地震观测

M. G. Gudzin, E. Holle
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引用次数: 0

摘要

本文介绍了在VELA统一项目下正在美国建立的一个地震观测站的仪器和主要工作特点。地震探测器排列成阵列,以提供方向灵敏度、噪声消除和速度过滤。它们位于偏远的、地震安静的地区。频率范围为0.001至10cps的信号由四个单独的仪器系统检测、放大和记录,每个仪器系统都显示出定制的频率响应,以允许研究特定类型的地球运动。在正常地球背景振动的驱动下,地震探测器的输出功率约为10-5瓦。放大由振镜-光管桥式放大器提供。数据记录在磁带,16毫米带状薄膜和热敏纸上。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Seismological Observatories
This paper describes the instrumentation and principal operating characteristics of one of the seismological observatories being established in the United States under Project VELA UNIFORM. Seismic detectors are arranged in arrays to provide directional sensitivity, noise cancellation, and velocity filtering. They are located in remote, seismically quiet areas. Signals in the frequency range of 0.001 to 10 cps are detected, amplified, and recorded by four individual instrumentation systems, each exhibiting a frequency response tailored to permit studies of a specific type of earth motion. Seismic detectors used produce output power levels of approximately 10-5 watts when driven by normal earth background vibrations. Amplification is provided by galvanometer-phototube bridge amplifiers. Data are recorded on magnetic tape, 16-mm strip film and on heat-sensitive paper.
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