一种基于卷积神经网络的地磁基准图构建方法

地磁匹配导航技术是一种重要的辅助导航制导方法，地磁基准图的构建精度对地磁匹配制导的精准度起着决定性作用。针对现有地磁基准图构建精度难以满足实际地磁匹配导航需求的问题，提出了一种基于卷积神经网络的地磁基准图构建方法。首先，利用卷积层提取低分辨率基准图中的特征图像块；然后，利用基于学习的阈值收缩算法（LISTA）实现图像块的稀疏表示；最后，利用三通道的地磁信息得到重建后的高分辨率基准图。实验结果表明:所提方法对地磁基准图具有更高的构建精度，同时对噪声有更好的鲁棒性，各种客观评价指标均高于现有的超分辨率重建方法。      

基于混杂非对称复合材料的自适应对日定向器

提出并设计了一种基于混杂非对称复合材料层合板的新型自适应对日定向器。该对日定向器采用混杂非对称复合材料层合板作为驱动元件，利用在轨光照条件的变化引起复合材料层合板温度变化，进而使其产生热变形并驱动太阳翼发生偏转。提出的自适应对日定向器结合传统的单自由度对日定向机构，能够实现太阳能帆板的双自由度对日定向。介绍了自适应对日定向器的基本原理，并结合地球静止轨道的光照条件进行了具体设计。利用能量变分原理建立了混杂非对称复合材料的热变形模型，分析其热变形特点，并利用有限元方法对定向器在地球静止轨道上的温度场特性、热变形及对日定向转动角度进行分析。有限元分析结果表明，通过合理设计，自适应对日定向器的转角能够随太阳光入射角变化呈线性变化，定向精度可达±1°。     

基于变刚度变阻尼的柔性喷管动态模型

针对柔性接头动态迟滞曲线受控制系统控制位置精度和动态响应速度影响较大的问题,基于电液伺服机构和柔性接头变刚度变阻尼模型,构建了柔性喷管的电液伺服机构-变刚度变阻尼模型,将其和电液伺服机构-定刚度定阻尼模型进行了对比。分析了电液伺服机构主要参数、柔性接头工作参数等对电液伺服机构-柔性接头系统动态特性的影响。分析结果表明:电液伺服机构-变刚度变阻尼模型所构造的迟滞曲线可更准确地与实验结果相吻合,并符合迟滞曲线随频率变化的规律,反馈系数、放大器静态放大系数、电液伺服机构增益、滑阀流量增益等参数对系统动态特性的影响更为明显。该模型为固体火箭发动机电液伺服机构-柔性接头系统动态特性的调整提供理论依据。     

基于轨道角动量的电磁涡旋SAR成像新方法

为研究电磁涡旋波在合成孔径雷达(SAR)领域的应用潜力,验证电磁涡旋SAR成像的可行性,将电磁涡旋与合成孔径雷达模型结合,通过使用单一模式的轨道角动量,用合成孔径原理实现方位聚焦。给出了基于电磁涡旋的SAR几何模型和回波信号模型,并提出了适用于电磁涡旋SAR的改进chirp-scaling(CS)成像算法。通过点目标仿真分析,验证了所提成像算法的有效性。该方法可为SAR系统新体制设计及雷达的研究提供参考。     

全模颤振双索悬挂系统刚体模态频率研究

研究绳系结构和绳索预紧力对全模颤振双索悬挂系统刚体模态频率的影响。首先，基于绳索并联机构理论，对双索悬挂系统进行静力学建模，引入加权矩阵，推导了双索悬挂系统静刚度模型；其次，建立双索悬挂系统无阻尼振荡方程，分析双索悬挂系统刚体模态频率变化规律；进而，搭建了双索悬挂系统地面样机，开展系统模态频率测试试验，研究系统刚体模态频率的影响因素及其变化规律；最后，参考试验结果修正所建数学模型。结果表明，随着绳索预紧力的增加，系统刚体模态频率呈上升趋势，但各阶刚体模态的固有频率上升速率不同，平动模态的固有频率受绳索预紧力影响比转动模态小得多；在转动模态方面，滚转模态的固有频率最大且上升快；在平动模态方面，升沉模态的固有频率大于横侧滑模态的固有频率；双索经过的机身前后滑轮与飞机模型质心之间的相对位置变化会不同程度地影响支撑系统俯仰模态、偏航模态的固有频率，但几乎不影响其滚转模态的固有频率。研究发现，通过控制悬挂绳索预紧力的大小，合理设计机身上的滑轮安装位置，能够有效降低双索悬挂系统刚体模态频率。研究结果对于优化设计全模颤振双索悬挂系统具有指导意义。     

