皮卫星姿态估计及粗太阳敏感器标定算法研究

粗太阳敏感器是一种由多个光电池片配置组成的模拟式太阳敏感器,它结构简单、资源要求少,在皮卫星平台应用较为广泛。光电池光伏输出特性是粗太阳敏感器测量的基础,使用余弦关系近似等效会引入很大的误差。通过实际测试和深入分析,建立了更高精度的粗太阳敏感器输出特性等效数值模型,并以此为基础,推导了卫星姿态估计及粗太阳敏感器标定的联合在轨实时算法。算法采用多级耦合结构,由1个扩展卡尔曼滤波器(EKF)和6个卡尔曼滤波器组成,同时估计卫星姿态、卫星角速度以及卫星6个面共30个标定参数。仿真表明,和常规的EKF姿态估计算法相比,联合算法的运算量只增加了一半,而估计精度却提高了一个量级。     

微小卫星剩磁在轨标定技术研究

 基于微小卫星姿态确定系统常采用无陀螺配置方案，克服环境干扰力矩的影响并提高微小卫星姿态确定的精度是此类姿态确定系统的关键。分析了星上稳定剩余磁场对无陀螺微小卫星姿态确定的干扰机理，建立了卫星剩余磁矩与磁强计偏置标定模型。以磁强计、太阳敏感器作为姿态敏感器件，并采用扩展卡尔曼滤波器实现标定算法，为无陀螺磁测微小卫星消除剩磁干扰，获得高精度姿态估计提供了一种新方法。仿真结果表明：该方法能准确估计卫星剩余磁矩与磁强计偏置，磁强计偏置的标定精度在1 nT左右，剩余磁矩的标定精度为0.000 1 A·m²量级，有效消除了剩磁对无陀螺卫星姿态确定的影响，显著提高了姿态确定精度，滤波器能在500 s内收敛。     

基于UKF算法的航天器自主导航研究

针对卫星上配备的多种姿态敏感器，进行了导航方案的设计，利用姿态敏感器的测量信息实现轨道参数的估计。通过UKF(Unscented Kalman Filter)算法研究了卫星的自主导航问题，较传统的扩展卡尔曼滤波方法(EKF)简化了计算过程。数值仿真结果验证了该导航算法的优越性。     

自适应UKF在北斗定位算法中的应用

北斗导航系统发展日益成熟，介绍了北斗定位解算与GPS解算的差异，针对扩展Kalman滤波(Extended Kalman Filter，EKF）算法在北斗解算过程中容易引入非线性误差，无迹Kalman滤波(Unscented Kalman Filter，UKF）算法受初值和系统噪声影响较大问题，提出了一种自适应无迹Kalman滤波(Adaptive Unscented Kalman Filter，AUKF）北斗定位解算算法。该算法利用观测残差信息构建自适应渐消矩阵，消除量测噪声异常带来的影响，同时提高了滤波精度。实验表明，与EKF和UKF定位解算算法相比，AUKF算法在定位精度和对系统噪声鲁棒性方面都有所提高，是一种可靠稳定的北斗定位算法。     

无源定位跟踪滤波算法研究及仿真分析

首先介绍了几种无源定位跟踪滤波算法原理,包括扩展卡尔曼滤波（EKF）,无迹卡尔曼滤波器（EKF）,交互多模型滤波器（IMM）;然后通过建立几种不同模型来对每一种滤波算法进行仿真,依据仿真图形和误差结果对滤波算法进行分析,从而实现不同滤波模型根据目标运动状态进行监视和切换,这对无源定位跟踪算法精度的提高和实际应用有很大的...     

一种星敏感器-陀螺组合定姿的实时在轨标定方法

研究了一种星敏感器一陀螺组合定姿方式中的姿态敏感器误差的实时在轨标定方法。首先,选择直观的欧拉角作为姿态描述参数,根据星敏感器和陀螺的测量原理建立星敏感器一陀螺在轨标定的测量方程和状态方程,并以此建立数学模型。其次,采用简单高效的EKF（ExtendedKalmanFilter,扩展卡尔曼滤波）作为估值算法,进行了在轨标定数值仿真。对于航天器姿态定向中出现的姿态角和星敏感器安装角之间的耦合问题,通过在特定姿态通道上施加简单姿态机动实现了解耦。数值结果表明,该实时在轨标定方法,尤其是所提出的姿态角和星敏感器安装角解耦策略,可以实现对航天器姿态的实时精确估计以及对星敏感器安装误差、陀螺常值漂移和相关漂移等误差的实时在轨标定。该方法可用于航天器姿态测量设备的实时在轨标定和航天器姿态的高精度实时确定。     

