基于机动平台序列图像的空间飞行器定轨技术研究

针对机动观测平台单目光学成像系统的特点,在不能测定目标飞行器位置和速度的前提下,通过对成像系统与空间飞行器空间关系的分析,提出了视平均运动角速度与真平均运动角速度的概念,并构建了关于二者的约束方程,实现了基于测角数据的观测斜距的估计,从而解算出定轨所需的初始状态参数。基于观测斜距估计的轨道确定方法把对空间飞行器的定轨问题,归结为根据图像序列计算目标测角和根据测角数据确定观测斜距,解决了利用空间单目光学成像数据的定轨问题,并以高轨卫星为实例对定轨精度进行了仿真验证。     

一种应用三角内插技术的频率估计算法

Rife和Quinn等基于FFT的频率估计算法性能不够稳定,在部分频率点能获得满意的估计效果,但在其它频点估计性能恶化严重。本文将三角内插技术应用于频率估计,提出了一种新的基于FFT的频率估计算法,能够克服他们的缺点,非常适合于低信噪比条件下卫星通信信号的接收。该算法首先用FFT实现频率的粗估,再应用三角内插技术提高估计精度,最后对估计偏差进行修正,保证了估计的无偏性。仿真结果表明该算法能实现非常精确的频率估计,且估计性能不受信号频率的影响,在各频点上估计方差都非常接近克拉美劳界（CRB）,具有很低的工作门限。与时域估计算法相比,相同估计方差条件下该算法运算量低、易于实现。     

空间失效慢旋卫星视觉特征跟踪与位姿测量

空间碎片或者失效卫星往往绕其惯性主轴做自旋运动,虽然处于一种稳定状态,但是对其运动状态测量的难度相比三轴稳定目标而言又增加了许多,主要体现在复杂光场环境下和目标观测面周期性进出视场引起的特征点丢失、尺度变化和旋转变化,以及长时间连续观测引起的累积误差增大、位姿解算不收敛等难题。通过构建优化目标特征数据库,将传统测量方式中前后帧的匹配转变为当前帧与特征数据库的匹配和特征点的优化,即使中间过程帧出现了偏差仍然可以较好地跟踪后续图像帧的正确位置。在李代数空间下建立位姿向量微分扰动方程,获得测量值与估计值的残差目标函数,基于贝叶斯法则最大后验概率和李群与李代数的对指变换法则,求取位姿向量最优解。解决了李群空间下由于位姿变换矩阵不可加性而无法优化的问题,提高了连续测量过程中系统的测量精度。实验结果表明,无优化测量方法无法保证整个旋转周期的有效测量;通过增加位姿优化过程,连续稳定测量时间明显延长,针对以12（°）/s自旋运动的目标,测量稳定段误差在2°以内,旋转角速度测量误差为0.12（°）/s。     

Particle acceleration and gamma rays in solar flares: Recent observations and new modeling

Experiments on SMM, GAMMA, Yohkoh, GRANAT, Compton GRO, INTEGRAL, RHESSI and CORONAS-F satellites over the past three decades have provided copious data for fundamental research relating to particle acceleration, transport and energetics of flares and to the ambient abundance of the solar corona, chromosphere and photosphere. We summarize main results of solar gamma-astronomy (including some results of several joint Russian–Chinese projects) and try to appraise critically a real contribution of those results into modern understanding of solar flares, particle acceleration at the Sun and some properties of the solar atmosphere. Recent findings based on the RHESSI, INTEGRAL and CORONAS-F measurements (source locations, spectrum peculiarities, ³He abundance etc.) are especially discussed. Some unusual features of extreme solar events (e.g., 28 October 2003 and 20 January 2005) have been found in gamma-ray production and generation of relativistic particles (solar cosmic rays, or SCR). A number of different plausible assumptions are considered concerning the details of underlying physical processes during large flares: (1) existence of a steeper distribution of surrounding medium density as compared to a standard astrophysical model (HSRA) for the solar atmosphere; (2) enhanced content of the ³He isotope; (3) formation of magnetic trap with specific properties; (4) prevailing non-uniform (e.g., fan-like) velocity (angular) distributions of secondary neutrons, etc. It is emphasized that real progress in this field may be achieved only by combination of gamma-ray data in different energy ranges with multi-wave and energetic particle observations during the same event. We especially note several promising lines for the further studies: (1) resonant acceleration of the ³He ions in the corona; (2) timing of the flare evolution by gamma-ray fluxes in energy range above 90 MeV; (3) separation of gamma-ray fluxes from different sources at/near the Sun (e.g., different acceleration sources/episodes during the same flare, contribution of energetic particles accelerated by the CME-driven shocks etc.); (4) asymmetric magnetic geometry and new magnetic topology models of the near-limb flares; (5) modeling of self-consistent time scenario of the event.     

