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基于古海平面观测的三维地幔粘度的GIA成像 - 第一部分:粘度横向变化地球的灵敏度核

GIA imaging of 3-D mantle viscosity based on palaeo sea level observations - Part I: Sensitivity kernels for an Earth with laterally varying viscosity.

作者信息

Lloyd Andrew J, Crawford Ophelia, Al-Attar David, Austermann Jacqueline, Hoggard Mark J, Richards Fred D, Syvret Frank

机构信息

Lamont Doherty Earth Observatory, Columbia University, Palisades, NY 10964, USA.

Bullard Laboratories, Department of Earth Sciences, University of Cambridge, Madingley Road, Cambridge CB30EZ, UK.

出版信息

Geophys J Int. 2023 Nov 21;236(2):1139-1171. doi: 10.1093/gji/ggad455. eCollection 2024 Feb.

Abstract

A key initial step in geophysical imaging is to devise an effective means of mapping the sensitivity of an observation to the model parameters, that is to compute its Fréchet derivatives or sensitivity kernel. In the absence of any simplifying assumptions and when faced with a large number of free parameters, the adjoint method can be an effective and efficient approach to calculating Fréchet derivatives and requires just two numerical simulations. In the Glacial Isostatic Adjustment problem, these consist of a forward simulation driven by changes in ice mass and an adjoint simulation driven by loads that are applied at the observation sites. The theoretical basis for this approach has seen considerable development over the last decade. Here, we present the final elements needed to image 3-D mantle viscosity using a dataset of palaeo sea-level observations. Developments include the calculation of viscosity Fréchet derivatives (i.e. sensitivity kernels) for relative sea-level observations, a modification to the numerical implementation of the forward and adjoint problem that permits application to 3-D viscosity structure, and a recalibration of initial sea level that ensures the forward simulation honours present-day topography. In the process of addressing these items, we build intuition concerning how absolute sea-level and relative sea-level observations sense Earth's viscosity structure and the physical processes involved. We discuss examples for potential observations located in the near field (Andenes, Norway), far field (Seychelles), and edge of the forebulge of the Laurentide ice sheet (Barbados). Examination of these kernels: (1) reveals why 1-D estimates of mantle viscosity from far-field relative sea-level observations can be biased; (2) hints at why an appropriate differential relative sea-level observation can provide a better constraint on local mantle viscosity and (3) demonstrates that sea-level observations have non-negligible 3-D sensitivity to deep mantle viscosity structure, which is counter to the intuition gained from 1-D radial viscosity Fréchet derivatives. Finally, we explore the influence of lateral variations in viscosity on relative sea-level observations in the Amundsen Sea Embayment and at Barbados. These predictions are based on a new global 3-D viscosity inference derived from the shear-wave speeds of GLAD-M25 and an inverse calibration scheme that ensures compatibility with certain fundamental geophysical observations. Use of the 3-D viscosity inference leads to: (1) generally greater complexity within the kernel; (2) an increase in sensitivity and presence of shorter length-scale features within lower viscosity regions; (3) a zeroing out of the sensitivity kernel within high-viscosity regions where elastic deformation dominates and (4) shifting of sensitivity at a given depth towards distal regions of weaker viscosity. The tools and intuition built here provide the necessary framework to explore inversions for 3-D mantle viscosity based on palaeo sea-level data.

摘要

地球物理成像的一个关键初始步骤是设计一种有效的方法来绘制观测对模型参数的敏感度,即计算其弗雷歇导数或敏感度核。在没有任何简化假设且面对大量自由参数的情况下,伴随方法可以是计算弗雷歇导数的一种有效且高效的方法,并且只需要两次数值模拟。在冰川均衡调整问题中,这两次模拟包括由冰量变化驱动的正演模拟和由观测点施加的载荷驱动的伴随模拟。在过去十年中,这种方法的理论基础有了相当大的发展。在这里,我们展示了利用古海平面观测数据集对三维地幔粘度进行成像所需的最终要素。进展包括计算相对海平面观测的粘度弗雷歇导数(即敏感度核),对正演和伴随问题数值实现的修改,以允许应用于三维粘度结构,以及对初始海平面的重新校准,以确保正演模拟符合现今地形。在解决这些问题的过程中,我们建立了关于绝对海平面和相对海平面观测如何感知地球粘度结构以及所涉及物理过程的直观认识。我们讨论了位于近场(挪威安德内斯)、远场(塞舌尔)和劳伦泰德冰盖前隆边缘(巴巴多斯)的潜在观测示例。对这些核的研究:(1)揭示了为何从远场相对海平面观测得到的地幔粘度一维估计可能存在偏差;(2)暗示了为何适当的差分相对海平面观测可以对局部地幔粘度提供更好的约束;(3)表明海平面观测对深部地幔粘度结构具有不可忽略的三维敏感度,这与从一维径向粘度弗雷歇导数获得的直观认识相反。最后,我们探讨了粘度横向变化对阿蒙森海湾区和巴巴多斯相对海平面观测的影响。这些预测基于从GLAD-M25的剪切波速度推导出来的新的全球三维粘度推断以及确保与某些基本地球物理观测兼容的反演校准方案。使用三维粘度推断导致:(1)核内通常具有更大的复杂性;(2)在较低粘度区域内敏感度增加且出现较短长度尺度的特征;(3)在弹性变形占主导的高粘度区域内敏感度核归零;(4)在给定深度处敏感度向较弱粘度的远端区域转移。这里构建的工具和直观认识为基于古海平面数据探索三维地幔粘度反演提供了必要的框架。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/bf4b/10753356/345c899d4f87/ggad455fig1.jpg

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