1Earthquake Research Institute, The University of Tokyo, Tokyo, Japan
2Department of Physics, Graduate School of Science, Nagoya University, Nagoya, Japan
Received: 13 Nov 2013 – Discussion started: 04 Dec 2013
Abstract. The aim of this study is to ascertain and confirm the source of background noise in cosmic-ray muon radiography (muography) using emulsion film detectors. For this, we build two types of emulsion detectors with different momentum thresholds and perform test measurements of an actual geoscientific target. This experiment reveals that contamination of nonsignal particles with momenta of less than 2 GeV c−1 cause significant systematic errors for the density estimation of muography. Utilizing the results of precedent studies, we conclude that the origin of these low-momentum particles is either electromagnetic components of air showers or cosmic-ray muons scattered in topographic material. In this paper, we analyze the emulsion data in detail, including the film-inefficiency compensation and momentum selection by applying an upper bound to the chi-square distribution for the data.
Revised: 22 Mar 2014 – Accepted: 28 Mar 2014 – Published: 16 Apr 2014
Nishiyama, R., Miyamoto, S., and Naganawa, N.: Experimental study of source of background noise in muon radiography using emulsion film detectors, Geosci. Instrum. Method. Data Syst., 3, 29-39, doi:10.5194/gi-3-29-2014, 2014.