Low latitude nighttime ionospheric vertical E × B drifts at African region

The nighttime vertical E × B drifts velocities of the F2-region were inferred from the hourly hmF2 values obtained from ionosonde data over an African equatorial station, Ilorin (8.50^oN, 4.68^oE; dip lat. 2.95^o) during period of low solar activity. For each season, the plasma drift Vz is characterized by an evening upward enhancement, then by a downward reversal at 1900 LT till around 0000 LT, except for June solstice. This was explained using the Rayleigh–Taylor (R-T) instability mechanism. The occasional drift differences in Vz obtained by inferred and direct measurement over Ilorin and Jicamarca, respectively are reflective of the importance of chemistry and divergent transport system due to both the E region electric and magnetic fields instead of simple motions. The pre-reversal enhancement (PRE) magnitude is higher during the equinoctial months than the solsticial months over Jicamarca, highest during December solstice and the equinoctial months over Ilorin, suggesting the dominance of higher E × B fountain during equinoxes at both stations. The lowest PRE magnitude was in June solstice. The appearance of post-noon peak in NmF2 around 1700 LT is highest during the equinoctial months and lowest during the solsticial period. A general sharp drop in NmF2 around 1800 LT is distinct immediately after sunset, lowest during June solstice and highest in March equinox. Our result suggests that between 0930 and 2100 LT, the general theory that vertical drifts obtained by digisonde measurements only match the E × B drift if the F layer is higher than 300 km is reliable, but does not hold for the nighttime period of 2200–0600 LT under condition of solar minima. Hence, the condition may not be sufficient for the representation of vertical plasma drift at nighttime during solar minima. This assertion may still be tentative, as more equatorial stations needed to be studied for better confirmation.     

单周期冲跃飞行轨迹性能参数影响程度分析

对高超声速飞行器的单周期冲跃飞行轨迹进行了研究。建立了动力学模型和约束条件。仿真分析了升阻比、初始速度和初始弹道倾角对飞行轨迹性能的影响,并讨论了影响程度,确定了适于该飞行器的最佳飞行走廊,为后续的冲跃飞行轨迹完整设计和优化提供了参考。     

基于单循环方法的涡轮叶片可靠性及多学科设计优化

为了得到适用于涡轮叶片复杂结构并同时考虑可靠性的多学科设计优化方法,将基于单循环方法的可靠性分析（SLBRA）与并行子空间设计优化方法 （CSSO）相结合,提出了一种基于可靠性的多学科设计优化（RBMDO）方法。在优化过程中使用Kriging近似模型并不断提高模型精度。该方法在计算最可能失效点（MPP）的过程中避免了优化迭代,提高了计算效率。以涡轮叶片的设计优化为例,对该方法进行了验证并与传统双循环方法进行了对比。结果表明,优化结果满足可靠性的要求,与双循环方法相比优化效率明显提高,证明了该方法在工程应用中的可行性和有效性。     

空间站空间因特网与空间通信链路设计

为改善在空间站长期值守的航天员的业务生活,提出建立空间站网吧,为航天员提供因特网服务的构想。为此分析研究空间站空间因特网服务系统及其关键技术,提出空间站空间因特网服务系统构建方案。结合这一系统构建方案,一是研究解决了支持复杂异构网络运行的空间因特网网络协议设计技术,空间站空间因特网直接采用TCP/IP协议,并通过系统设计,较好地克服了TCP/IP协议不能适应空间通信链路的难题,支持采用基于TCP/IP协议的商用货架(COTS)软、硬件产品,可明显降低空间站空间因特网服务系统建设与维护成本;二是研究解决了涉及空间站测控通信网运行安全和空间信息安全的空间通信链路设计技术,空间站在同一条空间通信链路同时传输空间因特网数据和空间站测控通信数据,空间通信链路采用CCSDS的AOS协议,并通过建立虚拟的物理信道,解决了空间因特网数据和空间站测控通信数据的安全隔离问题,能满足空间站测控通信网运行安全和空间信息安全的要求。     