FX型相关处理方案及野值剔除算法

分析了甚长基线干涉测量等干涉测量技术中FX型相关处理方案存在的问题,提出了一种新的FX相关处理方案。该方案经过两次整数比特时延补偿将两站接收信号相对时延缩小到1 bit内,从而避免了相位卷绕现象的出现,同时省去了原方案中的小数比特时延补偿,接着对新方案的计算量和相关长度做了深入的分析;改进了一种野值剔除算法,使剔除过程不受相位随频率变化趋势的影响。蒙特卡洛仿真和“嫦娥二号”实测数据处理结果验证了改进的准确性和有效性。     

基于星敏感器的卫星角速度估计精度分析

重点研究星敏感器自身特性对角速度估计精度的影响,分析了星敏感器动态情况下恒星矢量测量精度,推导出恒星矢量测量误差与星像目标中心提取误差之间的关系;进而研究了最小二乘角速度估计算法的精度,得出其精度影响因素:星像目标中心提取误差、曝光时间、恒星矢量数目及相互夹角;最后以给定的星敏感器参数和实际恒星分布进行数学仿真,验证了采用星敏感器估计角速度的可行性.     

基于MLR的机动平台传感器误差配准算法

 基于固定平台传感器误差极大似然配准(MLR)算法,针对机动平台存在姿态角系统误差的问题,提出了对机动平台传感器系统误差和目标状态进行批处理离线估计的机动极大似然配准(MLRM)算法.该算法利用所有传感器对目标的量测值,通过把传感器量测向目标状态进行投影、对传感器系统误差和目标状态进行期望最大化迭代以及对目标的状态进行融合估计,最终实现量测、姿态角系统误差和目标状态的有效估计.仿真结果表明,该算法迭代收敛速度快,对系统误差估计精度高,对系统误差可观测性较低的配准环境的适应性强并且对传感器姿态角的相关性不敏感,具有很强的工程实用性.     

Phase Residual Estimations for PCVs of Spaceborne GPS Receiver Antenna and Their Impacts on Precise Orbit Determination of GRACE Satellites

In-flight phase center systematic errors of global positioning system(GPS) receiver antenna are the main restriction for improving the precision of precise orbit determination using dual-frequency GPS.Residual approach is one of the valid methods for in-flight calibration of GPS receiver antenna phase center variations(PCVs) from ground calibration.In this paper,followed by the correction model of spaceborne GPS receiver antenna phase center,ionosphere-free PCVs can be directly estimated by ionosphere-free carrier phase post-fit residuals of reduced dynamic orbit determination.By the data processing of gravity recovery and climate experiment(GRACE) satellites,the following conclusions are drawn.Firstly,the distributions of ionosphere-free carrier phase post-fit residuals from different periods have the similar systematic characteristics.Secondly,simulations show that the influence of phase residual estimations for ionosphere-free PCVs on orbit determination can reach the centimeter level.Finally,it is shown by in-flight data processing that phase residual estimations of current period could not only be used for the calibration for GPS receiver antenna phase center of foretime and current period,but also be used for the forecast of ionosphere-free PCVs in future period,and the accuracy of orbit determination can be well improved.     

民用机场快速出口滑行道位置优化

位置合理的快速出口滑行道可有效提高跑道容量。通过提出候选出口最优位置假设,证明了跑道快速出口位置是一个候选最优位置的自然有限集。介绍了不同机型跑道占有时间的计算方法,并以最小加权跑道占用时间为目标函数．建立了确定最优出口位置的数学模型。并针对该模型提出了基于时间多项式的动态规划算法,给出了快速出口滑行道的定位计算方法。以大连机场为例,计算得到了该机场快速出口滑行道的合理数量与位置.     

一种多标校源的高轨伴星时差频差定位算法

针对高轨伴星时差频差无源定位系统中卫星位置、速度、时差和频差等参数的测量系统误差严重影响定位精度的问题,提出了一种基于四个或四个以上已知位置的地面标校源的高斯-牛顿定位算法。该算法首先利用差分法消除星间时差、频差测量的系统误差,再利用标校源的时差频差测量方程组估计出主星和伴星的相对位置和相对速度误差,最后结合时差、频差、地球球面以确定非合作辐射源位置。理论和数字仿真均表明在时差和频差测量的随机误差较小时,本文算法的均方根误差（MSE）接近克拉美-罗下限(CRLB)。