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ENHANCED ESTIMATION OF NEUTRAL THERMOSPHERIC DENSITIES WITH MICROSCOPE

机译:用显微镜增强中性热椎间密度的估计

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After more than 15 years of planning, developing, building, and testing, the French MICROSCOPE satellite was finally launched on 25th of April 2016. It is the first satellite testing the validity of the Weak Equivalence Principle up to an accuracy of the E?tv?s parameter η of 1E-15. The payload comprises two differential accelerometers, each containing two test masses. Due to the drag-free system non-gravitational disturbances are cancelled thus allowing the test masses to follow a pure gravitational orbit. An initial evaluation of the first science data has already led to an improvement of the determination of the E?tv?s parameter η by one order of magnitude compared to the best values achieved by torsion balance experiments. However, for calibration purposes and for identifying residual couplings between test mass motion and external perturbations, simulations of the satellite system and the mission are necessary. We present our approach of a high precision analysis of the non-gravitational perturbations acting on MICROSCOPE by means of the High Performance satellite dynamics Simulator (HPS). This simulation tool is being developed by the Center of Applied Space Technology and Microgravity (ZARM) at the University of Bremen, Germany, in cooperation with the Institute of Space Systems (DLR-IRS) of the German Aerospace Center. Here the calculation of the non-gravitational effects includes the specifics of spacecraft geometry and illumination conditions thus allowing for highest modeling accuracy. Furthermore, we introduce an application for MICROSCOPE which can be used for any spacecraft employing high performance accelerometers to conduct aeronomy experiments. By accurately modeling all non-gravitational effects we achieve subsequent estimates of all accelerations acting on the craft. When the satellite is operated in non-drag free mode and other dynamical effects derived from the rotational behaviour are known, we can subtract these estimated values from the acc
机译:经过15年多的规划,开发,建筑和测试,法国显微镜卫星终于在2016年4月25日推出。它是第一个测试弱等效原则的有效性的卫星测试,这是E的准确性?S参数η为1E-15。有效载荷包括两个差分加速度计,每个差分加速度计包含两个测试质量。由于无阻力系统,取消了不重力的扰动,从而允许测试质量遵循纯的重力轨道。与通过扭转平衡实验所实现的最佳值相比,对第一科学数据的初始评估已经导致了改善了一个数量级的一个数量级的确定。然而,为了校准目的,并且用于识别测试质量运动和外部扰动之间的残留联轴器,需要卫星系统的模拟和任务。我们借助于高性能卫星动力学模拟器(HPS),我们介绍了对显微镜作用的非重力扰动的高精度分析。该模拟工具是由德国不来梅大学的应用空间技术和微普理(ZARM)开发的,与德国航空航天中心的太空系统(DLR-IRS)合作。这里计算非重力效应包括航天器几何形状和照明条件的具体细节,从而允许最高的建模精度。此外,我们介绍了一种用于显微镜的施用,该显微镜可用于采用高性能加速度计进行航空实验的任何航天器。通过准确地建模所有非引力效应,我们实现了对工艺上所有加速度的后续估计。当卫星在非拖动自由模式下操作时,已知从旋转行为导出的其他动态效果,我们可以从ACC中减去这些估计值

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