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Shear wave anisotropy beneath the volcanic front in South Kyushu area, Japan: Development of C-type olivine CPO under H2O-rich conditions
https://doi.org/10.24517/00011083
https://doi.org/10.24517/00011083d040875c-bc49-4f16-b2ac-9c0b5d8c6a5f
名前 / ファイル | ライセンス | アクション |
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Item type | 学術雑誌論文 / Journal Article(1) | |||||||||
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公開日 | 2017-10-03 | |||||||||
タイトル | ||||||||||
タイトル | Shear wave anisotropy beneath the volcanic front in South Kyushu area, Japan: Development of C-type olivine CPO under H2O-rich conditions | |||||||||
言語 | ||||||||||
言語 | eng | |||||||||
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資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||||||
資源タイプ | journal article | |||||||||
ID登録 | ||||||||||
ID登録 | 10.24517/00011083 | |||||||||
ID登録タイプ | JaLC | |||||||||
著者 |
Terada, Tadashi
× Terada, Tadashi× Hiramatsu, Yoshihiro× Mizukami, Tomoyuki |
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著者別表示 |
平松, 良浩
× 平松, 良浩
× 水上, 知行
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書誌情報 |
Journal of Geophysical Research B: Solid Earth 巻 118, 号 8, p. 4253-4264, 発行日 2013-01-01 |
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ISSN | ||||||||||
収録物識別子タイプ | ISSN | |||||||||
収録物識別子 | 0148-0227 | |||||||||
NCID | ||||||||||
収録物識別子タイプ | NCID | |||||||||
収録物識別子 | AA10522493 | |||||||||
DOI | ||||||||||
関連タイプ | isVersionOf | |||||||||
識別子タイプ | DOI | |||||||||
関連識別子 | 10.1002/jgrb.50300 | |||||||||
出版者 | ||||||||||
出版者 | American Geophysical Union (AGU) | |||||||||
抄録 | ||||||||||
内容記述タイプ | Abstract | |||||||||
内容記述 | Shear wave splitting from local intermediate-depth earthquakes is investigated to detect the anisotropic structure in the mantle wedge beneath the South Kyushu area, Japan. We observed shear wave splitting with NEE-SWW to NWW-SEE polarization directions and delay times of 0.04-0.63 s. Trench-normal shear wave polarization anisotropy with a delay time greater than 0.3 s probably overlaps in the high VP/VS region at a depth of 100-150 km beneath the volcanic front. Model calculations for the cause of the anisotropy suggest that the development of "C-type" olivine crystallographic preferred orientation (CPO) with a trench-parallel b axis concentration and a trench-normal a axis concentration best reproduces observations compared to A-, B-, or E-type olivine CPOs and antigorite CPO. We conclude that a thick anisotropic layer, approximately 50 km, is formed by concentration of interstitial fluid in peridotite. We briefly discuss the mechanism carrying water to the deep mantle wedge. A possible explanation is that interstitial fluids in the mantle wedge are effectively released because of a decrease in dihedral angles of olivine-fluid interfaces at 150 km depth. Our results imply a close relation between the high density of explosive volcanoes in the South Kyushu area and the underlying water-rich mantle. © 2013. American Geophysical Union. All Rights Reserved. | |||||||||
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出版タイプ | AM | |||||||||
出版タイプResource | http://purl.org/coar/version/c_ab4af688f83e57aa |