A mobile detector for measurements of the atmospheric muon flux in underground sites

• Published in: Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment Accelerators, spectrometers, detectors and associated equipment, 2011-10, Vol.654 (1), p.176-183
• Main Authors: Mitrica, Bogdan, Margineanu, Romul, Stoica, Sabin, Petcu, Mirel, Brancus, Iliana, Jipa, Alexandru, Lazanu, Ionel, Sima, Octavian, Haungs, Andreas, Rebel, Heinigerd, Petre, Marian, Toma, Gabriel, Saftoiu, Alexandra, Stanca, Denis, Apostu, Ana, Gomoiu, Claudia
• Format: Article
• Language: English
• Subjects: Detectors; Dosage; Equivalence; Flux; Measuring instruments; Meters; Mobile detector; Monte–Carlo simulation; Muon; Muons; Underground
• ISSN: 0168-9002; 1872-9576
• DOI: 10.1016/j.nima.2011.07.006

Muons comprise an important contribution of the natural radiation dose in air (approx. 30 nSv/h of a total dose rate of 65–130 nSv/h), as well as in underground sites even when the flux and relative contribution are significantly reduced. The flux of muons observed underground can be used as an estimator for the depth in mwe (meter water equivalent) of the underground site. The water equivalent depth is important information to devise physics experiments feasible for a specific site. A mobile detector for performing measurements of the muon flux was developed in IFIN-HH, Bucharest. Consisting of two scintillator plates (approx. 0.9 m 2) which measure in coincidence, the detector is installed on a van which facilitates measurements at different locations at the surface or underground. The detector was used to determine muon fluxes at different sites in Romania. In particular, data were taken and the values of meter water equivalents were assessed for several locations at the salt mine in Slanic-Prahova, Romania. The measurements have been performed in two different galleries of the Slanic mine at different depths. In order to test the stability of the method, also measurements of the muon flux at the surface at different elevations were performed. The results were compared with predictions of Monte–Carlo simulations using the CORSIKA and MUSIC codes.