Characterizing the Background Noise Level of Rotational Ground Motions on Earth

IF 2.6 3区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
A. Brotzer, H. Igel, É. Stutzmann, J. Montagner, F. Bernauer, J. Wassermann, R. Widmer-Schnidrig, Chin-Jen Lin, Sergey Kiselev, Frank Vernon, K. U. Schreiber
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Abstract

The development of high-sensitive ground-motion instrumentation for Earth and planetary exploration is governed by so-called low-noise models, which characterize the minimum level of physical ground motions, observed across a very broad frequency range (0.1 mHz–100 Hz). For decades, broadband instruments for seismic translational ground-motion sensing allowed for observations down to the Earth’s low-noise model. Knowing the lowermost noise level distribution across frequencies enabled not only to infer characteristics of Earth such as the ocean microseismic noise (microseisms) and seismic hum, but also to develop highly successful ambient seismic noise analysis techniques in seismology. Such a low-noise model currently does not exist for rotational ground motions. In the absence of a substantial observational database, we propose a preliminary rotational low-noise model (RLNM) for transverse rotations based on two main wavefield assumptions: the frequency range under investigation is dominated by surface-wave energy, and the employed phase velocity models for surface waves are representative. These assumptions hold, in particular, for a period range of about 2–50 s and lose validity towards long periods when constituents produced by atmospheric pressure dominate. Because noise levels of vertical and horizontal accelerations differ, we expect also different noise levels for transverse and vertical rotations. However, at this moment, we propose a common model for both types of rotations based on the transverse RLNM. We test our RLNM against available direct observations provided by two large-scale ring lasers (G-ring and ROMY) and array-derived rotations (Piñon Flats Observatory array, Gräfenberg array, and ROMY array). We propose this RLNM to be useful as guidance for the development of high-performance rotation instrumentation for seismic applications in a range of 2–50 s. Achieving broadband sensitivity below such a RLNM remains a challenging task, but one that has to be achieved.
确定地球旋转地面运动的背景噪声水平
用于地球和行星探测的高灵敏度地动仪的开发受制于所谓的低噪声模型,该模型描述了在非常宽的频率范围(0.1 mHz-100 Hz)内观测到的物理地动的最低水平。几十年来,用于地震平移地动传感的宽带仪器可以观测到地球的低噪声模型。了解各频率的最低噪声级分布,不仅可以推断地球的特征,如海洋微地震噪声(微地震)和地震嗡嗡声,还可以在地震学中开发非常成功的环境地震噪声分析技术。目前还没有针对旋转地面运动的低噪声模型。在缺乏大量观测数据库的情况下,我们提出了一个初步的横向旋转低噪声模型(RLNM),该模型基于两个主要的波场假设:所研究的频率范围以面波能量为主,所采用的面波相速度模型具有代表性。这些假设尤其适用于 2-50 秒左右的周期范围,但当大气压力产生的成分占主导地位时,这些假设就失去了有效性。由于垂直加速度和水平加速度的噪声水平不同,我们预计横向旋转和垂直旋转的噪声水平也不同。不过,目前我们提出了一个基于横向 RLNM 的两类旋转的通用模型。我们用两个大型环形激光器(G-ring 和 ROMY)提供的现有直接观测数据和阵列衍生旋转(皮农平地观测站阵列、格拉芬伯格阵列和 ROMY 阵列)来测试我们的 RLNM。我们建议将该 RLNM 作为指导,用于开发 2-50 秒范围内的高性能地震应用旋转仪器。
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来源期刊
Seismological Research Letters
Seismological Research Letters 地学-地球化学与地球物理
CiteScore
6.60
自引率
12.10%
发文量
239
审稿时长
3 months
期刊介绍: Information not localized
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