虚拟仿真环境中的航路冲突调配规则研究

现行仿真工具在模拟管制员航路冲突调配上存在问题边界不一致、调配方案不适用等诸多问题。针对这种现状，根据航路飞行冲突的影响因素对航路冲突进行了详细分类，并基于决策树建立了航路冲突调配方案。以决策树为基础，使用VB工具进行系统开发，建立快速仿真工具。模拟运行表明，仿真工具可模拟管制员提供简易可行的航路冲突调配方案，驱动仿真系统的运行。     

进近过程中的排序和冲突解决算法研究

研究了终端区飞机进近过程中排序和冲突解决的调度算法.借鉴美国研制的最后进近间隔工具(FAST)中的排序、冲突预防和解决方法,讨论了这些方法在终端区飞机进近过程中将排序和冲突解决综合实现问题,分别给出了在飞行段和汇聚过程中排序和冲突解决的算法模型.仿真结果表明该模型能有效地解决最后进近过程中的排序和冲突问题,使到达飞机流快速有序地进入机场着陆.     

高分辨率航天光学遥感器发展新思路研究

简要介绍了高分辨率航天光学遥感器的发展，重点分析了新一代更高分辨率航天光学遥感器所采用的理论基础和发展趋势，指出了传递函数补偿（MTFC）和系统优化设计是高分辨率航天光学遥感器发展的方向之一。     

宽量程高分辨率自校准智能化电容表

本文是宽量程高分辨率自校准智能化电容表的研制总结。文章给出了它的功能、结构、原理及可行性分析，并对研制过程中的难点进行了分析介绍。     

在直流电流表不确定度评定中分辨力的影响

在直流电流表的检定或校准中,通常采用标准直流电流源输出标准电流,被检电流表的读数与标准直流电流源的数值进行比较。电流测量仪表的分辨力对重复性测量有一定影响,而且分辨力对测量结果的不确定度有影响。通过测量实例说明,如何在直流电流表的测量结果中考虑分辨力的影响。     

Multiple Coulomb scattering method to reconstruct low-energy gamma–ray direction in the GAMMA-400 space-based gamma–ray telescope

The GAMMA-400 currently developing space-based gamma-ray telescope is designed to measure the gamma-ray fluxes in the energy range from ～20?MeV to several TeV in the highly elliptic orbit (without shadowing the telescope by the Earth) continuously for a long time. The physical characteristics of the GAMMA-400 gamma-ray telescope, especially the angular and energy resolutions (at 100-GeV gamma rays they are ～0.01° and ～1%, respectively), allow us to consider this space-based experiment as the next step in the development of extraterrestrial high-energy gamma-ray astronomy. In this paper, a method to improve the reconstruction accuracy of incident angle for low-energy gamma rays in the GAMMA-400 space-based gamma-ray telescope is presented. The special analysis of topology of pair-conversion events in thin layers of converter was performed. Applying the energy dependence of multiple Coulomb scattering for pair components, it is possible to estimate the energies for each particle, and to use these energies as weight in the angle reconstruction procedure. To identify the unique track in each projection the imaginary curvature method is applied. It allows us to obtain significantly better angular resolution in comparison with other methods applied in current space-based experiments. When using this method for 50-MeV gamma rays the GAMMA-400 gamma-ray telescope angular resolution is about 4°.     

Inertial aided BDS triple-frequency integer ambiguity rounding method

The integer ambiguity resolution (AR) of carrier phase is significant for Global Navigation Satellite System (GNSS) precise positioning. However, in kinematic case, single-epoch AR methods based on alone GNSS are usually not reliable due to the instable pseudorange accuracy. Moreover, the computation of classical AR method Least Squares Ambiguity Decorrelation Adjustment (LAMBDA) is large. Thus, the inertial measurement unit (IMU) is introduced, a new inertial-aided AR method that directly rounds the float ambiguity of BeiDou triple-frequency combined observations, which is characterized by long wavelength, low carrier-phase noise and ionospheric delay, is proposed. The mathematical model of the new method is derived first. Then the impacts of the carrier-phase noise, ionospheric delay and inertial navigation system (INS) position error on the AR success ratio of combined observation are analyzed through probabilistic approach. Based on above investigation, the combinations (0, ?1, 1), (1, 4, ?5) and (4, ?2, ?3) are selected to resolve the original ambiguity. A vehicular integrated navigation test is performed to demonstrate the proposed method. The results show that the average AR success ratios of the three selected combinations, whose float ambiguity errors are 0.041, 0.146, 0.279 cycle respectively, are above 97.25% without regard to low-elevation C05. With respect to positioning accuracy based on our AR method when compared with IE software, the east, north, up error RMS of position are 0.042, 0.024, 0.069 m, respectively. In terms of the AR recover after the BeiDou signals outage, as long as 62 s BeiDou signal complete outage, all the ambiguities of all satellites could be re-fixed immediately. Besides, during the 90 s signals partial outage, the AR is not influenced by the position error, since the float ambiguity errors are all below half-cycle. The research of this contribution demonstrates the effectiveness of the proposed new method, which indicates it is applicable to kinematic positioning, even in BDS degraded and denied environments.     

低仰角射线对电离层CT成像的影响分析

电离层层析成像(Computerized Tomography, CT)是一个有限视角问题, 水平射线的缺失造成CT结果垂直分辨率的严重下降. 很多人直观地认为低仰角射线可以弥补水平射线的缺失, 然而本文的理论分析和数值模拟研究结果表明, 低仰角射线对CT结果的影响十分微小, 其无法弥补水平射线缺失所带来的垂直分辨率的下降. 模拟结果显示, 增加低仰角射线前后CT反演结果几乎没有变化; 而去掉680条低仰角射线和高仰角射线后, CT反演结果差别巨大; 去掉680条低仰角射线的CT结果与模型吻合很好; 去掉680条高仰角射线的CT反演结果失真严重, 几乎无法恢复模型的扰动特征.      

深空组合导航中天文测速观测研究

深空天文测速导航方法以空间中的某颗恒星为目标,利用航天器自身携带的光谱仪测量相对于恒星的移动速度来实时调整自行速度和路线。太阳是主要的测速导航源之一,利用目前运行的空间卫星的光谱观测资料,分析和研究了太阳相对于卫星的视线速度和速度误差变化情况,为本项目中自主导航光谱提供实测证据。选取了太阳表面5个位置的光谱观测,持续时间在一个小时左右,通过高斯谱线轮廓拟合观测数据,得到了太阳表面5个位置的亮度变化、谱线宽度和速度,其中主要参数速度平均值大约在10 km/s,和速度变化在3 km/s。这是由太阳表面存在大量的微观尺度上的物质运动所导致的。     

基于压缩感知的频率和DOA联合估计算法

波达方向（DOA）估计是阵列信号处理的一个重要问题,针对信号的DOA估计问题,本文基于压缩感知理论,提出了一种新的频率和角度联合估计算法。首先利用方向波数的空间稀疏性,建立过完备稀疏字典,然后利用压缩采样阵列结构通过求解最优化问题得到方向波数的高分辨估计,最后利用最优空域滤波实现信号到达角度和频率的配对。相对于传统算法,该算法能够实现多信号DOA的高分辨估计,且经过压缩采样后降低了运算量,仿真验证了该算法的正确性与有效性。