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针对高动态长时间积累情况下直扩信号能量无法有效积累的问题,提出了一种基于运动补偿的二倍分组块补零(Double Block Zero Padding,DBZP)算法。首先利用Keystone变换对输入信号与本地伪码在频域相乘后的结果进行处理,消除伪码自相关峰走动;再利用分段解线调技术同时补偿掉多普勒扩展和伪码自相关峰弯曲;最后对信号进行相干积累。仿真结果表明,基于运动补偿的DBZP算法能有效地消除动态的影响,大幅减小积累损耗,进而提升捕获灵敏度。该算法能广泛应用于基于直扩信号的高动态微弱目标捕获。 相似文献
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V. I. Abrashkin M. V. Volkov K. E. Voronov A. V. Egorov A. E. Kazakova V. A. Pankratov V. V. Sazonov N. D. Semkin 《Cosmic Research》2005,43(4):280-290
An integral statistical procedure of determination of the attitude motion of a satellite using the data of onboard measurements of angular velocity vectors and the strength of the Earth’s magnetic field (EMF) is suggested. The procedure uses only the equations of kinematics of a solid body and is applicable to determining both controlled and uncontrollable motions of a satellite at any external mechanical moments acting upon it. When applying this procedure, the data of measurements of both types, accumulated during a certain interval of time, are processed jointly. The data of measuring the angular velocity are smoothed by discrete Fourier series, and these series are substituted into kinematical Poisson equations for elements of the matrix of transition from a satellite-fixed coordinate system to the orbital coordinate system. The equations thus obtained represent a kinematical model of the satellite motion. The solution to these equations (which approximate the actual motion of a satellite) is found from the condition of the best (in the sense of the least squares method) fit of the data of measuring the EMF strength vector to its calculated values. The results of testing the suggested procedure using the data of measurements of the angular velocity vectors onboard the Foton-12 satellite and measurements of EMF strengths are presented.__________Translated from Kosmicheskie Issledovaniya, Vol. 43, No. 4, 2005, pp. 295–305.Original Russian Text Copyright © 2005 by Abrashkin, Volkov, Voronov, Egorov, Kazakova, Pankratov, Sazonov, Semkin. 相似文献
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三轴稳定通信卫星在地球搜索模式下的陀螺标定 总被引:1,自引:0,他引:1
本文介绍三轴稳定通信卫星在转移轨道远地点点火前,在地球搜索模式下的陀螺标定方法和计算公式。此种陀螺标定需进行两次姿态机动,利用太阳敏感器和速率积分陀螺遥测数据标定陀螺的常值漂移。 相似文献
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经典的捷联惯导积分算法往往需要在姿态更新过程中对圆锥误差项进行精确补偿。虽然考虑了载体姿态变化的影响,但速度更新算法通常忽略了圆锥效应的作用。就圆锥误差项引起的速度误差进行了研究。指出其与陀螺角增量对速度更新的影响方式相同。在假设的线性斜坡模型条件下,利用两个连续的角增量和比力增量,详细推导了新的速度误差项的二子样更新补偿算法。在一种特殊的机动条件下,即当载体绕横轴作圆锥角振动的同时又沿立轴作同频同相的线振动,推导的二子样优化算法能够使该误差补偿项的平均性能最优。仿真结果证明该优化算法能够对新的速度误差积分项进行有效的补偿。 相似文献
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The problems of investigation and optimization of the motion of spacecraft are extensively discussed in the literature. Nevertheless, in many cases a large variety of qualitative characteristics of their motion and of the form of their trajectories are still unclear. In this paper we consider a plane equiangular acceleration of a spacecraft both in a Newtonian field and in its absence (at a large distance from the center of attraction). The general equation of a trajectory of plane acceleration is presented with the introduction of a new variable, an index of an exponent, which allows one to obtain convenient solutions at different values of the time-independent angle of inclination of the vector of thrust to the spacecraft's radius vector (i.e., when equiangular acceleration takes place). Asymptotic solutions are constructed and an interesting fact is revealed. Namely, it is shown that when the center of attraction exists or is absent, for all initial conditions the trajectories appearing at the above equiangular acceleration of a material point tend to the standard logarithmic spirals at a large distance from the center. Specifically, when the value of transverse (perpendicular to the radius vector) thrust is constant, there appears a logarithmic spiral with an angle of inclination to the radius vector equal to 35.264°. Different forms of the trajectory of equiangular acceleration of spacecraft at a low thrust are also studied. The results obtained can be useful for the investigation and choice of optimum space trajectories. 相似文献
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研究了双体卫星(DFP)对日定向姿态机动控制问题。首先分析双体卫星工作机理,建立载荷舱与平台舱姿态模型,推导磁浮机构线圈和磁钢相对距离的数学表达式。提出基于PD控制的载荷舱对日姿态机动、平台舱姿态跟踪以及两舱避碰等控制策略。在此基础上,为提高平台舱姿态跟踪速度,设计反步控制器对平台舱飞轮的动态特性进行补偿。进一步,为提高两舱协同控制性能,对传统PD控制进行改进,提出基于变增益PD控制的载荷舱姿态机动控制律,将两舱相对姿态信息包含在载荷舱对日姿态机动控制律中,有效降低了两舱碰撞风险,提高了两舱姿态机动速度。仿真结果表明,本文控制算法能有效实现双体卫星对日定向,且能避免两舱碰撞。 相似文献
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重力梯度稳定小卫星的最优主动磁控和动量轮控制 总被引:1,自引:0,他引:1
为了提高小卫星定点精度,姿态控制系统采用俯仰轴动量轮控制和三轴磁力矩控制。用四元数方法建立起卫星动力学方程和运动学方程。以响应时间和响应时间内欧拉角误差和角速率误差的平方和这两个单目标作为目标函数,以三轴的位置增益、速率增益和卸载增益为设计变量,以三轴欧极子矩不超过要求值,俯仰轴的轮动量矩不超过要求值,以及末尾响应时间内应保证欧拉角和角速率逼近控制值为约束条件,建立起卫星最优控制模型。最后,作为例子应用到小卫星姿态控制中,结果证实最优控制算法是可行有效的。与传统PD控制相比,优化后的姿态控制性能也大大提高。 相似文献
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将在线变动模糊划分的模糊控制应用在挠性结构卫星单轴气浮台全物理仿真实验中,实现挠性结构的大角度机动控制,获得了机动性能好、稳态精度高的结果。在模糊控制中,模糊集合的划分在控制过程中在线变动,自动确定模糊集合隶属函数的参数,需人工设置的控制器参数很少,只需调整一个控制能量分配参数,易于应用到实际控制过程中。 相似文献
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编队卫星相对运动描述方法综述 总被引:2,自引:0,他引:2
对于近地轨道卫星编队飞行的相对运动理论研究,可以采用的方法包括直角坐标法和 轨道要素法。利用直角坐标法得到的相对运动动力学方程可以用于编队队形控制研究,轨道 要素法能够给出相对运动的运动学描述,便于定量研究摄动影响和进行编队队形设计。分析 了直角坐标法在描述卫星长期编队飞行方面的局限性,综述了利用轨道要素描述编队卫星相 对运动的各种研究方法,包括轨道要素差法、相对轨道要素法和参照轨道要素法等。 相似文献