基于滤波扩张观测器的有限时间收敛制导律

为提高拦截机动目标的精度,基于滤波扩张状态观测器提出了一种考虑自动驾驶动态特性的有限时间收敛制导律.通过滤波扩张状态观测器对制导律中目标机动信息进行补偿,使导弹在拦截目标时具有更高的拦截精度.仿真结果表明,在目标机动情况下,设计的制导律能保证视线角速度在有限时间内收敛到零,拦截弹过载较小,具有较好的动态特性和鲁棒性.同时与普通的扩张观测器的估计结果相比,滤波扩张状态观测器对机动目标的跟踪效果较佳.     

再入航天飞机表面热流密度辨识

本文给出了求解表面热流密度辨识这一热传导逆问题的顺序函数法。然后以某模型航天飞机迎风中心线上的某特征点为例，将航天飞机再入时的表面热流密度辨识问题简化为一维模型问题，用顺序函数法来对该特征点上的对流加热流密度进行了仿真辨识，得到了较理想的辨识结果。该方法在航天研究领域有着良好的工程应用前景。     

N2O4／UDMH火球特性的实验与理论研究

本文对液体推进剂四氧化二氮／偏二甲肼（Ｎ２Ｏ４／ＵＤＭＨ）爆炸热过程特性进行了实验与理论研究。研究结果显示出了火球尺寸变化、火球持续时间、火球内部温度、火球辐射热流传递过程等热过程特性参数随推进剂重量、时间和空间位置的变化规律。理论预测结果与实验测量结果相比符合较好，表明理论预测模型的正确性。本文还讨论了火球升离地面的临界条件、高空环境对火球直径的影响和火球随风漂移等三方面的问题。     

红外加热笼模拟航天器瞬变外热流的方法研究

文章以某型号航天器热平衡试验为工程应用背景,采用理论分析、仿真研究和实验研究相结合的方法,建立了红外加热笼和热流计的动态数学模型。在此基础上,讨论了利用红外加热笼作为热流模拟元件,绝热型热流计作为测量元件,模拟航天器在轨飞行时表面到达热流密度瞬态变化的方法和技术。     

Analysis of the Micrometeoroid and Debris Hazard Posed to an Orbiting Parabolic Mirror

Many concepts of future space systems involve the use of parabolic mirrors for optical applications. The need for a highly reflective finish means that performance of such systems will be particularly vulnerable to space debris and micrometeoroids. A case study was performed to examine the micrometeoroid and debris hazard posed to an orbiting parabolic mirror. The mirror considered was nominally Earth-pointed in a circular orbit with two candidate altitudes in low Earth orbit (LEO), well within the region inhabited by man-made debris. The timeframes of interest for the two missions were 2002–2004 and 2005–2015. Microgram and larger particles were considered.To perform this study, it was necessary to determine the debris and meteoroid flux across the parabolic surface. To assess sensitivity of results to uncertainity in available data, two approaches were taken. The first approach was an analytical procedure based on use of long duration exposure facility (LDEF) data and published theoretical results. The second approach used two readily available computer models: the ESA MASTER model and NASA's ORDEM96. In addition, an in-house implementation of the Grün meteoroid model was used. While multiple results were available for the total flux and flux distributed over azimuth, only the MASTER model was available for generating the desired elevation data to obtain the flux distribution over the parabolic mirror. In an attempt to bound the uncertainty in the knowledge of the elevation distribution, the results from both the MASTER and ORDEM96 models were processed together to form a separate, hybrid prediction. In addition, results were used in the preliminary design of a protective skirt.This case study elucidated the practical obstacles and considerations in performing a sufficiently accurate debris and meteoroid analysis using data and tools that are readily available to the broad space sector. The resulting procedures are useful in the assessment of the risk posed to optics by the meteoroid and debris environment and in the design of protection.     

