基于北斗卫星速度外推的GEO卫星速度解算方法

北斗二代导航系统是我国自主开发的区域卫星导航系统,该系统利用GEO卫星实现了区域卫星导航定位。针对GEO卫星的特点,现有的GEO卫星速度解算方法分为微分法与差分法两种,这两种方法各有优缺点。为了进一步提高GEO卫星速度计算的效率与精度,首先对两种计算GEO速度的计算方法进行了推导,从计算精度、计算量,计算时间和软件实现难易程度对两种方法进行了对比,同时提出了一种利用卫星加速度进行卫星速度外推的方法,仿真结果表明这种方法能够提高接收机的测速精度,且计算量较小,工程实现难度较低。     

轴流压气机小扰动诱发旋转失速的试验研究

为了了解压气机旋转失速产生的原因 ,用试验方法对一低速轴流压气机旋转失速前的小扰动波进行了研究 ,通过分析该扰动波的特性 ,推断出小扰动是从转子进口端壁附面层内产生的 ,该波的振荡是旋转失速产生的根源     

编队小卫星星间基线估计算法研究

H ill方程假设卫星轨道是小偏心率和无摄动的,实际应用时难以获得高精度的星间基线估计。本文提出了一种基于主星位置展开的扩展Kalm an滤波算法,该算法采用含摄动的卫星运动模型,综合利用星间无线电和红外仪器的原始量测,实现了小卫星星间基线的融合估计,提高了估计精度。仿真实验针对J2摄动模型验证了算法的可行性和有效性。     

Pc5 Oscillation Analysis by the Satellite and Ground-Based Data

Large amplitude Pc5 event was observed in the space and on ground on August 3, 2001, about three hours after contact of the strong discontinuity in the solar wind with the magnetosphere according to data from ACE and Wind satellites. The Pc5 amplitude was as high as 15 nT in the tail of magnetosphere and about 5 nT at the ground based stations. In the magnetosphere Pc5 waves were observed by Cluster and Polar satellites, which occupied positions in the morning part of the near tail at the close field lines but were parted by distance of 11.5 Re, mainly along the x-axis of the GSM coordinate system. Both compressional and transverse components of the Pc5 wave activity were observed in the space, with the transverse component having the larger amplitude. Time delay between the Cluster and Polar satellites was about 8 minutes, which could be interpreted as a wave propagation from the geomagnetic tail to the Earth with the 150 km/s group velocity. The ground-based Pc5 activity was analysed by using data from the Image magnetometer network. Doubtless demonstrations of a field line resonant structure were found in variations of amplitude and polarization with latitude. Finnish chain of search coil magnetometers observed modulated Pc1 emission simultaneously with the Pc5 wave train. A possibility of non-linear impact of Pc5 wave energy on the plasma and waves in the magnetosphere is discussed.     

一种利用面质比调整提高编队构形稳定性的方法

分布式卫星编队构形受大气摄动的影响会产生沿航迹方向的相对漂移。通过合理的面质比调整,可以降低漂移,提高构形稳定性。基于包含周日效应的大气密度模型,研究了编队卫星轨道能量耗散的差异,进而指出大气摄动引起的构形漂移与构形初始相位、以及轨道面和太阳密度周日峰方向夹角之间存在的关系。给出解析形式和数值方式2种面质比调整方法,并对后一种方法进行了仿真。仿真结果显示,利用文中给出的面质比调整方法,能够大大提高构形的稳定性。     

捷联惯组历次测试数据验前分布随机加权中心融合估计法

在小子样理论中,验前分布的获取与表示是一个关键问题。针对捷联惯性测量组合(捷联惯组)历次测试数据验前分布的获取问题,探讨了在异总体情况下,多种验前信息的融合问题。提出了通过随机加权中心融合法实现多种异源信息融合,以获取捷联惯组历次测试数据验前分布,从而减小了小样本情况下的统计分析误差。     

Orbital corrections by a single-input impulsive control applied along the geomagnetic field

This paper examines the possibility of regular orbital corrections for a satellite controlled by an impulsive force applied along the induction vector of the local geomagnetic field. The main purpose of the correcting considered in the paper is to eliminate the drift in secular variation of the relative orbital parameters over the orbital period. The obtained results are applied to the formation flying problem. The developed method is tested using numerical simulation.     

具有主动磁控的重力梯度稳定系统的研究

介绍了主动磁控太阳同步轨道遥感小卫星控制系统的分析与设计,其中包括卫星广义动力学模型的建立,磁偶极子分配与生成以及满足控制能限要求的系统分析与设计等,最后,通过数学仿真人出稳定系统的性能指标,仿真结果表明,对于具有非线性,变系数和交叉耦合的广义飞行器动力系统,主动磁控加重力梯度稳定可使卫星姿态达以优于５度的对地指向精度。     

相对轨道自主确定方法的改进

编队飞行卫星相对轨道的确定具有重要意义。本文提出一种完全自主的定轨方案,在利用星间测量信息实现编队飞行卫星自主定轨的基础上,引入太阳敏感器测量信息,利用扩展卡尔曼滤波算法提高环绕星相对轨道确定精度。仿真结果验证了这种导航方案和算法的有效性。     

CCSDS Proximity-1及其在编队飞行小卫星群中的应用

讨论近距离空间链路协议 Proximity- 1的层次结构和传输帧 Version- 3构成 ,分析包括 CCSDS标准包和用户自定义数据的数据业务及定时业务。针对编队飞行小卫星群的星间数据交换和自主测控 ,对 Proximity- 1应用于小卫星群星间通信和星间测距作了探讨