首页> 外文期刊>Physics of the Earth and Planetary Interiors: A Journal Devoted to Obsevational and Experimerntal Studies of the Chemistry and Physics of Planetary Interiors and Their Theoretical Interpretation >A Bayesian iterative geomagnetic model with universal data input: Self-consistent spherical harmonic evolution for the geomagnetic field over the last 4000 years
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A Bayesian iterative geomagnetic model with universal data input: Self-consistent spherical harmonic evolution for the geomagnetic field over the last 4000 years

机译:具有通用数据输入的贝叶斯迭代地磁模型:过去4000年来地质磁场的自我一致球形谐波演变

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摘要

Changes of the Earth's magnetic field have been observed with varying spatial and temporal resolution since the middle ages by means of compasses, and later by refined mechanical inclination and intensity instruments, until the modern use of quantum mechanical devices and satellite observations. Ancient records, on the other hand, rely on the natural magnetization of archaeological artifacts and other materials, such as rocks and sediments, being therefore indirect, less accurate and sparser. The combination of such heterogeneous records into a single, self-consistent, global model of the geomagnetic field is very challenging: the highly uneven data coverage, both in space and time, requires a careful handling of data uncertainties and error correlations. Previous models dealt with this problem using separated treatments of instrumental data and indirect records, respectively, as well as a different handling of the dipole field component, with respect to non-dipole terms. Here we present a global geomagnetic field model based, for the first time, on the simultaneous inversion of historical, archaeomagnetic, and volcanic records, using a Bayesian approach with minimal-committing time regularization that minimizes the energy of secular variation. A detailed assessment of data uncertainty and error correlation is used to minimize artifacts generated by the appearance of an overwhelming number of incomplete, mostly declination only records, associated with shipboard measurements in the early colonial period. Our model yields lower dipole energies, which better match modern values, as well as higher non-dipole energies and a stronger secular variation of the dipole moment. Some model artifacts associated with extremely heterogeneous distributions of records in time and space are not completely eliminable and might be caused by incorrect a-priori uncertainty assessments. Alternatively, they might represent an intrinsic limit that can be overcome only by adding new records
机译:由于中世纪通过指南针,以后通过精制的机械倾斜和强度仪器,因此已经观察到地球磁场的变化,以便通过精制的机械倾斜和强度仪器,直到现代使用量子机械装置和卫星观察。另一方面,古代记录依赖于考古文物的自然磁化和其他材料,例如岩石和沉积物,因此是间接的,不准确和稀疏的。这种异构记录成单一的,自我一致的全球模型的结合非常具有挑战性:在空间和时间内,高度不均匀的数据覆盖需要仔细处理数据不确定性和误差相关性。以前的模型分别处理了仪器数据和间接记录的分离处理以及偶极场分量的不同处理,相对于非偶极项。在这里,我们首次使用基于历史,archaeomagnetic和火山记录的同时反演的全球地理磁场模型,使用贝叶斯方面的方法,具有最小化的时间正则化,以最小化世俗变化的能量。对数据不确定性和误差相关性的详细评估用于最小化由早期殖民时期的船上测量相关的压倒性不容缩的外观产生的伪影,主要是终点。我们的模型产生较低的偶极能,更好地匹配现代值,以及更高的非偶极能量以及偶极矩的更强烈的世俗变化。与时间和空间中记录的极其异构分布相关的一些模型伪影不能完全消除,可能是由不正确的a-priori的不确定性评估引起的。或者,它们可能代表可以通过添加新记录来克服的内在限制

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