扩展旋转矢量捷联姿态算法

给出了一种新的旋转矢量捷联姿态构造算法，该算法由陀螺样本的多重积分来构造旋转矢量的最小二乘估计。新算法具有较好的顺序递推结构，易于在机载计算机上编程实现，比传统方法更容易满足一些限制较多的特殊应用。文中还给出了该算法在机载计算机上的计算流程及算法的局部硬件化实现。     

基于非等间距采样输出的旋转矢量姿态算法

基于实际系统中陀螺的输出为非等间隔的角增量信号，重点研究了采样时刻的变化对捷联姿态算法的影响，并推导出旋转矢量三子样算法和二子样算法的通用表达式及其误差方程。传统的Miller算法已被证明是本算法的特例。研究发现，算法误差与由采样时刻构成的误差系数阵密切相关，Miller算法中的等间距采样使得该矩阵奇异，而改变采样间距可使其满秩，从而降低算法误差。然而对角增量输出的二子样算法而言，等间隔采样比非等间距采样具有更小的箕法漂移。仿真及试验结果证明了本文的观点。     

基于规划航迹的“三自”光纤惯导系统航向耦合效应抑制技术

目前,国内"三自"(自标定、自对准、自检测)光纤惯导系统在长航时高精度自主导航领域已逐渐开展应用,但光纤陀螺安装误差、安装不正交度以及标度因数等参数稳定性大大限制了"三自"光纤惯导系统精度的提升,其主要原因是载体运动诱发的航向耦合效应严重影响了旋转调制效果。从航向耦合效应机理分析入手,指出了"三自"惯导系统航向耦合效应的不可解耦性,但针对无人飞行器和无人潜航器等通常需要规划航迹的载体,提出了一种基于规划航迹的旋转方案自适应调整技术,有效地抑制了航向耦合效应。试验结果表明,该方法可将系统的导航精度提升80%以上。     

ESPRIT算法在单快拍阵列信号中的应用

ESPRIT算法利用旋转不变技术估计信号参数,是近年来提出的阵列信号处理理论的一个新领域,它具有高分辨率、高精度、不需空间搜索等优点。单快拍总被当作相干信号处理,本文采用了Teoplitz结构协方差矩阵估计,起了空间平滑作用,所以可以估计相于信号源的波达方向(DOA),与标准空间平滑协方差矩阵估计相比较,Teoplitz协方差阵估计在总体上提高了信噪比,并且不牺牲阵列孔径。 计算机模拟结果表明,基于Teoplitz结构协方差矩阵的TLS-ESPRIT算法在20dB信噪比下,可以分辨出相隔0.2瑞利波束宽度的空间信号。     

Three-dimensional numerical analysis on combustion performance and flow of hybrid rocket motor with multi-segmented grain

This paper presents the combustion characteristics in hybrid rocket motors with multi-segmented grain through three-dimensional numerical simulations. Multi-segmented grain is composed of several thin grains with two or more ports. The numerical model consists of Navier-Stokes equations with turbulence, solid fuel pyrolysis, chemical reactions, a fluid–solid coupling model and a regression rate model. The simulations adopt 90% Hydrogen Peroxide (HP) and PolyEthylene (PE) as the propellant combination. The effects of the rotation, port number, fuel grain segment number and mid-chamber length on the flow field and combustion performances are analyzed. The results indicate that the multi-segmented grain configuration can strengthen the flow field, and the regression rate and combustion efficiency are enhanced. Take the cases with two grain segments and three ports for example, the regression rate is increased by 32.4%−45.1% and the combustion efficiency increases by 6%−8.6% in different rotation angles.     

Double-zone model with diffusive mixing and the mass and helium discrepancies in OB-stars

A model for massive main sequence (MS) stars is proposed that quantitatively accounts for the mass and helium discrepancies in luminous OB stars. The radiative envelope of the model consists of two zones being mixed by rotationally induced turbulent diffusion during the star's evolution on the MS. The rate of the mixing in the outer zone is assumed to be substantially lower than that in the inner zone. Both, the mass and helium discrepancy, are shown to be due to helium enrichment in the envelope produced by turbulent diffusion. Some arguments to support this double-zone stellar model are given.Alexander von Humboldt Fellow     

基于改进SSD的舰船目标精细化检测方法

以SSD为代表的主流深度学习方法在目标检测领域取得了显著的成绩，但由于该类方法只能以矩形框给出目标的概略位置，检测结果具有很大的背景冗余区域，特别是港口密集停泊的舰船在图像中会出现区域重叠，导致误检和漏检。针对以上问题，提出了一种具有旋转不变性的舰船目标精细化检测方法，该方法综合利用可变形卷积、可变形池化、旋转的边框回归和旋转的非极大值抑制等模块的优点，借鉴MobileNet架构对网络加速，通过学习密集区域目标的几何形变，有效预测目标的旋转角度，最终以旋转的矩形框给出目标的位置。实验结果表明，该算法可实现多类舰船目标类型区分和目标朝向判定的功能，有效地解决了实际应用中的目标精确定位定向难题，提高了自动目标识别的精确性，并满足工程应用的实时性要求。     

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.     

轨道面旋转角对GEO卫星广播星历参数拟合的影响

广播星历参数拟合是建立卫星导航系统的一项关键技术,星历用户算法的简洁高效直接决定了用户导航定位的效率。在基于GEO、IGSO和MEO三类卫星的北斗二代导航定位系统中,GEO卫星的广播星历参数拟合是迫切需要解决的难点之一。基于广播星历参数的最小二乘解法,推导出了轨道面旋转角对广播星历参数的影响表达式,分析了轨道面旋转角的大小对广播星历参数拟合稳定性的影响。计算结果表明,通过增加轨道面旋转角不仅很好地解决了GEO卫星广播星历参数超限的问题,而且确保了广播星历参数拟合算法的精度和可靠性。     

捷联惯性导航系统姿态算法研究

用四元数和旋转矢量在捷联惯导系统中表示姿态矩阵,在圆锥运动的条件下,对旋转矢量算法进行了优化。对四元数、旋转矢量优化算法进行了仿真比较。仿真结果表明:等效旋转矢量算法明显优于四元数算法。