一种不依赖剩余时间估计的巡航导弹多约束制导律

针对巡航导弹末段多约束精确打击问题,提出了一种不依赖剩余时间估计的攻击角度/时间制导律。推导了航向弹目相对运动关系,设计了一种基于附加航向角设计的时间约束制导律,通过对时间增益系数的设计和优化,实现附加航向角的调节,可使实际飞行时间向期望时间快速收敛;在此基础上,将角度约束制导律与时间约束制导律相结合,得到了一种角度/时间约束制导律。该制导律不依赖于剩余时间估计,进而实现多约束条件下航向轨迹自适应调整;通过求解偏置导引律闭环轨迹分析得到轨迹收敛条件,给出满足角度/时间约束制导律的显式收敛条件。最后通过数学仿真验证了本文提出的航向多约束制导律可满足时间和角度等多约束条件且具有快速收敛特性。     

非均匀入口与化学非平衡效应对尾喷管性能的影响研究

基于煤油燃料超燃冲压发动机尾喷管,对均匀入口和非均匀入口、冻结流动模型和化学非平衡模型下的尾喷管内流动进行数值模拟,采用两方程RNG k-ε湍流模型对三维NS方程组进行求解,获得非均匀入口与化学非平衡效应对尾喷管性能的影响。计算结果表明,尾喷管内流动非均匀性由尾喷管非对称膨胀和燃烧室出口非均匀等因素构成,尾喷管入口流动参数非均匀分布对尾喷管推力、升力及俯仰力矩均有影响,算例中非均匀入口使得尾喷管净推力相对于均匀入口增加了1.2%左右;尾喷管性能受化学非平衡效应的影响,非平衡流动模型下的其净推力计算结果相对于冻结流动模型增加3%~4%。     

大型回流边界层风洞的气动与结构设计

大型边界层风洞是开展风工程研究的必备装备。以浙江大学ZD-1边界层风洞的研制为背景,详细介绍了大型回流边界层风洞气动设计和立式结构设计中的关键问题,在风洞气动设计时采用了收缩比为4∶1的单回路单试验段气动轮廓,在试验段中设置了0．22°的当量扩散角,对拐角导流片外形作了特殊处理,并采用钢结构与混凝土结构相结合的立式结构。流场校验结果表明,大型回流边界层风洞的气动与结构设计能满足设计要求,某些指标甚至达到航空风洞的标准,在试验段中设置扩散角有利于降低轴向静压梯度,立式结构设计对提高试验段气流的水平均匀性有一定的作用,可为今后类似风洞的研制提供参考。     

POSS 催化剂改性氰酸酯复合材料的性能

通过POSS 催化剂改性氰酸酯树脂,并采用热熔法排布制备了碳纤维/ 中温固化氰酸酯预浸料, 验证了改性氰酸酯的工艺性。同时考察了氰酸酯树脂及其复合材料的性能。结果表明, POSS 催化剂的加入, 降低了氰酸酯的固化温度,同时其使用温度、室温及-18℃的储存性能和复合材料力学性能与改性前相当。     

基于A320飞机横航向控制律架构的LQ设计

空客A320飞机横航向控制律采用特征结构配置方法计算闭环增益,实现了期望特征值的配置及横航向关键参数之间的解耦。基于A320横航向控制律架构,提出使用线性二次型(Linear Quadratic,简称LQ)方法,对闭环增益进行重新设计。首先根据期望的特征值引入关键参数的频域整形环节,而后通过调整二次型性能指标加权矩阵实现期望特征值的逼近及关键参数之间的解耦,并求得闭环反馈增益,最后在特征结构、稳定裕度和横航向解耦效果方面与空客设计结果作了对比分析。仿真结果表明,LQ设计可获得与特征结构配置设计相近的结果,即得到接近期望值的特征值,并实现关键变量的解耦,同时保证了闭环稳定裕度。     

