• ISSN 2097-1893
  • CN 10-1855/P
侍文,陈石,韩建成,贾路路. 2022. 岩石圈有效弹性厚度估算方法研究进展. 地球与行星物理论评,53(3):301-315. DOI: 10.19975/j.dqyxx.2021-062
引用本文: 侍文,陈石,韩建成,贾路路. 2022. 岩石圈有效弹性厚度估算方法研究进展. 地球与行星物理论评,53(3):301-315. DOI: 10.19975/j.dqyxx.2021-062
Shi W, Chen S, Han J C, Jia L L. 2022. Estimation of the effective elastic thickness of the lithosphere: progress and prospects. Reviews of Geophysics and Planetary Physics, 53(3): 301-315. DOI: 10.19975/j.dqyxx.2021-062
Citation: Shi W, Chen S, Han J C, Jia L L. 2022. Estimation of the effective elastic thickness of the lithosphere: progress and prospects. Reviews of Geophysics and Planetary Physics, 53(3): 301-315. DOI: 10.19975/j.dqyxx.2021-062

岩石圈有效弹性厚度估算方法研究进展

Estimation of the effective elastic thickness of the lithosphere: progress and prospects

  • 摘要: 岩石圈有效弹性厚度(Te)是度量岩石圈力学强度的一个定量指标,是研究岩石圈大规模构造的有力工具. 研究岩石圈有效弹性厚度,对于了解岩石圈力学强度及其横向变化特征、重力均衡状态、热状态、地壳厚度变化、岩石圈内部圈层耦合关系和壳幔流变结构等信息具有重要作用. 本文介绍了岩石圈有效弹性厚度的研究背景和基本估算原理,并总结了国内外岩石圈有效弹性厚度估算方法的研究进展. 同时,本文也详细论述了这些岩石圈Te估算方法的工作原理,并分析比较了它们的优缺点. 目前估算岩石圈Te的方法主要包括:正演法、谱分析方法(包括:导纳法和相关性法)和屈服应力包络法. 近年来,随着数字信号处理技术的不断发展,谱分析方法已逐渐成为最流行的岩石圈Te估算方法. 地形和重力异常数据的功率谱估计是谱分析方法的关键环节,这些功率谱估计结果的质量会直接影响岩石圈Te计算结果的准确性和可靠性. 因此,周期图法、最大熵法、多窗谱分析、小波谱分析等在数字信号处理领域中应用效果较好的功率谱估算技术,逐渐被引入到了岩石圈有效弹性厚度的计算中,以获取准确可靠的Te计算结果. 最近,Te各向异性的研究也取得了一定的成果,为岩石圈垂直受力状态、不同圈层耦合程度以及岩石圈变形和流变特性的研究提供了重要科学依据. 最后,本文提出了未来值得深入的岩石圈有效弹性厚度研究方向,可为开展相关研究提供有益参考.

     

    Abstract: The lithospheric strength is a key factor in controlling the lithosphere dynamics and deformations. The effective elastic thickness (Te) of the lithosphere can always be used to address the lithospheric strength. Hence, it is a powerful tool for studying the large-scale lithospheric structure. Estimates of Te over both continent and ocean are important for understanding the lithospheric strength with its lateral variations, crustal gravity isostatic state, lithospheric thermal state and rheological structure, and the coupling at the lithosphere-asthenosphere boundary. This article summaries the background of Te estimation and reviews the domestic and overseas research progress on the estimation methods. The main methods for estimating Te include forward modeling of deformations, spectral techniques (i.e., admittance and coherence) based on the cross-spectral analysis of the gravity and topography data, and direct estimations of Te based on the yield strength envelope. The method of deformation forward modeling estimates Te from the optimal lithospheric deflection model, with which the calculated theoretical gravity anomalies best fit the observed ones. The spectral technique calculates Te through analyzing the relationship between observed gravity and topography data in the spatial wavenumber domain, including admittance and coherence methods. The admittance method operates the Te estimation basically based on the spectrum ratio of the gravity to topography signals, while the coherence method works by examining the variation characteristics of the relationship between those two signals in wavenumber domain. Under long-wavelength loading, the lithosphere tends to act as a regional isostatic equilibrium mode. In this model, the lithosphere deflected and the gravity anomaly could be completely related to the topography, i.e., the correlation between those two is close to 1. In contrast, under short-wavelength loading, the lithosphere usually does not deflect due to the lithospheric strength, hence the gravity-topography correlation is close to 0. The gravity-topography correlation decreases from 1 to 0 with the wavenumber. The wavelength around the change point of the correlation with the value of 0.5 representing the state transition of the lithosphere from isostatic equilibrium to disequilibrium, is determined by the lithospheric strength, hence could be used to address Te. The yield strength envelope method estimates Te based on the rock mechanics experiments which usually study how strength varies according to temperature and composition of the crust and mantle lithosphere. Recently, with the development of modern digital signal processing technology, spectral techniques have gradually become the most popular approaches for the Te estimation. Calculating the observed admittance and coherence needs the gravity and topography auto-spectra and the cross-spectrum to be computed first. Those two spectra can be obtained using periodogram, maximum entropy, multitapers and wavelet methods. Periodogram is a direct spectral estimation method used up until the late 1990s, although it is not a very accurate one due to the spectral leakage. While maximum entropy spectral estimation can minimize the spectral leakage to some extent and yield accurate spectra in small-window spectral estimation, multitaper method deals with spectral leakage well circumvent the problem of small window sizes. The wavelet method has also been widely developed for computing spectra during Te estimation, because the wavelet transform can separate closely spaced and high-wavenumber features, whilst the windowed Fourier transform likely to smear the information, either in space or wavenumber depending on the window size. The anisotropy of the lithosphere is an important parameter of the lithospheric mechanical property and can largely affect the calculated Te values. To obtain reliable Te, the anisotropy of Te should be considered during the Te estimation. Moreover, Te anisotropy can affect the crustal stress state, crustal rheological properties, and microfractures developments. Those subjects can provide important clues for the study of breeding environments, occurrence processes, and mechanisms of earthquakes. This review also discusses the principles, advantages, and disadvantages of the estimation methods. Finally, this article provides avenues for future research.

     

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