用LAGEOS、LAGEOS II和Ajisai激光测距卫星测试广义相对论

Q4 Earth and Planetary Sciences
L. Iorio
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引用次数: 20

摘要

卫星激光测距(SLR)在过去几年中所达到的精度允许通过人造卫星测量爱因斯坦广义相对论所预测的地球引力场的微小特征。通过分析LAGEOS和LAGEOS‡U的轨道残差的合适组合,目前正在测量测试体轨道的重力磁拖拽。本实验误差的下界为12.92%。这是由于在系统误差的最重要来源——地球势的均匀纬向谐波中建模错误造成的。类似的方法也可以用于测量地球场的相对论性引力电心心移,由于均匀的纬向谐波,系统相对误差的下界为6.59 μ ~10-3。将测距数据纳入日本无源大地测量卫星“Ajisai”将使这一限制分别提高到10.78%和8.1 μ ~10-4,并可提高PPN参数ƒA和ƒA的确定精度。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Testing General Relativity with LAGEOS, LAGEOS II and Ajisai laser-ranged satellites
The accuracy reached in the past few years by Satellite Laser Ranging (SLR) allows for measuring even tiny features of the Earth's gravitational field predicted by Einstein's General Relativity by means of artificial satellites. The gravitomagnetic dragging of the orbit of a test body is currently under measurement by analyzing a suitable combination of the orbital re siduals of LAGEOS and LAGEOS ‡U. The lower bound of the error in this experiment amount to 12.92%. It is due to the mismodeling in the even zonal harmonics of the geopotential which are the most important sources of systematic error. A similar approach could be used in order to measure the relativistic gravitoelectric pericenter shift in the field of the Earth with a lower bound of the systematic relative error of 6.59~10-3 due to the even zonal harmonics as well. The inclusion of the ranging data to the Japanese passive geodetic satellite Ajisai would im prove such limits to 10.78% and 8.1~10-4 respectively and would allow to improve the accu racy in the determination of the PPN parameters ƒA and ƒA.
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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)
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