北斗卫星导航空间信号模拟畸变研究

针对卫星导航信号生成载荷故障会导致信号畸变,对北斗卫星导航信号模拟进行了研究分析。首先,建立了北斗导航信号模拟畸变的数学模型并对其进行了理论分析;其次,推导了北斗信号发生模拟畸变后的相关函数、功率谱密度函数和相关损耗,并仿真分析了北斗信号模拟畸变的相关峰曲线、功率谱密度曲线和相关损耗曲线;最后,利用S曲线及S曲线锁定点偏差的模型,仿真了北斗模拟畸变信号S曲线及S曲线锁定点偏差,并分析了北斗信号发生模拟畸变对测距性能产生的影响。结果表明：北斗信号发生模拟畸变的畸变程度越大,伪距测量误差越大,则导航系统的测距精度和定位精度越低,增强系统的完好性越小。     

RTCA协议下北斗完好性降效参数算法设计及检验

目前我国北斗导航增强系统的完好性参数设计缺少针对差分信息有效性的降效参数设计,不满足航空无线电委员会（RTCA）提出的接口协议,无法同国际其他GNSS星基增强系统相兼容。根据RTCA接口协议,针对我国卫星导航系统的完好性降效参数处理算法进行了研究,利用北斗实测数据分析了完好性降效参数对用户增强服务的影响,验证了算法的有效性。结果表明,正常情况下,北斗导航系统增强服务三维定位精度可达到113m。当用户丢失部分差分改正信息时,定位精度约144m,精度下降约274%,利用完好性降效参数对过期差分信息进行降效处理,优化定位权阵,可将定位精度提高至117m,达到正常增强服务水平。     

空间非合作目标的多视角点云配准算法研究

为了提高相邻视角间稀疏扫描点云数据配准的速度和精度,实现多视角点云精确配准,提出一种基于KD Tree点云均匀采样简化算法,并且对传统四点算法（4 PointsCongruentSetsAlgorithm,4PCS）中的阈值参数进行了统一,确定了各误差阈值参数和点云密度之间的关系,通过基于姿态校正的方法有效解决了对称视角点云引起的误配准问题。仿真结果表明,该方法能够快速、有效地实现卫星稀疏点云的配准。     

采用弱攻角补偿与脱敏设计的火星进入段制导

为提升火星进入段存在多种扰动时的制导末端精度,在现有三自由度脱敏设计的基础上,提出针对大气密度及升阻力系数波动的弱攻角补偿方法。通过攻角调整,协调升、阻力加速度测量值相对理论计算值的偏离程度,使加权形式的偏离程度指标趋近于1,从而降低气动参数波动对制导精度的影响。相平面分析和反证法证明了攻角调整过程的稳定性。蒙特卡洛仿真结果表明,该方法可达到较高的纵向末端状态精度。     

解析计算在月球中继卫星Halo轨道设计中的应用

面向月球中继卫星工程轨道设计需求,研究解析计算方法在地月系L2点halo轨道设计中的应用问题。在讨论圆型限制性三体问题三阶解析近似计算方法的基础上,分析了解析计算与数值计算的差异,给出了解析近似计算在工程约束下的适用范围,进而提出了基于解析计算的轨道设计和特征筛选方法。分别采用解析初值和数值初值进行halo轨道外推,比对验证采用解析计算设计轨道的可行性。研究结果表明,解析计算方法适用于月球中继卫星轨道的初步设计、特征分析和构型筛选。     

国内民航客运需求价格点弹性与弧弹性研究

采用微观经济学的点弹性和弧弹性理论,对国内民航客运需求价格弹性进行初步对比研究.结合民航客运的自身特点,提出适用于民航客运需求价格弹性的点弹性和弧弹性分析方法,并采用此方法对国内民航客运市场进行分析,得出国内民航整体市场是富于弹性的和旺盛需求的结论,最后给出点弹性与弧弹性对比.     

