar study made from observations of the solar diurnal variation by neutron monitors and an ion chamber, which have median rigidities of response between 17 and 70 GV (Bieber and Chen 1991a). The product has a solar magnetic cycle dependence and our values are lower than those observed by neutron monitors, in agreement with the Bieber and Chen observation that reverses after a solar magnetic field reversal, in accordance with drift theories.


2009 ◽  
Vol 36 (9) ◽  
pp. 095001 ◽  
Author(s):  
L Ruan ◽  
G Lin ◽  
Z Xu ◽  
K Asselta ◽  
H F Chen ◽  
...  
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2011 ◽  
Vol 85 (6) ◽  
pp. 891-896
Author(s):  
L. Ruan ◽  
V. Ames
Keyword(s):  

2020 ◽  
Author(s):  
Simon Bouteille ◽  
Adnand Bitri ◽  
Michel Dietz ◽  
Julien Gance

<p>Absorption muon imaging is a technique that can measure density variations underground down to a few hundred meters. Then, it can prove to be useful in a mining environment: to help assess the ore bodies volumes and/or to monitor the underground for natural hazards that can happen at the surface because of the mining exploitation. Here we report the result of an experiment designed to test the capabilities and resolution power of a cosmic muon measurement in a mining environment compared to other standard geophysics tools: gravimetry and seismic studies. It consists of three independent measurement of a subset of the decommissioned iron mine of May-sur-Orne (France). The first one was made using a 50x50cm² micromegas based muon telescope installed at the deepest non-submerged level (50m underground) during 3 months. The second one is a gravimetry survey of the surface area inside the muon telescope acceptance cone. And the third one is a study of refracted and reflected seismic waves along a single line above the muon telescope location. The investigation volume was chosen because of the presence of surface risks (neighborhood), the unknown of some uncharted volume and the presence of an ore storage volume of several meter cubed that was used during the mine exploitation and which filling state is unknown.</p><p>The data analysis showed that while muon tomography is able to detect the negative density anomaly of the storage volume, the gravimetry measurement is not sensible to it. However, the seismic study was able to detect the volume as well and its location and extension is compatible with the muon measurement.</p>


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