超大口径环形天线包带展开过程动力学仿真

中间柔性包带是环形可展开天线的重要组成部分。中间包带拔销器解锁后，复材包带与环形桁架同步展开。因复材包带柔性较强，它会绕根部固定端进行回弹，因此展开过程存在金属接头和桁架上复材薄壁管件碰撞风险。随着天线口径增大，该风险会持续增大。基于柔性多体动力学理论对超大型口径环形可展开天线包带展开过程进行动力学建模仿真，并在此基础上分析得出包带展开过程金属接头到环形桁架最小距离主要和复材包带阻尼率以及桁架预展速度相关。通过进一步研究发现：复材包带阻尼率越高，展开过程金属接头到环形桁架最小距离越大；桁架预展速度越快，展开过程金属接头到环形桁架最小距离越小。此外，对逆止回弹机构失效这一在轨极端条件下包带展开过程进行建模仿真，分析得出包带在该条件下展开过程金属接头到环形桁架最小距离变化规律。该研究可为超大口径环形天线结构优化设计及包带在轨展开预示提供依据。     

内孔结构对旋转空化发生器水力特性的影响

空化普遍存在于工业生产、舰船推进、航空航天等领域.使用高速相机对闭式循环试验台的旋转空化发生器内部流动进行试验观测，然后基于RNG k ε湍流模型和Zwart Gerber Belamri空化模型开展了旋转空化发生器流场的数值模拟.结果表明数值模拟结果与试验观测数据吻合较好，验证了本文数值模拟方法的准确性和可靠性.受离心力作用，转子孔内的压力从内径到外径逐渐增大.内孔底部由于轴向旋涡的作用，产生较大旋涡并耗散能量.内孔顶部流体与腔体区主流相互作用，在内孔顶侧产生碰撞并形成较小漩涡.不同内孔结构对旋转空化发生器的空化效果具有重要影响，在相同工况下椭圆形内孔的空化率小于圆锥形和圆柱形，说明型线光滑的内孔结构局部损失小，产生的空化较弱.不同内孔结构下，旋转空化发生器内部压力脉动的主频为转频fi或24fi(对应圆周方向开孔排数)，压力脉动最大幅值出现在进口管侧和出口管侧，主要原因是受动静干涉作用影响.     

碳纳米管阵列推力器放电特性的数值模拟研究

基于直接蒙特卡洛(DSMC)算法、浸入式有限元算法(IFE)、粒子云及蒙特卡洛碰撞(PIC-MCC)算法以及Ammosov-Delone-Krainov(ADK)隧穿电离模型建立了碳纳米管阵列推力器工质气体和CNT场电离过程的三维仿真模型。利用文献中的实验数据对本文仿真模型的有效性进行了验证,结果表明本文仿真模型与实验结果基本一致。针对碳纳米管阵列推力器的放电特性进行了研究,并重点分析了离子与原子碰撞过程对碳纳米管阵列推力器放电特性的影响。结果表明CNT可以极大地增强局部电场,稳态时场增强因子约为1308;与原子的碰撞使得离子在CNT附近更加集中,降低了局部电场,进而降低了其场增强能力。     

The Kumtag meteorite strewn field

The Kumtag meteorite strewn field was found in the Kumtag desert, 132 km south of Hami city in the Xinjiang province, China. It is an ellipse of 2.5 × 7.9 km, with a long axis extending along the northeast-southwest direction. The largest individual meteorite of the strewn field weighs about 10 kg; the smallest individual has a mass of only 27 g. In total, more than 100 individuals with a total mass of more than 180 kg were collected. The location and the distribution of the fragments suggest that the Kumtag meteoroid entered the atmosphere in the direction Northeast-Southwest. All meteorites collected in this strewn field are samples from the same unique meteorite shower. The Kumtag meteorite is an H5 ordinary chondrite with a shock stage S2, and a weathering grade W2. The cosmic ray exposure age of Kumtag is 6.7 ± 0.8 Ma, which is rather typical for H chondrites and which indicates that Kumtag was derived from the massive impact event on its parent body ~7 Ma ago. A significant amount of He has been lost during certain unknown processe(s) before the Kumtag meteorite was ejected from its parent body.     

Stability of relative equilibria of the full spacecraft dynamics around an asteroid with orbit–attitude coupling

The full dynamics of spacecraft around an asteroid, in which the spacecraft is considered as a rigid body and the gravitational orbit–attitude coupling is taken into account, is of great value and interest in the precise theories of the motion. The spectral stability of the classical relative equilibria of the full spacecraft dynamics around an asteroid is studied with the method of geometric mechanics. The stability conditions are given explicitly based on the characteristic equation of the linear system matrix. It is found that the linearized system decouples into two entirely independent subsystems, which correspond to the motions within and outside the equatorial plane of the asteroid respectively. The system parameters are divided into three groups that describe the traditional stationary orbit stability, the significance of the orbit–attitude coupling and the mass distribution of the spacecraft respectively. The spectral stability of the relative equilibria is investigated numerically with respect to the three groups of system parameters. The relations between the full spacecraft dynamics and the traditional spacecraft dynamics, as well as the effect of the orbit–attitude coupling, are assessed. We find that when the orbit–attitude coupling is strong, the mass distribution of the spacecraft dominates the stability of the relative equilibria; whereas when the orbit–attitude coupling is weak, both the mass distribution and the traditional stationary orbit stability have significant effects on the stability. We also give a criterion to determine whether the orbit–attitude coupling needs to be considered.     