UKF方法及其在方位跟踪问题中的应用

采用UKF(Unscented Kalman Filter)方法处理了平面内地面站对目标的方位跟踪的估计问题。目标的位置和速度由选定的高斯分布采样点来近似，在每个更新过程中，采样点随着状态方程传播并随着非线性测量方程变换，由此不但得到目标位置和速度的均值及较高的计算精度，而且避免了对非线性方程的线性化过程。仿真结果表明，UKF方法比传统的扩展卡尔曼滤波(EKF)算法有更高的估计精度，并能有效地克服非线性严重时，方位跟踪问题中很容易出现的滤波发散问题。     

航空发动机气路故障诊断的平方根UKF方法研究

设计了适用于双轴涡扇发动机健康参数估计的平方根UKF滤波算法,解决了线性卡尔曼滤波器估计结果准确性依赖于线性模型精度;常规UKF算法中由于计算误差及噪声信号影响引起误差协方差矩阵负定而导致滤波结果发散等问题.提出了根据测量残差变化改进滤波收敛速度与稳定性的方法.发动机渐变与突变故障模式下仿真结果表明,平方根UKF估计算法收敛速度快,稳定性强,精度高,是一种有效的发动机气路部件健康参数估计与故障诊断方法.      

基于改进UKF的小卫星磁测定轨方法

针对小卫星设计简单、功耗低的特点,提出一种利用三轴磁强计测量信息实现卫星磁测自主定轨的方法。为了提高自主定轨的计算效率,采用基于球体单形ε点采样的改进UKF(Unscented Kalman Filter)作为处理自主定轨的滤波算法。最后对这种定轨方法进行了仿真试验,结果表明,该滤波算法能有效保证收敛的速度和定轨精度。     

基于联邦UKF的多机协同无源定位

为提高多机协同无源定位的精度和速度,同时满足应用性强的要求,提出了基于UKF(Unscented Kalman Filter)联邦滤波算法的纯方位无源定位技术。核心思想是利用联邦滤波算法去解决各子滤波器滤波结果的全局最优融合问题;利用UKF算法去消除非线性状态方程或量测方程中的高斯噪声,从而实现多机协同对目标辐射源的高精度无源定位。仿真结果表明,该算法可行性强,定位精度高、速度快,具有很高的应用价值。     

近地卫星磁测自主定轨及原型化

利用三轴磁强计的测量信息可实时地确定卫星轨道。采用扩展卡尔曼滤波作为处理磁测自主定轨问题的滤波算法．并以地磁场强度幅值作为测量值，建立了近地卫星磁测自主定轨的数学模型。在数学模型的基础上实现了基于PC机、dSPACE一体化系统的原型化(Prototyping)实验。该原型化实验对磁测自主定轨的方案、理论、算法及实时运行特性做了进一步的验证。     

Angular velocity determination of spinning solar sails using only a sun sensor

The direction of the sun is the easiest and most reliable observation vector for a solar sail running in deep space exploration. This paper presents a new method using only raw measurements of the sun direction vector to estimate angular velocity for a spinning solar sail. In cases with a con-stant spin angular velocity, the estimation equation is formed based on the kinematic model for the apparent motion of the sun direction vector;the least-squares solution is then easily calculated. A performance criterion is defined and used to analyze estimation accuracy. In cases with a variable spin angular velocity, the estimation equation is developed based on the kinematic model for the apparent motion of the sun direction vector and the attitude dynamics equation. Simulation results show that the proposed method can quickly yield high-precision angular velocity estimates that are insensitive to certain measurement noises and modeling errors.     

A new method of single celestial-body sun positioning based on theory of mechanisms

Considering defects of current single celestial-body positioning methods such as discon-tinuity and long period, a new sun positioning algorithm is herein put forward. Instead of tradi-tional astronomical spherical trigonometry and celestial coordinate system, the proposed new positioning algorithm is built by theory of mechanisms. Based on previously derived solar vector equations (from a C1R2P2 series mechanism), a further global positioning method is developed by inverse kinematics. The longitude and latitude coordinates expressed by Greenwich mean time (GMT) and solar vector in local coordinate system are formulated. Meanwhile, elimination method of multiple solutions, errors of longitude and latitude calculation are given. In addition, this algo-rithm has been integrated successfully into a mobile phone application to visualize sun positioning process. Results of theoretical verification and smart phone’s test demonstrate the validity of pre-sented coordinate’s expressions. Precision is shown as equivalent to current works and is acceptable to civil aviation requirement. This new method solves long-period problem in sun sight running fix-ing and improves applicability of sun positioning. Its methodology can inspire development of new sun positioning device. It would be more applicable to be combined with inertial navigation systems for overcoming discontinuity of celestial navigation systems and accumulative errors of inertial nav-igation systems.     

