Stability of relative equilibria of the full spacecraft dynamics around an asteroid with orbit–attitude coupling

The full dynamics of spacecraft around an asteroid, in which the spacecraft is considered as a rigid body and the gravitational orbit–attitude coupling is taken into account, is of great value and interest in the precise theories of the motion. The spectral stability of the classical relative equilibria of the full spacecraft dynamics around an asteroid is studied with the method of geometric mechanics. The stability conditions are given explicitly based on the characteristic equation of the linear system matrix. It is found that the linearized system decouples into two entirely independent subsystems, which correspond to the motions within and outside the equatorial plane of the asteroid respectively. The system parameters are divided into three groups that describe the traditional stationary orbit stability, the significance of the orbit–attitude coupling and the mass distribution of the spacecraft respectively. The spectral stability of the relative equilibria is investigated numerically with respect to the three groups of system parameters. The relations between the full spacecraft dynamics and the traditional spacecraft dynamics, as well as the effect of the orbit–attitude coupling, are assessed. We find that when the orbit–attitude coupling is strong, the mass distribution of the spacecraft dominates the stability of the relative equilibria; whereas when the orbit–attitude coupling is weak, both the mass distribution and the traditional stationary orbit stability have significant effects on the stability. We also give a criterion to determine whether the orbit–attitude coupling needs to be considered.     

TEC differences for the mid-latitude ionosphere in both sides of the longitudes with zero declination

Based on measurements of ground-based GPS station network, differences of the mid-latitude ionospheric TEC in the east and west sides of North America, South America and Oceania have been analyzed in this paper. Results show that for nearly all seasons from 2001 to 2010 and in both sides of the longitudes with zero declination, there exist systematic differences for the mid-latitude ionospheric TEC in the regions mentioned above and the features of these differences markedly depend upon the local time but less depend upon seasons and the level of solar activity. Theory analysis shows that the longitude variations of both declination and zonal thermospheric winds are one of important factors to cause differences of the mid-latitude ionospheric TEC in both sides of the longitudes with zero declination.     

Direction finding for two-dimensional incoherently distributed sources with Hadamard shift invariance in non-uniform orthogonal arrays

This paper proposes a novel algorithm for Two-Dimensional (2D) central Direction-of-Arrival (DOA) estimation of incoherently distributed sources. In particular, an orthogonal array structure consisting of two Non-uniform Linear Arrays (NLAs) is considered. Based on first-order Taylor series approximation, the Generalized Array Manifold (GAM) model can first be established to separate the central DOAs from the original array manifold. Then, the Hadamard rotational invariance relationships inside the GAMs of two NLAs are identified. With the aid of such relationships, the central elevation and azimuth DOAs can be estimated through a search-free polynomial rooting method. Additionally, a simple parameter pairing of the estimated 2D angular parameters is also accomplished via the Hadamard rotational invariance relationship inside the GAM of the whole array. A secondary but important result is a derivation of closed-form expressions of the Cramer-Rao lower bound. The simulation results show that the proposed algorithm can achieve a remarkably higher precision at less complexity increment compared with the existing low-complexity methods, which benefits from the larger array aperture of the NLAs. Moreover, it requires no priori information about the angular distributed function.     

作动器故障下的无人机容错控制方法

在执行任务过程中,无人机的传感器、作动器等均可能出现故障。文章针对常规布局无人机的作动器故障,提出了 1种反步法和控制分配相结合的容错控制方法。首先,建立无人机数学模型,并对作动器故障进行分类和建模;然后,根据模型设计反步最优控制器和基于控制分配的容错控制器;最后,通过仿真验证表明,所设计的容错控制方法能够实现作动器故障下的姿态快速稳定控制,且稳定性好,基本无侧滑角,各操纵面均在约束范围内,达到容错控制要求。     

三维五向编织复合材料的冲击压缩特性及破坏机制

利用分离式霍普金森压杆(split Hopkinson pressure bar,SHPB)实验系统和高速摄像技术对三维五向碳/环氧编织复合材料的动态压缩特性进行研究。通过对编织角为22.3°的试样分别进行沿纵向和横向方向的冲击压缩实验,得到材料在200~1200 s^-1应变率范围内的应力应变曲线,并结合高速摄像记录的动态压缩过程,对不同应变率下材料在高速变形下的渐进破坏规律进行分析。同时,综合试样的宏观破坏特征和微观断口形貌特征,进一步分析材料的破坏模式及破坏机理。结果表明:随着应变率的增加,材料在纵向和横向均具有一定的应变率强化效应,在横向方向的应变率强化效应更为显著;不同加载方向下材料的渐进破坏过程、应力应变曲线特征以及破坏方式均具有明显差异,且随着应变率的增加而发生改变。     

MR螺纹在修理过程及型号研制中的应用问题

读了《航空标准化与质量》１９９９年第１期胡富同志撰写的《ＭＲ螺纹在修理过程中的应用探讨》一文,笔者认为该文较全面分析了ＭＲ螺纹和ＭＪ螺纹之间的关系以及与普通螺纹之间的连带关系,同时还在综述中明确指出了：“ＭＲ螺纹和ＭＪ螺纹的大径和中径相同,小径和外螺纹牙底圆弧半径只有很小的差异,因此ＭＲ螺纹与ＭＪ螺纹可以互换,且不会产生干涉,也不会改变配合性质。因此ＭＲ螺纹的加工和检验可以使用与其公差带相同的ＭＪ螺纹的加工工具和检验工具”。但又提出：在修理过程中,ＭＲ螺纹不能用国军标ＭＪ螺纹替代,其理由是：“Ｍ…     

三芳基均三氮杂苯环（TSTR）耐高温树脂的研究

从制备最主要的原材料入手,研究了ＴＳＴＲ树脂的合成,并对树脂进行了红外光谱分析（ＩＲ）以及差示扫描量热法（ＤＳＣ）和热重量分析法（ＴＧＡ）等热分析,其中４－氰基苯酐的一步合成法已申请了国家专利。试验结果表明：该树脂的最高工作温度可达４００℃,接近美国先进的ＰＭＲ－Ⅱ－５０ 高温树脂的工作温度。     

铝合金锻件重复淬火保温时间对组织性能的影响

分析了铝合金锻件重复淬火保温时间的长短及其组织性能的影响情况。根据大量的试验数据,证实了重复淬火保温时间及时效保温时间的长短对锻件性能的直接影响,并以此确定了合理的工艺参数。     

一种用于飞机试验台的三分力传感器

多分力载荷传感器是一种常用的传感器,但通常当各分力的量程相差太大时难以取得良好的效果。提出了一种新型传感器结构形式,减少了各分力之间的耦合,使得在各分力量程不匹配的情况下亦可获得较高的测量精度。