面向航空节点的IP/LEO卫星网络移动性管理方法(英文)

Taking into chief consideration the features of aviation nodes in satellite networks, such as high moving speed, long communication distance, and high connection frequency, this article proposes an aviation-oriented mobility management method for IP/low earth orbit （LEO） satellite networks. By introducing the concept of ground station real-time coverage area, the proposed method uses ground-station-based IP addressing method and cell paging scheme to decrease the frequency of IP binding update requests as well as the paging cost. In comparison with the paging mobile IP （P-MIP） method and the handover-independent IP mobility management method, as is verified by the mathematical analysis and simulation, the proposed method could decrease the management cost. It also possesses better ability to support the aviation nodes because it is subjected to fewer influences from increased node speeds and newly coming connection rates.     

基于LabVIEW的皮卫星接收地面站解调器设计

针对皮卫星接收地面站测试系统解调器的应用场合,研究和开发了一种基于LabVIEW虚拟仪器开发平台的软件解调器,提出了一种简化的遥测信号解调算法。利用LabVIEW控制数据的采集和存储,通过VisualC 实现了解调算法,并在LabVIEW中调用该程序来实现地面站遥测信号的解调。给出了解调算法的原理、Costas环跟踪方差的MATLAB仿真和软件设计,通过误码率实验,测试结果证明了该设计的有效性。本解调系统具有应用灵活和便于改进的优点,已应用于皮卫星的测试实验。     

一种模拟整星热环境的小型单机热平衡试验

文章通过对一个典型的单机热分析和热试验的研究,提出了一种小型单机热平衡试验方法,模拟单机在整星环境下的热平衡试验,以避免只为验证其热设计而再次补做整星热平衡试验。为准确模拟单机在星内的辐射和导热过程,通过灰体间辐射热网络法和仪器安装板处单元体热平衡法,给出了等效辐射特征点和等效导热特征点的确定方法;并结合试验结果,对模型修正的合理性、局限性进行了分析,提出了在实际应用过程中应注意的问题。     

卫星天线极化向量的跟踪定向分析

卫星地球观测站跟踪观测卫星时,天线跟踪极化角方向相对星体坐标系下的极化倾角存在偏移,其偏差大小与观测点地理位置有关。为了更好地实现星地链路跟踪极化匹配,必须确定跟踪极化角。通过对卫星天线极化向量的坐标分解,采用坐标转换法,建立地球观测站天线坐标系中的天线极化倾角对卫星坐标系中极化角的定向关系。基于上述转换关系,通过编程计算,可以对任意线极化信号相对任意观测位置的跟踪极化倾角进行定量分析。     

利用地月间空间站的载人登月飞行模式分析

为提高空间站利用率,降低载人登月任务成本,有效开发地月空间,研究了基于地月空间不同轨道空间站的载人登月飞行模式。首先对比直接往返登月飞行模式,对基于空间站的载人登月飞行模式进行任务分析,通过空间站将载人登月任务解耦为载人天地往返任务和登月任务两部分;其次通过轨道设计和稳定性分析提出考虑登月任务需求的地月间空间站可运行轨道和停泊点;最后建立一套飞行模式评价模型,从速度增量需求、飞行时间、空间环境、登月任务窗口、测控条件、交会对接技术难度、后续任务支持性和任务可靠性方面对6种不同位置空间站的登月飞行模式进行分析和定量评价。评价结果表明基于L2点Halo轨道空间站的载人登月飞行模式为更优飞行模式。     

“和平号”空间站SGCMG系统及其操纵

综述了“和平号”空间站ＳＧＣＭＧ系统的组成和操纵，并给出了梯度型操纵律回避奇异的一般化解释。同时指出，奇异问题和失效操纵问题是ＳＧＣＭＧ系统的两个重要问题，也是今后ＳＧＣＭＧ系统研究的主要课题。