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地球上重量信号的检测限

Limits of Detection of Gravimetric Signals on Earth.

作者信息

Rosat S, Hinderer J

机构信息

Institut de Physique du Globe de Strasbourg, UMR 7516, Université de Strasbourg/EOST, CNRS, Strasbourg, France.

出版信息

Sci Rep. 2018 Oct 17;8(1):15324. doi: 10.1038/s41598-018-33717-z.

DOI:10.1038/s41598-018-33717-z
PMID:30333563
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC6193024/
Abstract

Gravimetry is a well-established tool to probe the deep Earth's processes. Geophysical signals coming from the deep Earth, like the inner core free oscillations, have however never been detected. Challenging quests raise the question of the limits of detection of elusive signals at the Earth's surface. Knowledge of the instrumental limits and of the environmental noise level at a site is fundamental to judge the true sensitivity of an instrument. We perform a noise level comparison of various gravimeters and a long-period seismometer at the J9 gravimetric observatory of Strasbourg (France) to provide a reference of instrumental performances. We then apply a three-channel correlation analysis of time-varying surface gravity from superconducting gravimeter records to isolate the instrumental self-noise from the environmental noise. The self-noise coherence analysis shows that the instrumental noise level remains flat towards lower frequencies till 10 Hz. At seismic frequencies, the self-noise is well explained by a Brownian thermal noise model. At daily and sub-daily time-scales, self-noise is increasing with the period but to a much lesser extent than observed noise level. Observed Earth's ambient noise level at sub-seismic frequencies is hence mostly due to unmodeled geophysical processes. At hourly time-scales, our ability to detect elusive signals coming from the deep Earth's interior is not limited by the instrument capability but is mostly due to the environmental effects.

摘要

重力测量是探测地球深部过程的一种成熟工具。然而,来自地球深部的地球物理信号,如内核自由振荡,从未被检测到。具有挑战性的探索引发了关于在地球表面探测难以捉摸信号的检测极限问题。了解某一地点的仪器极限和环境噪声水平对于判断仪器的真正灵敏度至关重要。我们在法国斯特拉斯堡的J9重力观测站对各种重力仪和一台长周期地震仪进行了噪声水平比较,以提供仪器性能的参考。然后,我们对超导重力仪记录的随时间变化的地表重力进行三通道相关性分析,以将仪器自噪声与环境噪声分离。自噪声相干分析表明,仪器噪声水平在低频至10赫兹范围内保持平稳。在地震频率下,自噪声可以用布朗热噪声模型很好地解释。在日和亚日时间尺度上,自噪声随周期增加,但增幅远小于观测到的噪声水平。因此,在亚地震频率下观测到的地球环境噪声水平主要是由于未建模的地球物理过程。在小时时间尺度上,我们探测来自地球深部内部难以捉摸信号的能力不受仪器能力限制,主要是由于环境影响。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/77ee/6193024/ceafbe568474/41598_2018_33717_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/77ee/6193024/ebd98459dc25/41598_2018_33717_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/77ee/6193024/abb6c4105224/41598_2018_33717_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/77ee/6193024/ceafbe568474/41598_2018_33717_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/77ee/6193024/ebd98459dc25/41598_2018_33717_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/77ee/6193024/abb6c4105224/41598_2018_33717_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/77ee/6193024/ceafbe568474/41598_2018_33717_Fig3_HTML.jpg

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