BAMO-THF叠氮型热塑性聚氨酯弹性体的合成与表征

为了研究叠氮型热塑性含能粘合剂的合成方法及反应条件对其力学性能的影响,通过熔融预聚二步法合成了以3,3-双(叠氮甲基)环氧丁烷-四氢呋喃共聚醚(BAMO-THF)为软段、异佛尔酮二异氰酸酯(IPDI)及1,4-丁二醇(BDO)为硬段的叠氮型热塑性聚氨酯弹性体(ATPE)。采用傅立叶变换红外光谱(FTIR)对所制备的ATPE的结构进行了表征。通过二正丁胺滴定法确定了最佳的预聚反应时间。研究比较了固化参数R和硬段含量对ATPE力学性能的影响。利用差示扫描量热(DSC)测定了ATPE的玻璃化转变温度,计算了硬段溶于软段的百分数。研究结果表明,所合成的ATPE具有典型的叠氮聚醚聚氨酯特征;确定了预聚反应时间为2 h;当R=1.02时,ATPE的拉伸强度最大,约为4 MPa;硬段含量为40%的ATPE的拉伸强度最大,为3.54 MPa;当硬段含量超过40%以后,硬段溶入软段的百分数小于10%,ATPE体现出良好的微相分离。     

Statistical study of interplanetary condition effect on geomagnetic storms: 2. Variations of parameters

We investigate the behavior of mean values of the solar wind’s and interplanetary magnetic field’s (IMF) parameters and their absolute and relative variations during the magnetic storms generated by various types of the solar wind. In this paper, which is a continuation of paper [1], we, on the basis of the OMNI data archive for the period of 1976–2000, have analyzed 798 geomagnetic storms with D _st ≤ −50 nT and their interplanetary sources: corotating interaction regions CIR, compression regions Sheath before the interplanetary CMEs; magnetic clouds MC; “Pistons” Ejecta, and an uncertain type of a source. For the analysis the double superposed epoch analysis method was used, in which the instants of the magnetic storm onset and the minimum of the D _st index were taken as reference times. It is shown that the set of interplanetary sources of magnetic storms can be sub-divided into two basic groups according to their slowly and fast varying characteristics: (1) ICME (MC and Ejecta) and (2) CIR and Sheath. The mean values, the absolute and relative variations in MC and Ejecta for all parameters appeared to be either mean or lower than the mean value (the mean values of the electric field E _y and of the B _z component of IMF are higher in absolute value), while in CIR and Sheath they are higher than the mean value. High values of the relative density variation sN/〈N〉 are observed in MC. At the same time, the high values for relative variations of the velocity, B _z component, and IMF magnitude are observed in Sheath and CIR. No noticeable distinctions in the relationships between considered parameters for moderate and strong magnetic storms were observed.     

Detonation engine fed by acetylene–oxygen mixture

The advantages of a constant volume combustion cycle as compared to constant pressure combustion in terms of thermodynamic efficiency has focused the search for advanced propulsion on detonation engines. Detonation of acetylene mixed with oxygen in various proportions is studied using mathematical modeling. Simplified kinetics of acetylene burning includes 11 reactions with 9 components. Deflagration to detonation transition (DDT) is obtained in a cylindrical tube with a section of obstacles modeling a Shchelkin spiral; the DDT takes place in this section for a wide range of initial mixture compositions. A modified ka-omega turbulence model is used to simulate flame acceleration in the Shchelkin spiral section of the system. The results of numerical simulations were compared with experiments, which had been performed in the same size detonation chamber and turbulent spiral ring section, and with theoretical data on the Chapman–Jouguet detonation parameters.     

Thermodynamic properties of mixed fuel combustion products

In this paper, the results of calculating the processes of two fuel mixture combustion in different proportions are presented. The values of temperature, thermal capacity, specific gas constant and isentropic expansion ratio of combustion products are given. Also shown is the distinction of thermodynamic properties from the additivity law.