首页> 外文会议>Conference on Laser Optics 2000: Solid State Lasers Jun 26-30, 2000, St. Petersburg, Russia >Large scale laser gravitational interferometer with suspended mirrors for fundamental geodynamics
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Large scale laser gravitational interferometer with suspended mirrors for fundamental geodynamics

机译:带有悬吊镜的大型激光重力干涉仪,用于基本地球动力学

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A Fabry-Perot-Michelson gravitational free mass interferometer is considered for a registration of the low frequency-Earth gravity gradients. A variation of the Earth gravity force vector cause the corresponding misalignment of the interferometer mirrors thus providing information about the Earth gravity field. Gravitational interferometer with suspended mirrors provides a unique possibility to measure a relative angle variations between two "plumb lines" (gravity force vectors) separated by the large distance 3 / 4 km. So at very low frequencies the set up presents a long based angular gravity gradiometer for registering global geodynamics through the surface gravity gradient. A possibility of measuring the geophysical phenomena resulted in gravity field variations (core movements, Earth free oscillations, tidal harmonics, Earth rotation variations, etc.) is discussed and technical requirements for the set up optical elements are formulated. Comparison with conventional geophysical devices is carried out. Estimates of the basic instrumental and seismic noises limiting the sensitivity at low frequency (in the quasi-static regime) are discussed briefly. These estimates show that there is a hope for measurement of the gravitational angular perturbation of the mirrors at the level of 10~(-12)/10~(-13) rad for the observation time about several hours. The possibility of arm signals reconstruction in the presence of recycling mirror is demonstrated. The auxilliary optical system for precise justification between up-down movements and tilts of the end spherical mirrors is considered. The requirements on the stability of laser system are discussed.
机译:考虑使用Fabry-Perot-Michelson重力自由质量干涉仪来记录低频-地球重力梯度。地球重力矢量的变化会引起干涉仪镜的相应失准,从而提供有关地球重力场的信息。带有悬挂镜的引力干涉仪提供了一种独特的可能性,可测量相距3/4 km的较大距离的两条“铅垂线”(重力矢量)之间的相对角度变化。因此,在极低的频率下,该装置提供了一个基于长角的重力重力梯度仪,用于通过表面重力梯度记录全球地球动力学。讨论了测量由于重力场变化(岩心运动,地球自由振荡,潮汐谐波,地球自转变化等)而导致的地球物理现象的可能性,并提出了设置光学元件的技术要求。与常规地球物理设备进行了比较。简要讨论了限制低频灵敏度的基本仪器噪声和地震噪声的估计(在准静态状态下)。这些估计表明,对于约几小时的观测时间,有希望在10〜(-12)/ 10〜(-13)rad的水平上测量反射镜的重力角摄动。演示了在存在回收镜的情况下重建手臂信号的可能性。考虑了辅助光学系统,用于在端部球面镜的上下运动和倾斜之间精确调整。讨论了对激光系统稳定性的要求。

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