液晶热图技术在脉冲风洞中的应用

在短时间脉冲风洞中,对液晶热图实验技术进行了试验。在实验时间为20ms的炮风洞中,获得了清晰的三维高超声速分离流场的热图显示照片。热图照片不仅与油流图谱所显示的特征位置吻合,而且能半定量地显示表面热流的分布。该项技术的研究为国内空气动力学实验研究提供了一项新的方法。     

Analysis on capabilities of density-based solvers within OpenFOAM to distinguish aerothermal variables in difusion boundary layer

Open source feld operation and manipulation（OpenFOAM）is one of the most prevalent open source computational fluid dynamics（CFD）software.It is very convenient for researchers to develop their own codes based on the class library toolbox within OpenFOAM.In recent years,several density-based solvers within OpenFOAM for supersonic/hypersonic compressible flow are coming up.Although the capabilities of these solvers to capture shock wave have already been verifed by some researchers,these solvers still need to be validated comprehensively as commercial CFD software.In boundary layer where diffusion is the dominant transportation manner,the convective discrete schemes＇capability to capture aerothermal variables,such as temperature and heat flux,is different from each other due to their own numerical dissipative characteristics and from viewpoint of this capability,these compressible solvers within OpenFOAM can be validated further.In this paper,frstly,the organizational architecture of density-based solvers within OpenFOAM is analyzed.Then,from the viewpoint of the capability to capture aerothermal variables,the numerical results of several typical geometrical felds predicted by these solvers are compared with both the outcome obtained from the commercial software Fastran and the experimental data.During the computing process,the Roe,AUSM＋（Advection Upstream Splitting Method）,and HLLC（Harten-Lax-van Leer-Contact）convective discrete schemes of which the spatial accuracy is 1st and 2nd order are utilized,respectively.The compared results show that the aerothermal variables are in agreement with results generated by Fastran and the experimental data even if the1st order spatial precision is implemented.Overall,the accuracy of these density-based solvers can meet the requirement of engineering and scientifc problems to capture aerothermal variables in diffusion boundary layer.     

上面级发射中高轨道卫星外热流分析

研究发射轨道的外热流是卫星热控制系统设计的基础。针对上面级发射轨道的特点和卫星姿态，推导出上面级滑行段和点火段瞬态及平均外热流计算公式。以北斗三号中轨导航卫星为例，给出了阳光和轨道面夹角随太阳黄经和升交点赤经的变化关系，以及最长阴影时间、滑行段旋转角速度约束条件的分析方法，在此基础上确定了上面级阶段卫星的极端外热流工况并给出了外热流计算结果。     

尾迹对涡轮动叶全表面气膜冷却效率的影响

采用压敏漆（PSP）测量技术研究了尾迹对涡轮动叶气膜冷却效率的影响，测试叶片带有11排圆柱形气膜孔。获得了不同质量流量比和尾迹斯特劳哈尔数（Sr=0，0.12，0.36）条件下全表面气膜冷却效率分布的试验数据，结果表明：随着尾迹Sr数的增加，叶片前缘区域径向平均气膜冷却效率最大降低幅度达36.5%，吸力面径向平均气膜冷却效率最大降低幅度达53.5%，压力面径向平均气膜冷却效率最大降低幅度达24.2%；尾迹对前缘和吸力面气膜冷却效率的影响大于压力面；随着质量流量比增加，尾迹的影响减小；在进行涡轮动叶表面气膜冷却结构设计时，不考虑尾迹效应会增加设计风险。     

The electron formations under the radiation belts at L-shells 1.2–1.9

We continue to analyze the distribution of electron fluxes with energy 30–500 keV under the radiation belts at low and middle latitudes (L = 1.2–1.9) using experimental data obtained onboard ACTIVE satellite. Special attention is given to altitudinal distribution of electron fluxes and detailed analysis of these electron formations. We observe three main regions of electron flux registration that seem to exist constantly under the radiation belts. These regions are: magneto-conjugated to SAA region (in the north hemisphere), local zone of low intense electron flux accumulation to the west of SAA, and extensive region in the north hemisphere to the east. The analysis of experimental data obtained from ACTIVE satellite (orbit height 500–2500 km) shows that electron fluxes are registered in the wide altitude range up to 1100 km. It is shown that these formations have complicated initial structure with two regions of flux maximums: at L = 1.3 and L = 1.6–1.8. We compare particle data with low frequency (LF) data (ARIEL-4 satellite) and high frequency (HF) data (CORONAS-I satellite). Also we discuss the possible mechanisms of the appearance of these formations under the radiation belts.