卫星线阵立体影像的倾斜仿射变换核线模型

核线约束是构建摄影测量立体模型的重要条件。由于卫星线阵影像的多中心投影特性,难以建立其严格的核线模型。文章从上下视差最小的同名核线特征出发,在仿射变换模型基础上引入核线倾角变化参数,提出一种新的倾斜仿射变换核线模型。通过“无误差”的虚拟同名点仿真试验表明,文章提出的模型受影像范围及地表高差影响较小,在影像区块6 000像元×6 000像元、地表高差1 000m情况下,对于不同形式卫星立体影像的模型误差均小于1个像元。进一步使用实际匹配同名点平差,实验表明：对于SPOT-5、“资源三号”和“高分七号”等卫星影像,文章模型误差相对于匹配观测误差可忽略,实际核线精度在整景影像范围内优于0.8像元,所生成核线影像能够满足后续密集匹配要求。新模型的精确性和普适性相比现有同类模型显著提升,可实际应用于卫星摄影测量处理。     

环型与线型聚能装药射流成型机理对比

环型聚能装药药型罩2侧在挤压汇聚形成射流过程中存在不对称性,不能完全套用线型聚能装药射流成型的现有理论。利用DYNA3D软件对相同剖面结构的环型、线型聚能装药射流成型过程进行数值模拟,通过比较分析得出了环型聚能装药形成杵体及射流参数的分布特性,为进一步理论研究及工程应用提供参考。     

Direct position determination using single moving rotating linear array: Noncoherent and coherent processing

To improve the resolution and accuracy of Direct Position Determination (DPD), this paper investigates the problem of positioning multiple emitters directly with a single moving Rotating Linear Array (RLA). Firstly, the geometry of the RLA is formulated and analysed. According to its geometry, the intercepted noncoherent signals in multiple interception intervals are modeled. Correspondingly, the MUltiple SIgnal Classification (MUSIC) based noncoherent DPD approach is proposed. Secondly, the synchronous coherent pulse signals are individually considered and formulated. And the coherent DPD approach which aims for localizing this special type of signal is presented by stacking all array responses at different interception intervals. Besides, we also derive the constrained Cramér-Rao Lower Bound (CRLB) expression for both noncoherent and coherent DPD with RLA under the constraint that the altitudes of the emitters are known. At last, computer simulations are included to examine the performance of the proposed approach. The results demonstrate that the localization accuracy and resolution of DPD with single moving linear array can be significantly improved by the array rotation. In addition, coherent DPD with RLA further improves the resolution and increases the maximum emitter number that can be localized compared with the noncoherent DPD with RLA.     

Families of halo orbits in the elliptic restricted three-body problem for a solar sail with reflectivity control devices

Solar sail halo orbits designed in the Sun-Earth circular restricted three-body problem (CR3BP) provide inefficient reference orbits for station-keeping since the disturbance due to the eccentricity of the Earth’s orbit has to be compensated for. This paper presents a strategy to compute families of halo orbits around the collinear artificial equilibrium points in the Sun-Earth elliptic restricted three-body problem (ER3BP) for a solar sail with reflectivity control devices (RCDs). In this non-autonomous model, periodic halo orbits only exist when their periods are equal to integer multiples of one year. Here multi-revolution halo orbits with periods equal to integer multiples of one year are constructed in the CR3BP and then used as seeds to numerically continue the halo orbits in the ER3BP. The linear stability of the orbits is analyzed which shows that the in-plane motion is unstable while the out-of-plane motion is neutrally stable and a bifurcation is identified. Finally, station-keeping is performed which shows that a reference orbit designed in the ER3BP is significantly more efficient than that designed in the CR3BP, while the addition of RCDs improve station-keeping performance and robustness to uncertainty in the sail lightness number.     