运输机空投起始点研究

根据货物空投着陆点及空投轨迹,计算出运输机空投起始点,并将所计算的空投起始点信息提供给航电系统,引导运输机执行空投点航线。空投起始点的研究对运输机实现空投功能及提高空投精度具有重要的理论意义和现实意义。     

一种利于交班的舰空导弹最优中制导律设计

针对舰空导弹超视距拦截低空飞行目标问题,在复合制导的中制导段,建立了导弹拦截目标的相对运动模型,依据制导平台无线电指令修正信息,考虑舰空导弹拦截低空目标时的飞行速度特性,给出了预测遭遇点的实时解算模型,并确定了利于中末制导交班的中制导终端约束条件。基于拦截预测遭遇点,引入伪控制量的概念,应用线性二次型最优控制理论,设计了一种基于拦截预测遭遇点的利于制导交班的最优中制导律,仿真结果验证了预测遭遇点实时解算模型和最优中制导律的正确性与有效性。     

Libration point orbits for lunar global positioning systems

With the development of lunar exploration, a lunar global positioning system (LGPS) is demanded for both on-ground and in-flight lunar exploration missions. The traditional configuration of constellation requires at least eighteen satellites to cover the whole lunar surface continuously. In this paper, the configurations of the libration point orbits (LPOs) constellations are investigated. By using the constellations on the Earth–Moon _L1$L_1$ and _L2$L_2$ LPOs, the basic functions of the LGPS can be realized by using eight to fourteen satellites. First, the LPO and the combinations of LPOs, which can be used in the constellations of the LGPS, are investigated. The criteria and procedures of the configuration design are introduced. Second, the configurations of LPOs constellations are investigated in the Earth–Moon circular-restricted three-body problem (CR3BP). The size of the LPOs and the distribution of the satellites on these LPOs are determined by using an exhaustive algorithm and a global optimization method, respectively. The key performance parameters of these constellations are computed. Third, the constellations with good performance in the CR3BP are redesigned in the more accurate Earth–Moon based Sun-perturbed bicircular four-body problem (B4BP). Moreover, in order to avoid the ground coverage problem caused by the perturbation of the Sun, some modifications are implemented, and the configuration of the no blind area LGPS in the B4BP is obtained.     

Symmetry and asymmetry of ionospheric weather at magnetic conjugate points for two midlatitude observatories

Variations of the ionospheric weather W-index for two midlatitude observatories, namely, Grahamstown and Hermanus, and their conjugate counterpart locations in Africa are studied for a period from October 2010 to December 2011. The observatories are located in the longitude sector, which has consistent magnetic equator and geographic equator so that geomagnetic latitudes of the line of force are very close to the corresponding geographic latitudes providing opportunity to ignore the impact of the difference of the gravitational field and the geomagnetic field at the conjugate points on the ionosphere structure and dynamics. The ionosondes of Grahamstown and Hermanus provide data of the critical frequency (foF2), and Global Ionospheric Maps (GIM) provide the total electron content (TECgps) along the magnetic field line up to the conjugate point in the opposite hemisphere. The global model of the ionosphere, International Reference Ionosphere, extended to the plasmasphere altitude of 20,200 km (IRI-Plas) is used to deliver the F2 layer peak parameters from TECgps at the magnetic conjugate area. The evidence is obtained that the electron gas heated by day and cooled by night at the summer hemisphere as compared with the opposite features in the conjugate winter hemisphere testifies on a reversal of plasma fluxes along the magnetic field line by the solar terminator. The ionospheric weather W-index is derived from NmF2 (related with foF2) and TECgps data. It is found that symmetry of W-index behavior in the magnetic conjugate hemispheres is dominant for the equinoxes when plasma movement along the magnetic line of force is imposed on symmetrical background electron density and electron content. Asymmetry of the ionospheric storm effects is observed for solstices when the plasma diffuse down more slowly into the colder winter hemisphere than into the warmer summer hemisphere inducing either plasma increase (positive phase) or decrease (negative phase of W-index) in the ionospheric and plasmaspheric plasma density.