Shallow resistivity structure around the 2018 craters of Mt. Motoshirane of Kusatsu-Shirane Volcano, Japan, revealed by audio-frequency magnetotellurics

Bibliographic Details
Title: Shallow resistivity structure around the 2018 craters of Mt. Motoshirane of Kusatsu-Shirane Volcano, Japan, revealed by audio-frequency magnetotellurics
Authors: Asami Honda, Wataru Kanda, Takao Koyama, Shinichi Takakura, Yasuo Matsunaga, Tatsuji Nishizawa, Satoshi Ikezawa
Source: Earth, Planets and Space, Vol 75, Iss 1, Pp 1-15 (2023)
Publisher Information: SpringerOpen, 2023.
Publication Year: 2023
Collection: LCC:Geography. Anthropology. Recreation
LCC:Geodesy
LCC:Geology
Subject Terms: Mt. Motoshirane, Phreatic eruption, Audio-frequency magnetotellurics, Resistivity structure, Hydrothermal system, Geography. Anthropology. Recreation, Geodesy, QB275-343, Geology, QE1-996.5
More Details: Abstract In 2018, a phreatic eruption occurred at Mt. Motoshirane, a pyroclastic cone group of the Kusatsu-Shirane Volcano in central Japan. The eruption was abrupt, and no signs of volcanic activity have been observed in recent years, in contrast to the other major pyroclastic cone group, Mt. Shirane, which hosts the active crater lake and has endured repeated phreatic eruptions. To understand the mechanism of the eruption at Mt. Motoshirane, information on the shallow hydrothermal system, which is thought to be the source region of phreatic eruptions, is required; however, few studies have been conducted on this particular cone group. In this study, we conducted an audio-frequency magnetotelluric survey in 2020 to reveal the shallow resistivity structure around the 2018 craters. A three-dimensional resistivity structure model showed generally two layers, with high resistivities at shallow depths overlain by low resistivities underneath. The boundary between the layers corresponded to the top boundary of the Neogene basement rocks. These low resistivities were not found beneath the 2018 craters; therefore, part of the Neogene basement rocks could have been lost by the eruption beneath the 2018 craters. This is consistent with the geochemical study on the mineral assemblage of the erupted deposits, which suggested that the explosions reached the depth of the basement. Graphical Abstract
Document Type: article
File Description: electronic resource
Language: English
ISSN: 1880-5981
Relation: https://doaj.org/toc/1880-5981
DOI: 10.1186/s40623-023-01799-3
Access URL: https://doaj.org/article/dd23ea6381944fc197ca039557a31a19
Accession Number: edsdoj.23ea6381944fc197ca039557a31a19
Database: Directory of Open Access Journals
More Details
ISSN:18805981
DOI:10.1186/s40623-023-01799-3
Published in:Earth, Planets and Space
Language:English