水下重力匹配定位算法综述

随着重力测量和水下导航技术的发展,惯性/重力匹配导航技术因其精度高、自主性强和航时长等优点,已成为水下自主导航的重要研究方向。惯性/重力匹配导航系统主要由惯性导航系统、重力实时测量、海洋重力场背景图和重力匹配定位算法构成。重力匹配定位算法通过将实时测量的重力异常值与构建的重力场背景图进行匹配,得到水下运载体当前时刻的位置信息,是惯性/重力匹配导航技术的核心。本文详细介绍了重力匹配算法的技术发展现状,重点分析了具有代表性的ICCP算法、SITAN算法、矢量匹配算法及其衍生算法,并对惯性/重力匹配水下自主导航技术的未来发展进行了展望。     

Design of on-board calibration methods for a digital sun sensor based on Levenberg–Marquardt algorithm and Kalman filters

Digital sun sensor is one of the most important sensors used in the Attitude Determination System (ADS) of the satellite. Due to the harsh environmental conditions that exist in the space, various distortions may occur in the sun sensor optical system that lead to the reduced accuracy of this equipment. So, it is necessary to recalibrate the optical parameters of the aforementioned sensors. For this purpose, first a novel attitude independent error model is proposed for the SS-411 sun sensor that includes the central point of the CCD array, installation error, filter thickness and sensor misalignment. So, the mutual interfaces between the sensor parameters are considered in the developed model. In order to extract the sensor parameters, a nonlinear optimization technique called the Levenberg–Marquardt is applied to the developed model as a batch algorithm. In addition, the Extended Kalman Filter (EKF) and the Unscented Kalman Filter (UKF) have been utilized as sequential strategies. It will be shown that by considering a worst case of variation amount for sensor parameters, an accuracy improvement of about 17° is achieved by the developed calibration algorithms. Comparison between the developed algorithms represents that UKF has higher accuracy, shorter time convergence but higher computational load.     

车载里程仪参数的实时标定方法

针对里程仪输出的速度(或位置增量),其参数标定误差残差是影响定位定向系统性能的关键因素,传统里程仪参数标定方法需在行车过程中设置精确标志点,且有行驶路线受限的缺点,因此提出一种基于速度量测的定位定向系统误差实时估计和补偿方法.该方法将里程仪刻度系数误差、安装误差残差纳入状态变量进行实时估计并补偿,将惯性导航系统输出的速度与里程仪输出的速度进行对比,构建量测方程.设计跑车试验对该方法进行验证,结果表明该车载里程仪参数的实时标定方法,仅需要在里程仪安装在车辆上后,导航系统做一次正常罗经对准并转惯性/里程仪组合导航模式,在车辆正常行驶过程中,即可自动标定出里程仪参数误差,具有自主、灵活简便、精度高的特点,同时提高了惯性/里程仪组合导航系统定位精度.     

基于直线成像特征的视觉测量系统综合标定方法

针对视觉测量系统存在复杂系统误差的特点,提出一种基于直线成像特征的系统综合标定方法,有效地保证了测量精度.该方法通过对1等量块的平行直线边缘提取,建立量块边缘空间物点位置和像点位置的原始对应关系,利用量块边缘的理想直线特征,通过统计计算对测量系统进行综合标定,建立描述空间物点位置和像点位置的相互对应关系的二元三次标定函数.对在测量范围内不同方位的量块进行多次测量,表明使用这种标定方法标定的视觉测量系统的测量精度能够达到.     

多传感器组合导航系统的多尺度异步信息融合算法

首先,将状态方程采用数据块变换的方式得到新的状态块方程,并将量测方程表达为数据块的形式;然后,将量测向量进行多层小波变换以得到新的量测向量,结合状态块方程进行卡尔曼滤波;最后,利用异步贯序滤波的方法,建立了基于全局的最优估计值。将上述算法应用于GPS/SST/高度表/SINS多组合导航系统,仿真结果表明:相对于单一尺度的异步滤波算法,该算法可明显地提高系统的滤波精度。     

On-orbit real-time magnetometer bias determination for micro-satellites without attitude information

Due to the disadvantages such as complex calculation, low accuracy of estimation, and being non real time in present methods, a new real-time algorithm is developed for on-orbit magnetometer bias determination of micro-satellites without attitude knowledge in this paper. This method uses the differential value approach. It avoids the impact of quartic nature and uses the iterative method to satisfy real-time applications. Simulation results indicate that the new real-time algorithm is more accurate compared with other methods, which are also tested by an experiment system using real noise data. With the new real-time algorithm, a magnetometer calibration can be taken on-orbit and will reduce the demand for computing power effectively.