考虑未知飞轮摩擦力矩的航天器姿态跟踪鲁棒自适应控制

针对存在未知飞轮摩擦力矩和外干扰力矩情况下的姿态跟踪问题,提出并分析一种鲁棒自适应姿态控制律。姿态控制律采用一种间接处理未知飞轮摩擦力矩和外干扰力矩的方法。该方法并不直接关注未知摩擦力矩和外干扰力矩本身,而是关注其界,并用其进行控制器设计。最后基于Barbalat引理证明所得闭环系统的稳定性,并给出数值仿真结果。仿真结果校验了所提方法的有效性。     

平面遮挡分析法及其在航天器气动力矩分析中的应用

针对空间站等复杂构型航天器迎流面积和气动力矩的快速分析问题,提出一种平面遮挡分析法。该方法在与迎流垂直的方向上,选定一个二维投影平面进行航天器组成单元的划分和二维外形信息的定义;通过标志符、差值函数及相关的单元外形边界搜索规则定义和操作,实现迎流面积和遮挡面积的计算。平面遮挡分析法减少了遮挡分析所需使用的航天器外形信息维度,可以提高遮挡分析的效率。然后给出基于该平面遮挡分析法对迎流面积和压心位置进行计算的数学模型,对使用的气动力矩分析模型进行说明。以一个非对称构型的空间站为例,对相应的迎流面积和气动力矩进行仿真计算和对比验证。结果表明,平面遮挡分析法具有较为明显的计算时间优势,同时具备较高的计算精度。     

两轮升压式空气动压轴承涡轮冷却器起浮压力计算

通过分析两轮升压式空气动压轴承涡轮冷却器的起浮原理,建立了计算起浮压力的方法.按照该方法编制程序计算了某型涡轮冷却器在不同条件下的起浮压力,计算结果与试验实测数据吻合较好,说明计算方法具有较高准确度.通过计算和分析可以看到涡轮出口背压和轴承预紧对轴承起浮影响较大,背压越低则起浮压力越低;轴承预紧力越大则起浮压力越高.      

螺纹结构力矩及其衰退机理分析

阐述了得出螺栓拧紧力矩的方法,结合预紧力和预紧力矩之间的关系,给出其理论方程和实验方程,分析了预紧力、螺纹摩擦转矩和螺母支承面摩擦转矩三者的分配情况。以此为基础,从结构变形与应力释放、材料表面摩擦力变化等方面对力矩衰退的原因进行了初步分析,并提出设定拧紧力矩安全系数和定期校核拧紧的措施,供螺纹结构设计及其使用维护参考。     

滚动轴承摩擦力矩的乏信息模糊预报

滚动轴承摩擦力矩的波动具有不确定性,属于概率分布与趋势规律都未知的乏信息系统.这阻碍了对轴承摩擦力矩的小样本分析与总体把握.为此,以模糊集合理论为基础,从小样本入手,建立了航天轴承摩擦力矩参数的经验概率密度函数及其模糊预报模型,并对摩擦力矩的均值上界和最大值上界进行预报.对HKTA和HKTB两种轴承摩擦力矩参数的试验研究表明,在99%～100%置信水平下,预报结果与试验结果之间的误差很小,最大绝对误差仅为0.081 1个设定单位,最大相对误差仅为10.165%,可以满足航天工程的要求.      

Impact of the orbital eccentricity on the attitude performance before and after the deorbiting phase for Alsat-1

Due to the presence of periodic forcing terms in the gravity gradient torque, orbit eccentricity may produce large response for the roll, yaw and pitch angles. This paper investigates the influence of the orbit eccentricity on the performance of the attitude determination and control subsystem (ADCS) pointing of passive Low Earth Orbit (LEO) satellites stabilized by a gravity gradient boom or having long appendages before and after the deorbiting operation. The contribution of this work is twofold. First, the satellite attitude dynamics and kinematics are modeled by introducing the orbit eccentricity in the equations of motion of a LEO satellite in order to provide the best scenario in which satellite operators can keep the nominal functionality of LEO satellites with a gravity gradient boom after the deorbiting operation. Second, a Quaternion-based Extended Kalman Filter (EKF) is analyzed when the orbit eccentricity is considered in order to determine the influence of this disturbance on the convergence and stability of the filter. The simulations in this work are based on the true parameters of Alsat-1 which is a typical LEO satellite stabilized by a gravity gradient boom. The results show that the orbit eccentricity has a big influence on the pointing system accuracy causing micro-vibrations that affect the geocentric pointing particularly after the deorbiting phase. In this case, satellites have no orbital correction option. The Quaternion-based Extended Kalman Filter analyzed in this paper, achieved satisfactory results for eccentricity values less than 0.4 with respect to pointing system accuracy. However, singularities were observed for eccentricity values greater than 0.4.     

