Cosmic ray muon radiography can measure the density distribution within a volcano. Unidirectional radiography shows a precise cross-sectional view of a conduit and a magma body through a volcano parallel to the plane of the detector. However, it only resolves the average density distribution along individual muon paths. Precise size and shape of underground structure, such as a conduit or a magma body, provide clear and pervasive information on understanding dynamics of volcanic eruption. Here we show a highly resolved three-dimensional tomographic image of an active volcano Asama in Japan. Specifically, we developed a portable power-effective muon radiography telescope that can be operated stable with a realistically sized solar panel so as to place it around an active volcano where commercial electric power is not available. The resulting image below the crater floor shows that a local low-density region accumulates sufficient gas pressure to cause Vulcanian eruption. The present muon computational axial tomography scan has a resolving power with a resolution of 100 m, allowing it to see great detail in volcanoes. Copyright 2010 by the American Geophysical Union.
CITATION STYLE
Tanaka, H. K. M., Taira, H., Uchida, T., Tanaka, M., Takeo, M., Ohminato, T., … Tsuiji, H. (2010). Three-dimensional computational axial tomography scan of a volcano with cosmic ray muon radiography. Journal of Geophysical Research: Solid Earth, 115(12). https://doi.org/10.1029/2010JB007677
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