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3-D multiobservable probabilistic inversion for the compositional and thermal structure of the lithosphere and upper mantle. I: a priori petrological information and geophysical observables

机译:岩石圈和上地幔的成分和热力结构的3-D多观测概率反演。一:先验岩石学信息和地球物理观测

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摘要

Traditional inversion techniques applied to the problem of characterizing the thermal and compositional structure of the upper mantle are not well suited to deal with the nonlinearity of the problem, the trade-off between temperature and compositional effects on wave velocities, the nonuniqueness of the compositional space, and the dissimilar sensitivities of physical parameters to temperature and composition. Probabilistic inversions, on the other hand, offer a powerful formalism to cope with all these difficulties, while allowing for an adequate treatment of the intrinsic uncertainties associated with both data and physical theories. This paper presents a detailed analysis of the two most important elements controlling the outputs of probabilistic (Bayesian) inversions for temperature and composition of the Earth's mantle, namely the a priori information on model parameters, (m), and the likelihood function, L(m). The former is mainly controlled by our current understanding of lithosphere and mantle composition, while the latter conveys information on the observed data, their uncertainties, and the physical theories used to relate model parameters to observed data.The benefits of combining specific geophysical datasets (Rayleigh and Love dispersion curves, body wave tomography, magnetotelluric, geothermal, petrological, gravity, elevation, and geoid), and their effects on L(m), are demonstrated by analyzing their individual and combined sensitivities to composition and temperature as well as their observational uncertainties. The dependence of bulk density, electrical conductivity, and seismic velocities to major-element composition is systematically explored using Monte Carlo simulations. We show that the dominant source of uncertainty in the identification of compositional anomalies within the lithosphere is the intrinsic nonuniqueness in compositional space. A general strategy for defining (m) is proposed based on statistical analyses of a large database of natural mantle samples collected from different tectonic settings (xenoliths, abyssal peridotites, ophiolite samples, etc.). This strategy relaxes more typical and restrictive assumptions such as the use of local/limited xenolith data or compositional regionalizations based on age-composition relations. We demonstrate that the combination of our (m) with a L(m) that exploits the differential sensitivities of specific geophysical observables provides a general and robust inference platform to address the thermochemical structure of the lithosphere and sublithospheric upper mantle. An accompanying paper deals with the integration of these two functions into a general 3-D multiobservable Bayesian inversion method and its computational implementation.
机译:适用于表征上地幔热和成分结构问题的传统反演技术不太适合解决该问题的非线性,温度和成分对波速的影响之间的权衡,成分空间的不唯一性,以及物理参数对温度和成分的敏感性不同。另一方面,概率反演提供了强有力的形式主义来应对所有这些困难,同时允许对与数据和物理理论相关的内在不确定性进行适当处理。本文对控制地幔温度和组成的概率(贝叶斯)反演输出的两个最重要元素进行了详细分析,即关于模型参数的先验信息(m)和似然函数L( m)。前者主要受我们目前对岩石圈和地幔组成的了解所控制,而后者则传达有关观测数据,其不确定性以及用于将模型参数与观测数据相关联的物理理论的信息。结合特定地球物理数据集(Rayleigh和Love色散曲线,体波层析成像,大地电磁,地热,岩石学,重力,高程和大地水准面)及其对L(m)的影响,通过分析它们对成分和温度的敏感性以及各自的观测值进行了证明。不确定性。使用蒙特卡洛模拟系统地探索了堆积密度,电导率和地震速度对主要元素组成的依赖性。我们表明,岩石圈内组成异常识别中不确定性的主要来源是组成空间中的固有非唯一性。基于对从不同构造环境(异岩,深渊橄榄石,蛇绿岩样品等)收集的天然地幔样品的大型数据库的统计分析,提出了定义(m)的一般策略。该策略放宽了更典型和限制性的假设,例如使用局部/有限的异种岩数据或基于年龄-成分关系的成分区域划分。我们证明,我们的(m)与L(m)的组合利用了特定地球物理观测值的差异敏感性,为解决岩石圈和岩石圈下上地幔的热化学结构提供了一个通用而强大的推断平台。随附的论文讨论了将这两个函数集成到通用的3-D多观测贝叶斯反演方法中及其计算实现。

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