星球激光干扰测量地震声学天文台
Grigory Dolgikh1, Sergey Budrin1, Stanislav Dolgikh1
1V.I. Il'ichev Pacific Oceanological Institute FEB RAS, 690041 Vladivostok, Russia.
Sensors (Basel, Switzerland)
|January 11, 2025
概括
一个新的行星激光干扰测量地震声学天文台可以精确地确定全球范围内超声波干扰的来源. 该系统识别信号分歧和传播期间的能量损失,增强地震和声学监测能力.
科学领域:
- 地质物理学 地质物理学
- 声学 声学 在声学方面
- 激光干扰计是指激光干扰计.
背景情况:
- 地震声学监测依赖于检测和定位干扰.
- 星球范围内的超声波探测在信号定位和特征化方面提出了重大挑战.
研究的目的:
- 描述行星激光干扰测量地震声学天文台的发展和能力.
- 建立在行星距离处的超声波干扰的方向查找和信号分析方法.
主要方法:
- 使用一个六个静止激光压力计的网络与不平等的手臂.
- 采用三角测量方法,用于查找超声波干扰的方向.
- 集成一个高精度计时系统 (TRIMBLE 5700) 进行同步测量.
主要成果:
- 开发了基本方法,用于在任何行星距离处发现超声波干扰的方向.
- 证明了使用空间分离压力计来确定信号分歧和传播期间的能量损失的能力.
- 在0-1000 Hz频率范围内,实现了10 pm的位移记录准确度.
结论:
- 已建立的行星激光干扰测量地震声学天文台可以确定全球变形超声波干扰的主要来源.
- 该系统可以对信号特征进行详细分析,包括分歧和能量减弱.
- 这个天文台增强了监测和理解行星规模地震声学现象的能力.
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