改进的参考电压矢量获取方法

针对基于空间矢量调制的永磁同步电机直接转矩控制方法中,参考电压矢量获取涉及电机参数,而电机参数的变化又导致预测结果不可靠的问题,提出了一种不依赖电机参数的参考电压矢量获取方法。通过对转矩误差以及定子磁链幅值误差进行PI控制,对其输出量分别分配一定的权重,用其绝对值的加权,作为参考电压矢量幅值的控制量,用其比值作为确定参考电压矢量相对于定子磁链矢量角度偏差的依据。仿真结果表明,该方法能很好克服电机参数变化造成的影响,从而试验验证了该方法的有效性。     

An estimation of Envisat’s rotational state accounting for the precession of its rotational axis caused by gravity-gradient torque

The rotational state of Envisat is re-estimated using the specular glint times in optical observation data obtained from 2013 to 2015. The model is simplified to a uniaxial symmetric model with the first order variation of its angular momentum subject to a gravity-gradient torque causing precession around the normal of the orbital plane. The sense of Envisat’s rotation can be derived from observational data, and is found to be opposite to the sense of its orbital motion. The rotational period is estimated to be $(120.674\pm 0.068)·\exp \left((4.5095\pm 0.0096)\times {10}^{-4}·t\right)\text{s}$, where t is measured in days from the beginning of 2013. The standard deviation is 0.760?s, making this the best fit obtained for Envisat in the literature to date. The results demonstrate that the angle between the angular momentum vector and the negative normal of the orbital plane librates around a mean value of $8.53°\pm 0.42°$ with an amplitude from about $0.7°$ (in 2013) to $0.5°$ (in 2015), with the libration period equal to the precession period of the angular momentum, from about 4.8?days (in 2013) to 3.4?days (in 2015). The ratio of the minimum to maximum principal moments of inertia is estimated to be $0.0818\pm 0.0011$, and the initial longitude of the angular momentum in the orbital coordinate system is $40.5°\pm 9.3°$. The direction of the rotation axis derived from our results at September 23, 2013, UTC 20:57 is similar to the results obtained from satellite laser ranging data but about $20°$ closer to the negative normal of the orbital plane.     

空间太阳能电站的准对日定向姿态

针对空间太阳能电站的俯仰姿态运动,提出一种能追踪太阳运动的准对日定向(QSP)姿态方案。此方案的太阳能电池阵列在万有引力梯度力矩的作用下,始终在垂直于太阳光的方向附近作幅值约为18.8°的振动,且几乎不需要姿态控制力矩。准对日定向姿态方案解决了大型太阳能电池阵列对日定向所需的巨大俯仰姿态控制力矩问题。准对日定向姿态的发电效率为对日定向姿态的97.3%,对Abacus空间太阳能电站而言每年可节省燃料约36791 kg。通过数值方法得到了准对日定向姿态的精确初始条件。随后,设计了比例-微分控制器,保证了系统存在初始姿态误差的条件下收敛到准对日定向姿态。最后研究了轨道、姿态和结构振动对准对日定向姿态的影响,并发现准对日定向姿态下的结构振动幅值比对日定向姿态减小约40倍。     

基于高功率因数控制的永磁同步电机无电解电容驱动系统控制策略

永磁同步电机无电解电容驱动系统因其成本与寿命的优势,在白色家电领域逐步得到广泛的应用。然而,由于使用小容量的薄膜电容取代大容量的电解电容,母线电压会以两倍工频波动,在母线电压处于波谷时,逆变器输出电压容易饱和,导致控制性能恶化,网侧电流畸变。因此,提出了一种基于高功率因数控制的转矩控制环和电压矢量修正策略,能够有效提升网侧功率因数,抑制网侧电流谐波并符合IEC 6100032标准。该算法的有效性通过仿真得以验证。