NS005
Cosmic-Ray Muon Imaging: Methodological Advances and Applications
Cosmic-Ray Muon Imaging: Methodological Advances and Applications
Session ID#: 77725
Session Description:
Cosmic-ray muon imaging or muography uses the natural flux of elementary particles called muons to characterize the density structure of geological bodies. Density is estimated by comparing muon fluxes before and after traversing the body, in a similar way to X-ray radiography. Density changes in time can also be estimated by continuously measuring the muon flux with a fixed muon detector. This technique offers new opportunities to study targets ranging from large bodies such as volcanoes or geological structures above deep tunnels; to meter-scale ore bodies and archeological structures.
We seek to further advance this method by bringing together methodological and numerical studies, data processing techniques, instrumentation developments, and case studies. We particularly welcome studies combining muon imaging with other geophysical methods or data constraints, aiming for an improved characterization and understanding of the subsurface.
Index Terms:
0910 Data processing [EXPLORATION GEOPHYSICS]
0933 Remote sensing [EXPLORATION GEOPHYSICS]
0994 Instruments and techniques [EXPLORATION GEOPHYSICS]
8494 Instruments and techniques [VOLCANOLOGY]
Primary Convener: Marina Rosas-Carbajal, Institut de Physique du Globe de Paris, Paris, France
Conveners: Giovanni Macedonio, Istituto Nazionale di Geofisica e Vulcanologia, Napoli, Italy, Jacques Marteau, IPNL, Lyon, France and Simon Bouteille, IRIS Instruments, Orleans Cedex 2, France
Primary Liaison: Marina Rosas-Carbajal, Institut de Physique du Globe de Paris, Paris, France
See more of: Near Surface Geophysics
