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General Relativity Measurements in the Field of Earth with Laser-Ranged Satellites: State of the Art and Perspectives

机译:激光测距卫星在地球领域的广义相对论测量:最新进展和观点

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Recent results of the LARASE research program in terms of model improvements and relativistic measurements are presented. In particular, the results regarding the development of new models for the non-gravitational perturbations that affect the orbit of the LAGEOS and LARES satellites are described and discussed. These are subtle and complex effects that need a deep knowledge of the structure and the physical characteristics of the satellites in order to be correctly accounted for. In the field of gravitational measurements, we present a new measurement of the relativistic Lense-Thirring precession with a 0.5 % precision. In this measurement, together with the relativistic effect we also estimated two even zonal harmonics coefficients. The uncertainties of the even zonal harmonics of the gravitational field of the Earth have been responsible, until now, of the larger systematic uncertainty in the error budget of this kind of measurements. For this reason, the role of the errors related to the model used for the gravitational field of the Earth in these measurements is discussed. In particular, emphasis is given to GRACE temporal models, that strongly help to reduce this kind of systematic errors.
机译:提出了LARASE研究计划在模型改进和相对论测量方面的最新成果。特别是,描述和讨论了有关影响LAGEOS和LARES卫星轨道的非重力微扰新模型的开发结果。这些是微妙而复杂的影响,需要对卫星的结构和物理特性有深入的了解,才能正确地加以考虑。在重力测量领域,我们提出了相对论的Lense-Thirring进动的新测量,精度为0.5%。在此测量中,连同相对论效应,我们还估计了两个偶数的纬向谐波系数。迄今为止,地球重力场的偶数纬向谐波的不确定性一直是这类测量误差预算中较大的系统不确定性的原因。因此,在这些测量中讨论了与用于地球重力场的模型有关的误差的作用。特别是,重点是GRACE时间模型,该模型强烈有助于减少此类系统错误。

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