一种简单的高精度外推Sat-AIS系统性能的方法

E. Re, V. Boissinot, A. Ginesi, C. Tobehn
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引用次数: 5

摘要

由于用户的推动以及正在进行的各种机构和私人倡议,SAT-AIS正在获得动力。系统性能表征是系统设计的中心任务,因为星座必须有效地大小以满足用户需求。然而,由于系统的复杂性,通常由近地轨道星座中的10多颗卫星组成,当采用完整的处理方法时,这种表征可能非常耗时。本文提出了一种基于星座卫星探测技术部分特征的SAT-AIS星座系统性能外推方法。由于欧空局在2011年底至2012年初进行的比较绩效评估(CPA)框架内收集了有价值的数据,因此对外推技术进行了广泛的验证。由于这些数据,该方法在不同系统的全处理模拟中进行了测试,并被证明是非常准确的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A simple high precision method for extrapolating Sat-AIS system performance
SAT-AIS is gaining momentum thanks to the push of the users and to the different ongoing institutional and private initiatives. System performance characterization is a central task for the system design, as the constellation has to be sized efficiently to meet the user requirements. However due to the complexity of the systems, often composed of more than 10 satellites in a LEO constellation, this characterization can be extremely time consuming when a full processing approach is undertaken. This paper presents a method for extrapolating the system performance of a SAT-AIS constellation based on a partial characterization of the detection technology onboard the satellites of the constellation. An extensive validation of the extrapolation technique was carried out thanks to the valuable data collected by ESA in the frame of the Comparative Performance Assessment (CPA) carried out between the end of 2011 and beginning of 2012. Thanks to these data, the method was tested against full processing simulations for different systems, and was proven to be extremely accurate.
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