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Comparison of ENVISAT's attitude simulation and real optical and SLR observations in order to refine the satellite attitude model

机译:Envisat态度模拟和真实光学和单反观测的比较,以改进卫星姿态模型

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The Astronomic Institute of the University of Bern (AIUB) in cooperation with other three partners is involved in an ESA study dedicated to the attitude determination of large spacecraft and upper stages. Two major goals are defined. First is the long term prediction of tumbling rates (e.g. 10 years) for selected targets for the future Active Debris Removal (ADR) missions. Second goal is the attitude state determination in case of contingencies, when a short response time is required between the observations themselves and the attitude determination. One of the project consortium partners, Hypersonic Technology Goettingen (HTG), is developing a highly modular software tool ?OTA to perform short- (days) to long-term (years) propagations of the orbit and the attitude motion of spacecraft in space. Furthermore, ?OTA's post-processing modules will generate synthetic measurements, e.g. light curves, SLR residuals and Inverse Synthetic Aperture Radar (ISAR) images that can be compared with the real measurements. In our work we will present the first attempt to compare real measurements with synthetic measurements in order to estimate the attitude state of tumbling satellite ENVISAT from observations performed by AIUB. We will shortly discuss the ESA project and tOTA software tool. We will present AIUB's ENVISAT attitude state determined from the SLR ranges acquired by the Zimmerwald SLR station. This state was used as the initial conditions within the ?OTA software. Consequently the attitude of satellite was predicted by using ?OTA and compared with the real SLR residuals, as well with the high frame-rate light curves acquired by the Zimmerwald 1 -m telescope.
机译:伯尔尼大学(AIUB)与其他三个合作伙伴合作的天文学研究所参与了致力于态度决定大型航天器和上阶段的ESA研究。定义了两个主要目标。首先是对未来活性碎片拆卸(ADR)任务的选定目标的翻滚率(例如10年)的长期预测。第二个目标是在偶然的情况下确定态度状态,当观察到自己和姿态决定之间需要短暂的响应时间。该项目的联盟合作伙伴之一超音速技术Goettingen(HTG)正在开发一种高度模块化的软件工具?OTA,以便在空间中的轨道和航天器态度运动的长期(几年)传播。此外,ota的后处理模块将产生合成测量​​,例如,光曲线,单反渣和逆合成孔径雷达(ISAR)图像可以与真实测量进行比较。在我们的工作中,我们将展示第一次尝试使用合成测量进行比较真实测量,以估计从AIUB进行的观察结果中估计翻滚卫星Envisat的姿态状态。我们很快将讨论ESA项目和TOTA软件工具。我们将展示AIUB的Envisat态度状态,从Zimmerwald SLR站收购的SLR范围内确定。此状态被用作?OTA软件中的初始条件。因此,通过使用Zimmerwald 1-M望远镜获取的高帧速率光曲线来预测卫星的态度,并与真实的单反渣相比。

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