斜出口合成射流激励器横流输运特性与边界层控制

研制了一种斜出口合成射流(BSJ)激励器,应用粒子图像测速(PIV)技术获得了合成射流的瞬态和时均流动结构,分析比较了斜出口和常规平直出口激励器流场的异同。该斜出口激励器能将周围气体进行有方向的能量和质量输送控制,时均流场呈现沿壁面的横向流动输运特性。解释了横向流动输运的形成机理,并应用该激励器进行了边界层控制实验。研究结果表明:通过改变激励器的工作电压和频率,可方便有效地实现对平板边界层速度型的调控,使受控边界层速度型更"饱满",这对控制推迟边界层分离非常有利。     

真空热试验中闭环温度控制参数分析

为了满足航天器真空热试验温度控制的新要求,文章通过对控制参数与温度控制设定目标值之间数值关系的分析与研究,得出通过电阻性加热器加热、以辐射换热为主要加热途径的温控系统对象,最优比例参数Kc值与目标设定温度成近似正比关系,积分参数Ti值可取固定值,微分参数Td对控制动态品质影响可忽略。具有上述特性的系统可使用参数寻找方法:即在真空热试验之前通过热响应曲线套用公式确定该对象的数学模型,然后使用数值分析的方法,寻找最优的PID参数。通过这种预先估计PID控制参数方法,可以改善电阻特性类控温系统的控制品质。     

“2010.8.24”飞机积冰过程分析

通过对2010年8月24日积冰过程的分析得出:这次积冰发生地点附近为垂直运动上升区,配合云中密集的冰水混合物,是造成这次飞机严重积冰的主要原因。积冰指数对于积冰强度和区域的预报具有指示意义。WRF中尺度数值模式选用Eta Ferrier微物理方案的模式结果中的云冰、云水以及总凝结混合比,这对于积冰强度和范围有一定的预报能力。     

基于贝叶斯网络的航空灾害成因机理探析

为了预防和矫正航空事故诱发因素的萌生与发展,改善民航安全管理的科学性和可靠性,进一步降低事故率,减少航空灾害造成的损失.针对航空灾害的形成特点,探讨致灾因素的相互作用是成因机理分析的关键.基于贝叶斯网络模型,综合运用诊断推理和支持推理形式,分析致灾因素的因果关系,揭示了人、机、环境与管理因素相互作用的内在规律.通过高斯贝叶斯网络在典型案例致灾成因机理分析中的应用,挖掘隐含的内部因素对系统的影响程度,发现了隐含因素从不确定性状态向确定性状态的演变过程,以及表层因素与隐含因素的关系.     

Ultrasonic Computed Tomography Imaging Method of Concrete Materials Based on Simulated Annealing Genetic Algorithm

Stability and accuracy of the imaging results are still unmet practical demands for ultrasonic computed tomography(CT)of concrete material.To address these issues,a CT technique based on simulated annealing genetic algorithm(SAGA)is presented in this work.Firstly,a natural weight matrix with clear physical meaning is introduced in the inverse algorithm and then a quadric broadening objective function is formed according to the propagation characteristics of ultrasound in concrete.After that,the simulated annealing(SA)searching is added to speed up the inverse process and to improve the convergence and stability of the algorithm.Finally,the optimal inverse imaging results have been achieved by variable ectopic adaptive genetic algorithm.The numerical simulation experiments have shown that the usage of the correct priori information and the excellent characteristic of SAGA in searching the global minimum value of the function have produced accurate and effective results with stable numerical values.The imaging resolution is improved and the imagining results reflecting the inner defections of the tested objects are more reliable and accurate.     

一种基于航空器气象资料下传数据的飞行剖面生成方法

由于飞行剖面识别是航空器四维(Four-dimensional,4D)航迹预测研究的热点问题,提出一种基于航空器气象资料下传(Aircraft meteorological data relay,AMDAR)数据的全飞行过程剖面生成方法,包括由高度-航程构成的标称高度剖面和空速-航程构成的标称速度剖面。首次将动态空间规整算法(Dynamic space warping,DSW)应用到飞行高度剖面的相似距离计算中,计算出标称飞行高度剖面;为解决在地速未知情况下标称速度剖面的计算问题,结合大椭圆距离算法与航空器基本性能数据库(Base of aircraft data,BADA),给出一种标称飞行速度剖面的计算方法,该方法保留了AMDAR实测历史数据中所隐含的飞行意图与气象因素。实际算例表明,本文提出的方法能够有效地得到真实反映航空器飞行状态的全飞行剖面。     

Optical/radio/pulsars integrated navigation for Mars orbiter

In this paper, we address the issue of the integrated navigation algorithm with different combination of measurements for Mars orbiter. First, system dynamic model and navigation measurement models using optical measurement information, radio measurement information and X-ray pulsars measurement information are respectively established. Second, optical/radio/pulsars integrated navigation algorithm is proposed, and observability analysis of the integrated navigation system is also conducted. Third, adaptive extended Kalman filter is adopted to fuse measurement information and suppress measurement and process noise to optimally estimate the state of Mars orbiter. Monte Carlo simulation results show that optical/radio/pulsars integrated navigation can effectively improve the navigation accuracy and satisfy the navigation requirements of Mars orbiter.     

Enrichment of the Hot Intracluster Medium: Observations

Four decades ago, the firm detection of an Fe-K emission feature in the X-ray spectrum of the Perseus cluster revealed the presence of iron in its hot intracluster medium (ICM). With more advanced missions successfully launched over the last 20 years, this discovery has been extended to many other metals and to the hot atmospheres of many other galaxy clusters, groups, and giant elliptical galaxies, as evidence that the elemental bricks of life—synthesized by stars and supernovae—are also found at the largest scales of the Universe. Because the ICM, emitting in X-rays, is in collisional ionisation equilibrium, its elemental abundances can in principle be accurately measured. These abundance measurements, in turn, are valuable to constrain the physics and environmental conditions of the Type Ia and core-collapse supernovae that exploded and enriched the ICM over the entire cluster volume. On the other hand, the spatial distribution of metals across the ICM constitutes a remarkable signature of the chemical history and evolution of clusters, groups, and ellipticals. Here, we summarise the most significant achievements in measuring elemental abundances in the ICM, from the very first attempts up to the era of XMM-Newton, Chandra, and Suzaku and the unprecedented results obtained by Hitomi. We also discuss the current systematic limitations of these measurements and how the future missions XRISM and Athena will further improve our current knowledge of the ICM enrichment.     

纺织结构复合材料的细观力学分析

纺织结构复合材料细观力学分析中的若干基本问题是单层几何特性的描述，单元体细观结构的模型、应力应变假设以及强度分析等。对前人在前三个问题上已进行的研究工作作出扼要的回顾，并介绍其当前的技术发展动态，针对这些研究工作中存在的不足之处和未来的发展，提出几点意见。