Influences of the turbulence model and the slot width on the transverse slot injection flow field in supersonic flows

Transverse slot injection scheme is very important for the mixing process between the air and the fuel in supersonic flows. The effect of the turbulence model and slot width on the transverse slot injection flow field has been investigated numerically based on the grid independency analysis, and the predicted results have been compared with the experimental data available in the open literature. The obtained results show that the grid scale makes only a slight difference to the wall pressure profiles for all jet-to-crossflow pressure ratios employed in this study, and the wall pressure profile with low jet-to-crossflow pressure ratio is predicted accurately by the RNG k–ε turbulence model, the SST k–ω turbulence model for the flow field with high jet-to-crossflow pressure ratio. High jet-to-crossflow pressure ratio can increase the jet penetration depth in supersonic flows, and the gradient of the length of the upstream separation region is larger than that of the height of the Mach surface. At the same time, when the jet-to-crossflow pressure ratio is maintained constant, the jet penetration depth increases with the increase of the slot width.     

Spatial approaches to moons from resonance relative to invariant manifolds

In this study, the final approach to a moon or other body from resonance is explored and compared to the invariant manifolds of unstable periodic orbits. It is shown that the stable manifolds of planar Lyapunov orbits can act as a guide for the periods or resonances that are required for the final approach in both the planar and spatial problems. Previously developed techniques for the planar problem are expanded for use with resonances and used for comparison with trajectories approaching a moon from these resonances. A similar technique is then used for exploring the relationship of invariant manifolds to approach trajectories in the spatial problem. It is shown that the invariant manifolds of unstable periodic orbits provide insight into the trajectory design, and they can be used as a guide to the more direct approach trajectories.     

迎角变化引起的高超声速进气道起动迟滞现象试验研究

高超声速进气道在起动过程中存在迟滞现象，起动迟滞对发动机的工作范围有重要影响。以一种Bump/前体一体化进气道为研究对象，通过试验和数值仿真结合的方法，研究迎角变化引起的进气道起动迟滞现象。试验在国防科技大学LF-220自由射流风洞中进行，来流条件Ma=5.0，采用蓄热式加热器对上游气流进行加热，稳定段总压1.59MPa，试验段静温91.67K。试验模型由底座、进气道前体前锥、进气道前体后锥和唇罩4部分组成，模型总长度285mm。采用PSI压力传感器对模型壁面压力进行测量，采样频率为100Hz。试验成功捕捉到进气道随迎角变化由不起动转化为起动的动态过程。研究表明，高超声速进气道随迎角变化存在明显的迟滞现象。试验获得进气道自起动迎角为-1.3°，而进气道自不起动迎角大于10°。在进气道自起动/自不起动过程的研究中发现，随着进气道流动状态的不同，迎角和大尺度分离区交替主导流量变化。     

弹道跟踪数据野值剔除方法性能分析

弹道跟踪数据中的野值会影响导弹目标定位精度。对用于弹道跟踪数据的野值剔除方法进行了综述。结合事后和实时两大类处理模式,分析了各野值剔除方法在理论和工程应用上的优缺点,给出了实际应用时的限制因素,建立了野值判决准则和相应的野值剔除实现步骤。仿真结果表明:野值剔除方法可以有效提高弹道跟踪数据的精度。事后处理模式中,基于格拉布斯准则的野值剔除效果最佳;实时处理模式中,基于自适应门限的五点线性预报法野值剔除效果相对较好,且时间复杂度相对较低,适合实时处理。     

Electromagnetic dissociation and space radiation

Relativistic nucleus–nucleus reactions occur mainly through the strong or electromagnetic (EM) interactions. Transport codes often neglect the latter. This work shows the importance of including EM interactions for space radiation applications.     

基于实测星载原子钟数据的脉冲星守时方法

利用脉冲星估计星载原子钟钟差是实现卫星自主守时的途径之一。为充分分析基于脉冲星的自主守时系统性能，利用实测的星载原子钟钟差数据和中子星内部组成探测器(neutron star interior composition explorer, NICER)的PSR B1937+21脉冲星的观测数据，对比分析了星载原子钟和脉冲星的误差特性。设计了脉冲星守时系统框架和星载原子钟钟差估计方法。以实测的星载原子钟钟差数据为基础，计算分析了脉冲星守时系统的性能。计算结果表明，若脉冲星的脉冲到达时间（time of arrival, TOA）解算精度为1 μs/30 d，则原子钟钟差估计精度可达到优于1 μs的水平，初步验证了脉冲星守时系统的可行性。     

A non-local vectorial total variational model for multichannel SAR image speckle suppression

This paper aims at the multichannel synthetic aperture radar(SAR)image speckle reduction.This paper proposes a novel energy minimized regularization model for multichannel image denoising,which is an extension of the non-local total variational model for gray-scale image.It contains two terms,namely the vectorial data fidelity term and the non-local vectorial total variation term.The latter is constructed by high-dimensional non-local gradient that contains the structure information of the multichannel image.The existence and the uniqueness of the solution of the model are proved.A fixed point iterative algorithm is designed to acquire the solution of this model.The convergence property of this algorithm is proved as well.This model is applied to the multipolarimetric and multi-temporal RADARSAT-2 images despeckling.The result shows that this model performs better than the original vectorial total variational model on texture preserving.     

基于机械飞轮干扰补偿的小卫星自适应滑模变结构姿态控制

针对机械飞轮内干扰可能导致小卫星姿态控制系统性能下降问题,提出了一种加入机械飞轮干扰补偿的自适应滑模变结构姿态控制方法.本文针对基于机械飞轮的三轴稳定卫星姿态控制系统,首先建立系统详细的数学模型,包括基于机械飞轮的三轴稳定卫星姿态动力学方程和机械飞轮控制系统模型,然后针对此系统设计了一种基于机械飞轮干扰补偿的自适应滑模变结构控制器,其中通过设计一种状态观测器得到机械飞轮摩擦干扰的估计值,用于对机械飞轮摩擦干扰的补偿,并通过Lyapunov定理证明了此控制律能保证系统的渐近稳定性.最后仿真结果显示,此方法缩短了飞轮转速过零时间,降低了最大的姿态扰动量且提高了卫星姿态控制的精度和稳定度.     

基于目标分解和SVM的极化SAR图像分类方法

极化SAR图像分类是新体制雷达应用研究中的一类基础前沿问题。文章提出了一种基于目标分解及支持矢量机(Support Vector Machine,SVM)的极化SAR图像分类方法。首先根据Cloude分解和Freeman分解两种方法提取极化SAR图像的多类散射特征,从而构造出图像各像素的特征向量。接着利用样本区域像素的特征向量对SVM进行训练,获得经训练的SVM。最后,以各待分类像素的特征向量为输入,利用经训练的SVM即可完成极化SAR图像的分类。对两幅AIRSAR实测极化SAR图像数据分类的结果表明,文章方法能够有效地利用多类散射特征的互补信息,具有较高的分类精度。