Amagase观测站的潮汐应变测量

Q4 Earth and Planetary Sciences
M. Harada, T. Furuzawa, F. Ohya, W. Morii, Masaru Yamada
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引用次数: 0

摘要

自1967年以来,在Amagase天文台使用“滚轮”超invar-bar延伸计对地面应变进行了连续观测。但Takemoto(1975)报道,由于带有滚柱式放大镜的探测器产生的摩擦阻力,其表观位移小于激光干涉仪。因此,自1995年以来,我们一直采用带差动变压器的检测仪,并配套不锈钢丝的超高压棒。利用1997年1月1日至1999年12月31日的新系统数据,确定潮汐因子,特别是O1和M2成分。并将实测潮汐因子与考虑海洋负荷效应的理论潮汐因子进行了比较。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Measurement of Earth Tidal Strain in Amagase Observatory
In Amagase Observatory, the continuous observation of ground strain has been carried out since 1967 by "roller" super-invar-bar extensometers. But Takemoto (1975) reported that apparent displacement is smaller than that obtained laser interferometer due to the frictional resistance arising from detector with roller type magnifier. Therefore we have been employing the detector with differential transformer and supporting the super-invar-bar with stainless wire since 1995. In order to define tidal factors, especially O1 and M2 constituents, we used the new system data from January 1, 1997 to December 31, 1999. And we compared the observed tidal factor with theoretical it, which including ocean loading effect.
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来源期刊
Journal of the Geodetic Society of Japan
Journal of the Geodetic Society of Japan Earth and Planetary Sciences-Earth and Planetary Sciences (all)
CiteScore
0.20
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