Predicting performance in manually controlled rendezvous and docking through spatial abilities

Manually controlled rendezvous and docking (manual RVD) is a challenging space task for astronauts. This study aims to identify spatial abilities that are critical for accomplishing manual RVD. Based on task analysis, spatial abilities were deduced to be critical for accomplishing manual RVD. 15 Male participants performed manual RVD task simulations and spatial ability tests (the object-manipulation spatial ability and spatial orientation ability). Participants’ performance in the test of visualization of viewpoints (which measures the spatial orientation ability) was found to be significantly correlated with their manual RVD performance, indicating that the spatial orientation ability in the sense of perspective taking is particularly important for accomplishing manual RVD.     

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.     

Characterization of ionospheric amplitude scintillations using wavelet entropy detrended GNSS data

The extensive monitoring networks of Global Navigation Satellite System (GNSS) ionospheric scintillation have been established to continuously log observation data. Further, the amplitude scintillation index and the phase scintillation index, which are derived from scintillation observations, are anticipated to accommodate the accuracy requirement of both the user level and the monitoring station level. However, raw scintillation observations essentially measure superposed waveform impairments of GNSS signals propagating through ionosphere and troposphere. It implies that fluctuations of raw scintillation observations are caused by multiple factors from the entire radio propagation environment. Hence, it is crucial to characterize ionospheric scintillations from GNSS observation data. And the characterization is implemented through extracting fluctuations of raw observations merely induced by ionospheric scintillations. Designed to address this problem by means of Fourier filtering detrending, the present work investigates the influence of varying detrending cutoff frequencies on wavelet statistical energy and wavelet entropy distributions of scintillation data. It consequently derives criteria on the optimum detrending cutoff frequency for three types of raw amplitude scintillation data, which are classified by their wavelet energy distributions. Results of the present work verify that detrending with specific optimum cutoff frequencies rather than the fixed and universally applicable one renders the validity and credibility of characterizing ionospheric scintillations as the part of GNSS observation fluctuations purely induced by ionosphere electron density irregularities whose scale sizes are comparable with or smaller than the Fresnel scale.     

NVNA谐波相位检验件设计及定标

本文介绍了一种用于检验非线性网络分析仪谐波相位指标的检验件设计方法，并搭建了基于实时示波器的测量系统对谐波相位进行定标。通过高速实时示波器对检验件的输出信号进行采样，利用傅立叶变换提取谐波相位信息。为了得到高准确度的测量结果，采用去缠绕、最小二乘等算法对相位结果进行优化处理。实验结果表明，该方法可以作为NVNA谐波相位指标的验证手段对NVNA的谐波相位进行验证。     

Sliding mode control design for oblique wing aircraft in wing skewing process

When the wing of Oblique Wing Aircraft (OWA) is skewed, the center of gravity, inertia and aerodynamic characteristics of the aircraft all significantly change, causing an undesirable flight dynamic response, affecting the flying qualities, and even endangering the flight safety. In this study, the dynamic response of an OWA in the wing skewing process is simulated, showing that the three-axis movements of the OWA are highly coupled and present nonlinear characteristics during the wing skewing. As the roll control efficiency of the aileron decreases due to the shortened control arm in an oblique configuration, the all-moving horizontal tail is used for additional roll and the control allocation is performed based on minimum control energy. Given the properties of pitch-roll-yaw coupling and control input and state coupling, and the difficulty of establishing an accurate aerodynamic model in the wing skewing process due to unsteady aerodynamic force, a multi-loop sliding mode controller is formulated by the time-scale separation method. The closed-loop simulation results show that the asymmetric aerodynamics can be balanced and that the velocity and altitude of the aircraft maintain stable, which means that a smooth transition is obtained during the OWA’s wing skewing.