Д-30发动机ЭИ868合金扇形块的钎焊修复

针对某Д-30发动机大修对ЭИ868合金(对应于我国的牌号GH3044)扇形块的修复要求,采用真空钎焊的方法对扇形块进行了钎焊补焊。对钎焊补焊的扇形块进行超声波探伤。结果表明,钎缝内部质量满足HB7575-97一级钎焊接头的要求,表明所确定的修复工艺可实现ЭИ868合金扇形块的可靠修复。     

Spectroscopy peculiarities of thermal plasma of electric arc discharge between electrodes with Zn admixtures

Plasma of the free burning electric arc between Ag–SnO₂–ZnO composite electrodes as well as brass electrodes were investigated. The plasma temperature distributions were obtained by Boltzmann plot method involving Cu I, Ag I or Zn I spectral line emissions. The electron density distributions were obtained from the width and from absolute intensity of spectral lines. The laser absorption spectroscopy was used for measurement of copper atom concentration in plasma. Plasma equilibrium composition was calculated using two independent groups of experimental values (temperature and copper atom concentration, temperature and electron density). It was found that plasma of the free burning electric arc between brass electrodes is in local thermodynamical equilibrium. The experimental verification of the spectroscopic data of Zn I spectral lines was carried out.     

三维自适应终端滑模协同制导律

针对多枚导弹协同作战的问题,且多枚导弹之间保持有向拓扑通信的条件下,基于终端滑模法设计了视线方向及视线法向的双层协同制导律。其中,视线方向的制导指令能够保证导弹同时完成拦截任务;视线法向上的三维制导律能够保证每枚导弹以期望的视线角攻击目标,从而发挥各枚导弹的最大杀伤力,并且视线角的约束相当于规划了末制导段导弹的弹道问题,在一定程度上避免攻击目标前导弹间发生碰撞。同时,针对所设计的滑模制导律设计了新的自适应律,从而加快了滑模面的收敛速度并且削弱了由符号函数引起的系统抖振现象。基于李雅普诺夫稳定性理论,证明了所设计制导律的正确性,并在最后给出了数学仿真实验,验证了所设计制导律的有效性及优越性。     

超声速膨胀角入射激波/湍流边界层干扰直接数值模拟

为了揭示膨胀效应对激波/湍流边界层干扰区内复杂流动现象的影响规律,采用直接数值模拟方法对来流马赫数2.9、30°激波角的入射激波与10°膨胀角湍流边界层相互作用问题进行了数值研究。系统地探讨了激波入射点分别位于膨胀角上游、膨胀角角点和膨胀角下游3种工况下膨胀角干扰区内若干基本流动现象,如分离泡、物面压力脉动及激波非定常运动、湍流边界层统计特性和相干结构动力学过程等。结果表明,激波入射点流向位置改变对分离区流向和法向尺度的影响显著,尤其是当激波入射点位于角点及其下游区域。研究发现,膨胀角干扰区内物面压力脉动强度急剧减小,分离区内压力波向下游传播速度将降低而在膨胀区内将升高,膨胀效应极大地抑制了分离激波的低频振荡运动。相较于入射激波与平板湍流边界层干扰,入射激波流向位置改变对膨胀角再附区速度剖面对数区及尾迹区影响显著,将导致其内层结构参数升高而外层降低,近壁区内将呈现远离一组元湍流状态的趋势。此外,流向速度脉动场本征正交分解分析指出,主模态空间结构集中在分离激波及剪切层根部附近而高阶模态以边界层内小尺度正负交替脉动结构为主。低阶重构流场结果表明,前者对应为分离泡低频膨胀/收缩过程而后者表征为分离泡高频脉动。     

变循环发动机过渡态性能直接模拟方法

为了实现多变量可调的变循环发动机（VCE）过渡态性能模拟和控制规律设计,在稳态逆算法和过渡态性能隐式格式计算方法的基础上开发了变循环发动机过渡态直接模拟方法。在稳态逆算法模型中加入容积效应和转子动力学方程,实现了同时给定加速率、涡轮前温度和压缩部件工作点的条件下直接模拟计算过渡态过程中变几何参数和燃油流量的调节规律,验证了方法的精度和可行性,并将该方法用于变循环发动机转模态性能模拟和控制规律设计。计算结果表明,过渡态直接模拟方法的误差在0.58%以内,超声速巡航状态下由单外涵模态转换到双外涵模态的时间约为1 s,海平面静止状态下双外涵转单外涵的时间约为3 s,且推力、转速、涡轮前温度、喘振裕度等参数过渡平稳。该方法可简化转模态控制规律设计流程,并提高设计精度。