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Generation and driving forces of plate-like motion and asymmetric subduction in dynamical models of an integrated mantle-litho sphere system

https://hiroshima.repo.nii.ac.jp/records/2008644
https://hiroshima.repo.nii.ac.jp/records/2008644
19a5acf1-c2a3-4666-bade-9d66e25628e3
名前 / ファイル ライセンス アクション
PEPI_166_128.pdf PEPI_166_128.pdf (2.2 MB)
Item type デフォルトアイテムタイプ_(フル)(1)
公開日 2023-03-18
タイトル
タイトル Generation and driving forces of plate-like motion and asymmetric subduction in dynamical models of an integrated mantle-litho sphere system
言語 en
作成者 Nakakuki, Tomoeki

× Nakakuki, Tomoeki

en Nakakuki, Tomoeki

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Hamada, Chiho

× Hamada, Chiho

en Hamada, Chiho

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Tagawa, Michio

× Tagawa, Michio

en Tagawa, Michio

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アクセス権
アクセス権 open access
アクセス権URI http://purl.org/coar/access_right/c_abf2
権利情報
権利情報 Copyright (c) 2008 Elsevier B.V.
主題
主題Scheme Other
主題 plate-like motion
主題
主題Scheme Other
主題 mantle convection
主題
主題Scheme Other
主題 asymmetric subduction
主題
主題Scheme Other
主題 yield strength
主題
主題Scheme NDC
主題 450
内容記述
内容記述 The dynamical effects of an asymmetric subduction structure on the generation of plate-like motion were investigated using two-dimensional numerical models of the integrated lithosphere-mantle system. To dynamically generate the plate boundary, we introduce a history-dependent rheology in which the yield strength is determined by past fractures. Only the buoyancy due to the internal density contrast consistently drives convective flow, including the motion of the viscous lithosphere, without imposed boundary conditions. We first investigate the effects of plate yield strength, friction at the plate boundary, and plate age on the emergence of plate-like motion with asymmetric subduction. Plate-like motion is generated when maximum plate strength is as high as that estimated by experimental rheology studies. The reason for this is that asymmetric subduction requires a plate-bending force much less than that for symmetric subduction because the plate gently bends when one-sided subduction occurs. In contrast, the strength of the plate boundary has to be very small for emergence of subduction, as several previous studies on the numerical convection and subduction modeling have pointed out. Development of the subducted slab is also controlled by the age of the plate. In the early stages of subduction, older plates increase their velocities faster because of their larger negative buoyancy. After the slab develops, the plate stiffness, that is, both the yield strength and the plate thickness, control plate velocity so that an older plate subducts more sluggishly. We next explore effects of viscosity layering in the underlying mantle, focusing on the mechanism in which the asthenosphere promotes plate motion. The low viscosity under the lithosphere enhances a mantle drag force that drives the plate, not only concentrating the convective flow beneath the plate but also enlarging its aspect ratio. We also examine longevity of the plate-like motion using the convection models with asymmetric subduction. The asymmetrically s
言語 en
出版者
出版者 Elsevier B.V.
言語
言語 eng
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_6501
資源タイプ journal article
出版タイプ
出版タイプ AO
出版タイプResource http://purl.org/coar/version/c_b1a7d7d4d402bcce
関連情報
識別子タイプ DOI
関連識別子 10.1016/j.pepi.2007.12.004
関連情報
関連タイプ isVersionOf
識別子タイプ DOI
関連識別子 http://dx.doi.org/10.1016/j.pepi.2007.12.004
収録物識別子
収録物識別子タイプ ISSN
収録物識別子 0031-9201
収録物識別子
収録物識別子タイプ NCID
収録物識別子 AA00773963
開始ページ
開始ページ 128
書誌情報 Physics of the Earth and Planetary Interiors
Physics of the Earth and Planetary Interiors

巻 166, 号 3-4, p. 128-146, 発行日 2008-02
旧ID 25580
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