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洋中脊的高地震衰减揭示了深部熔体的分布。

High seismic attenuation at a mid-ocean ridge reveals the distribution of deep melt.

机构信息

Lamont-Doherty Earth Observatory, Columbia University, 61 Rte. 9W, Palisades, NY 10964, USA.

Department of Earth, Environmental, and Planetary Sciences, Brown University, 324 Brook Street, Providence, RI 02912, USA.

出版信息

Sci Adv. 2017 May 24;3(5):e1602829. doi: 10.1126/sciadv.1602829. eCollection 2017 May.

DOI:10.1126/sciadv.1602829
PMID:28560338
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC5443646/
Abstract

At most mid-ocean ridges, a wide region of decompression melting must be reconciled with a narrow neovolcanic zone and the establishment of full oceanic crustal thickness close to the rift axis. Two competing paradigms have been proposed to explain melt focusing: narrow mantle upwelling due to dynamic effects related to in situ melt or wide mantle upwelling with lateral melt transport in inclined channels. Measurements of seismic attenuation provide a tool for identifying and characterizing the presence of melt and thermal heterogeneity in the upper mantle. We use a unique data set of teleseismic body waves recorded on the Cascadia Initiative's Amphibious Array to simultaneously measure seismic attenuation and velocity across an entire oceanic microplate. We observe maximal differential attenuation and the largest delays ([Formula: see text] s and δ ~ 2 s) in a narrow zone <50 km from the Juan de Fuca and Gorda ridge axes, with values that are not consistent with laboratory estimates of temperature or water effects. The implied seismic quality factor ( ≤ 25) is among the lowest observed worldwide. Models harnessing experimentally derived anelastic scaling relationships require a 150-km-deep subridge region containing up to 2% in situ melt. The low viscosity and low density associated with this deep, narrow melt column provide the conditions for dynamic mantle upwelling, explaining a suite of geophysical observations at ridges, including electrical conductivity and shear velocity anomalies.

摘要

在大多数大洋中脊,必须协调宽的减压熔融区、狭窄的新火山带以及靠近裂谷轴的全洋壳厚度的建立。有两个相互竞争的范式被提出来解释熔体聚焦:由于与原地熔体相关的动力学效应引起的狭窄地幔上涌,或具有侧向熔体输送的倾斜通道中的宽地幔上涌。地震衰减测量为识别和表征上地幔中熔体和热非均质性的存在提供了一种工具。我们使用凯斯卡迪亚倡议两栖阵列上记录的远地震体波的独特数据集,同时测量整个大洋微板块的地震衰减和速度。我们在距胡安·德富卡和戈达脊轴不到 50 公里的狭窄区域中观察到最大的差分衰减和最大的延迟([公式:见文本] s 和 δ~2 s),其值与实验室估计的温度或水效应不一致。隐含的地震品质因数(≤25)是全球观测到的最低的之一。利用实验得出的粘弹性标度关系的模型需要一个 150 公里深的海底区域,其中包含高达 2%的原地熔体。这种深而狭窄的熔体柱的低粘度和低密度为地幔动力上涌提供了条件,解释了一系列在海脊的地球物理观测,包括电导率和剪切速度异常。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/31f3/5443646/f9b2cc31877c/1602829-F4.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/31f3/5443646/5ad66f2aa877/1602829-F1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/31f3/5443646/ddb737dd253d/1602829-F2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/31f3/5443646/96bbeb027c0e/1602829-F3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/31f3/5443646/f9b2cc31877c/1602829-F4.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/31f3/5443646/5ad66f2aa877/1602829-F1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/31f3/5443646/ddb737dd253d/1602829-F2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/31f3/5443646/96bbeb027c0e/1602829-F3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/31f3/5443646/f9b2cc31877c/1602829-F4.jpg

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