Satellite magnetic field measurements: Applications in studying the deep Earth

C. Constable, S. Constable
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引用次数: 28

Abstract

Following a 20 years hiatus, there are several magnetometry satellites in near-Earth orbit providing a global view of the geomagnetic field and how it changes. The measured magnetic field is an admixture of all field sources, among which one must identify the contributions of interest, namely (1) the field generated in Earth's core, and (2) the fields induced in Earth's mantle by external magnetic variations used in studies of electrical conductivity. Models of the core field can be downward continued to the core surface under the assumption that Earth's mantle is a source free region with zero electrical conductivity. Additional assumptions are invoked to estimate the fluid flow at the core surface. New satellite measurements provide an unprecedented view of changes in the core over the past 20 years; further measurements will clarify the temporal spectrum of the secular variation. Secular changes are coupled to changes in length of day, and recent modeling of torsional oscillations in the core can provide an explanation for the abrupt changes in the field known as geomagnetic jerks. Mantle induction studies require a comprehensive approach to magnetic field modeling. Unwanted internal field contributions are removed to yield time series of external variations and their induced counterparts: improved modeling, combined with the increased data accuracy, and longer term magnetic measurements make conductivity studies feasible. One-dimensional global conductivity responses have been estimated under strong assumptions about the structure of the source field. Ongoing improvements to this work will take account of more complicated source-field structure, three-dimensional Earth structure, and spatio-temporal aliasing due to satellite motion. Modeling of three-dimensional near surface conductivity structure, and the use of time-domain rather than frequency-domain techniques to estimate the 3-D Earth response are needed. Progress could be furthered by future magnetometer missions that involve multiple satellite configurations.
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卫星磁场测量:在地球深部研究中的应用
在中断了20年之后,近地轨道上有几颗磁强计卫星提供了地磁场及其变化的全球视图。测量的磁场是所有场源的混合物,其中必须确定感兴趣的贡献,即(1)地核产生的场,(2)电导率研究中使用的由外部磁场变化在地幔中引起的场。假设地幔是零电导率的无源区,地核场模型可以向下延续到地核表面。附加的假设被用来估计岩心表面的流体流动。新的卫星测量为过去20年来地核的变化提供了前所未有的视角;进一步的测量将阐明长期变化的时间谱。长期的变化与白昼长度的变化相关联,最近对地核扭转振荡的建模可以解释地磁的突然变化。地幔感应研究需要一个全面的磁场建模方法。去除不必要的内部磁场贡献,产生时间序列的外部变化及其诱导对应物:改进的建模,结合提高的数据准确性,以及更长期的磁测量,使电导率研究变得可行。在对源场结构的强假设下,估计了一维全球电导率响应。这项工作的持续改进将考虑到更复杂的源场结构、三维地球结构和卫星运动引起的时空混叠。三维近地表电导率结构的建模,以及使用时域而不是频域技术来估计三维地球响应是必要的。未来涉及多种卫星配置的磁力计任务可能会进一步推动这一进展。
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