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利用 TRIAD 和 MEKF 方法对 UVSQ-SAT 立方体卫星进行在轨姿态确定。

In-Orbit Attitude Determination of the UVSQ-SAT CubeSat Using TRIAD and MEKF Methods.

机构信息

Université de Versailles Saint-Quentin-en-Yvelines, Université Paris-Saclay, Sorbonne Université (SU), CNRS, LATMOS, 11 Boulevard d'Alembert, 78280 Guyancourt, France.

ACRI-ST CERGA, 10 Avenue Nicolas Copernic, 06130 Grasse, France.

出版信息

Sensors (Basel). 2021 Nov 5;21(21):7361. doi: 10.3390/s21217361.

Abstract

Ultraviolet and infrared sensors at high quantum efficiency on-board a small satellite (UVSQ-SAT) is a CubeSat dedicated to the observation of the Earth and the Sun. This satellite has been in orbit since January 2021. It measures the Earth's outgoing shortwave and longwave radiations. The satellite does not have an active pointing system. To improve the accuracy of the Earth's radiative measurements and to resolve spatio-temporal fluctuations as much as possible, it is necessary to have a good knowledge of the attitude of the UVSQ-SAT CubeSat. The attitude determination of small satellites remains a challenge, and UVSQ-SAT represents a real and unique example to date for testing and validating different methods to improve the in-orbit attitude determination of a CubeSat. This paper presents the flight results of the UVSQ-SAT's attitude determination. The Tri-Axial Attitude Determination (TRIAD) method was used, which represents one of the simplest solutions to the spacecraft attitude determination problem. Another method based on the Multiplicative Extended Kalman Filter (MEKF) was used to improve the results obtained with the TRIAD method. In sunlight, the CubeSat attitude is determined at an accuracy better than 3° (at one σ) for both methods. During eclipses, the accuracy of the TRIAD method is 14°, while it reaches 10° (at one σ) for the recursive MEKF method. Many future satellites could benefit from these studies in order to validate methods and configurations before launch.

摘要

高量子效率的紫外和红外传感器在小型卫星(UVSQ-SAT)上,是一颗专门用于观测地球和太阳的立方卫星。该卫星自 2021 年 1 月以来一直在轨道上运行。它测量地球的出射短波和长波辐射。卫星没有主动指向系统。为了提高地球辐射测量的精度,并尽可能地解决时空波动问题,需要很好地了解 UVSQ-SAT 立方卫星的姿态。小卫星的姿态确定仍然是一个挑战,UVSQ-SAT 是迄今为止一个真实而独特的例子,用于测试和验证不同的方法,以提高立方卫星的在轨姿态确定。本文介绍了 UVSQ-SAT 姿态确定的飞行结果。使用了三轴姿态确定(TRIAD)方法,它是解决航天器姿态确定问题的最简单方法之一。另一种基于乘法扩展卡尔曼滤波器(MEKF)的方法被用来改进 TRIAD 方法的结果。在阳光照射下,两种方法都能以优于 3°(一个标准差)的精度确定立方卫星的姿态。在日食期间,TRIAD 方法的精度为 14°,而递归 MEKF 方法的精度为 10°(一个标准差)。许多未来的卫星都可以从这些研究中受益,以便在发射前验证方法和配置。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/1292/8588341/2abdf58dc6df/sensors-21-07361-g001.jpg

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