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Estimation of Interplanetary Magnetic Field for attitude control of small spacecraft in deep space missions

机译:太空飞行中小航天器姿态控制的星际磁场估计

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In recent years, interplanetary space missions using nano-spacecraft have been introduced. However, due to its limitation,traditional attitude methods cannot be used in nano-spacecraft. In order to handle this problem, a new method of attitudecontrol using torque generated from magnetic torquer (MTQ) and Interplanetary Magnetic Field (IMF) was introduced.This method, however, depend heavily on getting the information of the IMF, which is very difficult to obtain usingmagnetic sensor. In this paper, a new method to obtain the IMF information using actuator is introduced. The method isfirst tested using Unscented Kalman Filter (UKF) under ideal environment and then improved to work under environmentwith disturbance using Adaptive Unscented Kalman Filter (AUKF). In conclusion, by using the proposed method it ispossible to estimate the IMF at 0.1 nT order error even under solar disturbance while performing attitude control.
机译:近年来,已经引入了使用纳米航天器的行星际航天任务。但是,由于其局限性, 纳米航天器无法使用传统的姿态方法。为了解决这个问题,一种新的态度方法 引入了利用磁力转矩发生器(MTQ)和行星际磁场(IMF)产生的转矩进行控制的方法。 但是,此方法在很大程度上取决于获取IMF的信息,而使用IMF很难获得该信息。 磁性传感器。本文介绍了一种使用执行器获取IMF信息的新方法。方法是 首先在理想环境下使用无味卡尔曼滤波器(UKF)进行测试,然后进行改进以在环境下工作 使用自适应无味卡尔曼滤波器(AUKF)产生干扰。总之,通过使用所提出的方法,它是 甚至在进行姿态控制时,即使在太阳干扰下​​,也可能以0.1 nT阶次误差估算IMF。

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