Accurate approximation of in-ecliptic trajectories for E-sail with constant pitch angle

Propellantless continuous-thrust propulsion systems, such as electric solar wind sails, may be successfully used for new space missions, especially those requiring high-energy orbit transfers. When the mass-to-thrust ratio is sufficiently large, the spacecraft trajectory is characterized by long flight times with a number of revolutions around the Sun. The corresponding mission analysis, especially when addressed within an optimal context, requires a significant amount of simulation effort. Analytical trajectories are therefore useful aids in a preliminary phase of mission design, even though exact solution are very difficult to obtain. The aim of this paper is to present an accurate, analytical, approximation of the spacecraft trajectory generated by an electric solar wind sail with a constant pitch angle, using the latest mathematical model of the thrust vector. Assuming a heliocentric circular parking orbit and a two-dimensional scenario, the simulation results show that the proposed equations are able to accurately describe the actual spacecraft trajectory for a long time interval when the propulsive acceleration magnitude is sufficiently small.     

平面叶栅尾流板开孔率对跨声速涡轮叶栅流道影响的数值分析

跨声速平面叶栅风洞中通常通过尾流板来改善平面叶栅周期性,针对尾流板的设计需求,利用数值模拟的方法,研究了尾流板在15%、30%、50%开孔率下对实验叶栅的影响。数值分析结果表明:叶栅尾缘激波在自由边界上反射后,返回到叶栅通道中,破坏了叶栅通道的周期性;开槽尾流板减少了反射波对叶栅通道的影响,减弱叶栅尾缘激波的反射波强度,在某特定情况下能使反射波变成膨胀波,从而提高了叶栅通道周期性;尾流板开孔率为15%时能极大地改善平面叶栅通道的周期性,相对于开孔率为50%时叶栅的周期性误差降低约16.43%。      

基于模型补偿的风力机变桨距线性自抗扰控制器设计

设计了一种变桨距线性自抗扰控制器,估计和补偿了系统未建模部分和外界干扰,实现额定风速以上时系统输出功率稳定于额定值;并采用模型补偿方法对自抗扰控制器进行优化,减少了参数整定的数目,提高了系统控制精度。对额定功率为300 kW的风电机组分别在阶跃风、阵风以及湍流风作用下进行系统仿真。结果表明,该方法可以快速调节风速变化引起的输出波动,使得系统输出稳定且超调量小,具有很好的稳定性和鲁棒性。     

一种高光谱图像的双压缩感知模型

高光谱图像因其海量数据性,给存储、传输及后续分析处理带来了挑战。压缩感知理论提供了一种全新的信号采集框架。针对高光谱数据的三维特性,提出一种双压缩感知的采样与重构模型。该模型在采样阶段兼顾高光谱数据的空间和谱间稀疏特性,构造了能同时实现空间和谱间压缩采样的感知矩阵;重构阶段不同于传统的压缩感知重构方法直接重构高光谱数据,而是将高光谱数据分离成端元和丰度分别进行重构,然后利用重构的端元和丰度信息合成高光谱数据。实验结果表明,所提双压缩感知在低采样率下重构精度较三维压缩采样提高了10 dB以上,更为显著的是运算速度提升了3个数量级,同时该方法还便于获得端元和丰度信息。     

基于LPV状态空间模型的小型航空煤油二冲程发动机喷油控制策略

为了简化基于平均值模型的喷油控制模型的计算,根据线性变参数(LPV)状态空间模型原理,在平均值模型的基础上建立了LPV状态空间喷油控制模型,利用Matlab/Simulink工具对稳态工况和瞬态工况的喷油脉宽控制模型进行仿真,最后在发动机试验台架上进行试验验证.仿真和试验结果表明:①基于LPV状态空间模型的喷油控制模型能够满足瞬态工况和稳态工况控制的要求,计算的喷油脉宽精度略低于平均值模型,由于LPV状态空间模型计算简单,能够直接应用于控制算法的设计,因此在工程中容易实现.②与插值算法相比,基于LPV状态空间模型的控制策略使发动机的动力输出有所下降,主要是由于模型简化造成进气空气流量减小引起的.