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基于三维各向异性波动层析成像的地中海中部板块几何结构与上地幔流动模式

Slab Geometry and Upper Mantle Flow Patterns in the Central Mediterranean From 3D Anisotropic -Wave Tomography.

作者信息

Rappisi F, VanderBeek B P, Faccenda M, Morelli A, Molinari I

机构信息

Dipartimento di Geoscienze Università di Padova Padova Italy.

Istituto Nazionale di Geofisica e Vulcanologia Bologna Italy.

出版信息

J Geophys Res Solid Earth. 2022 May;127(5):e2021JB023488. doi: 10.1029/2021JB023488. Epub 2022 May 8.

DOI:10.1029/2021JB023488
PMID:35865146
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC9286615/
Abstract

We present the first three-dimensional (3D) anisotropic teleseismic -wave tomography model of the upper mantle covering the entire Central Mediterranean. Compared to isotropic tomography, it is found that including the magnitude, azimuth, and, importantly, dip of seismic anisotropy in our inversions simplifies isotropic heterogeneity by reducing the magnitude of slow anomalies while yielding anisotropy patterns that are consistent with regional tectonics. The isotropic component of our preferred tomography model is dominated by numerous fast anomalies associated with retreating, stagnant, and detached slab segments. In contrast, relatively slower mantle structure is related to slab windows and the opening of back-arc basins. To better understand the complexities in slab geometry and their relationship to surface geological phenomenon, we present a 3D reconstruction of the main Central Mediterranean slabs down to 700 km based on our anisotropic model. -wave seismic anisotropy is widespread in the Central Mediterranean upper mantle and is strongest at 200-300 km depth. The anisotropy patterns are interpreted as the result of asthenospheric material flowing primarily horizontally around the main slabs in response to pressure exerted by their mid-to-late Cenezoic horizontal motion, while sub-vertical anisotropy possibly reflects asthenospheric entrainment by descending lithosphere. Our results highlight the importance of anisotropic -wave imaging for better constraining regional upper mantle geodynamics.

摘要

我们展示了首个覆盖整个地中海中部的上地幔三维(3D)各向异性远震波层析成像模型。与各向同性层析成像相比,研究发现,在反演中纳入地震各向异性的大小、方位角,尤其是倾角,可通过减小低速异常的幅度来简化各向同性非均匀性,同时产生与区域构造一致的各向异性模式。我们首选的层析成像模型的各向同性成分主要由与后撤、停滞和脱离的板块段相关的众多高速异常主导。相比之下,相对较慢的地幔结构与板块窗和弧后盆地的张开有关。为了更好地理解板块几何形状的复杂性及其与地表地质现象的关系,我们基于各向异性模型展示了地中海中部主要板块向下至700公里的三维重建。在地中海中部上地幔中,远震波地震各向异性广泛存在,且在200 - 300公里深度处最强。各向异性模式被解释为软流圈物质主要围绕主要板块水平流动的结果,这是对它们新生代中后期水平运动所施加压力的响应,而近垂直各向异性可能反映了下降岩石圈对软流圈的裹挟。我们的结果凸显了各向异性远震波成像对于更好地约束区域上地幔地球动力学的重要性。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2da0/9286615/7d8b43922d57/JGRB-127-0-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2da0/9286615/32e56e02c5e3/JGRB-127-0-g005.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2da0/9286615/1b2ca8d4ba4b/JGRB-127-0-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2da0/9286615/c55702bc06fc/JGRB-127-0-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2da0/9286615/7d8b43922d57/JGRB-127-0-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2da0/9286615/32e56e02c5e3/JGRB-127-0-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2da0/9286615/f97f2ab508b1/JGRB-127-0-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2da0/9286615/fa69f7fc9440/JGRB-127-0-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2da0/9286615/9e05b8099b9f/JGRB-127-0-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2da0/9286615/1b2ca8d4ba4b/JGRB-127-0-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2da0/9286615/c55702bc06fc/JGRB-127-0-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2da0/9286615/7d8b43922d57/JGRB-127-0-g001.jpg

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Slab narrowing in the Central Mediterranean: the Calabro-Ionian subduction zone as imaged by high resolution seismic tomography.
地中海中部板块变薄:高分辨率地震层析成像显示的卡拉布里亚-爱奥尼亚俯冲带
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