Item talk:Q269614
From geokb
{
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"@type": "Article",
"additionalType": "Journal Article",
"name": "Local earthquake Vp and Vs tomography in the Mount St. Helens region with the iMUSH broadband array",
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"value": "10.1029/2019GC008888",
"url": "https://doi.org/10.1029/2019GC008888"
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"journal": {
"@type": "Periodical",
"name": "Geochemistry, Geophysics, Geosystems",
"volumeNumber": "21",
"issueNumber": "3"
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"inLanguage": "en",
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"datePublished": "2020",
"dateModified": "2023-10-03",
"abstract": "We present new 3-D\u00a0P\u00a0wave and\u00a0S\u00a0wave velocity models of the upper 20 km of the Mount St. Helens (MSH) region. These were obtained using local-source arrival time tomography from earthquakes and explosions recorded at 70 broadband stations deployed as part of the imaging Magma Under St. Helens (iMUSH) project and augmented by several data sets. Principal features of our models include (1) low\u00a0P\u00a0wave and\u00a0S\u00a0wave velocities along the St. Helens seismic zone to depths of at least 20 km corresponding to high conductivity imaged by iMUSH magnetotelluric studies. This delineates a zone of weakness that magma can exploit at the location of MSH; (2) a 5- to 7-km diameter, 6\u201315 km deep, 3\u20136% negative\u00a0P\u00a0wave and\u00a0S\u00a0wave velocity anomaly beneath MSH, consistent with previous estimates of the source region for recent eruptions. We interpret this as a magma storage region containing up to 15\u201320 km3\u00a0of partial melt, which is about 5 times more than the largest documented eruption at MSH; (3) a broad region of low\u00a0P\u00a0wave velocity below 10-km depth extending between Mount Adams and Mount Rainier along and to the east of the main Cascade arc, which is likely due to high-temperature arc crust and possible presence of fluids or melt; (4) several anomalies associated with surface-mapped features, including high-velocity igneous units such as the Spud Mountain and Spirit Lake plutons and low velocities in the Chehalis sedimentary basin and the Indian Heaven volcanic field. Our results place further constraints on the geometry of these features at depth.",
"description": "e2019GC008888, 19 p.",
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"name": "American Geophysical Union"
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"name": "Ulberg, Carl W",
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"name": "University of Washington"
}
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"name": "Creager, Kenneth C",
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"name": "University of Washington"
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"name": "Moran, Seth C. smoran@usgs.gov",
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"name": "Cornell University"
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"name": "Kiser, Eric",
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"name": "Department of Earth & Planetary Sciences, Harvard University, Cambridge, MA"
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"name": "University of New Mexico"
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"name": "University of New Mexico"
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