高速圆柱滚子轴承保持架动力学特性分析

建立了高速圆柱滚子轴承动力学微分方程,采用精细积分法和预估-校正Adams-Bashforth-Moulton多步法相结合的算法,对高速圆柱滚子轴承动力学微分方程进行求解,并对保持架的动力学特性进行了理论分析.结果表明:过大的保持架间隙比不利于保持架稳定运转;在一个套圈固定、另一个套圈工作状态下,保持架引导方式采用旋转套圈引导时,保持架打滑率较低;保持架采用外引导方式时保持架质心运动较为稳定;在内外圈同向旋转且外圈转速高于内圈转速条件下,保持架采用外引导方式时,保持架打滑率较低;在内外圈反向旋转且外圈转速高于内圈转速条件下,保持架质心轨迹变得不规则;保持架采用外引导方式时,保持架打滑率为负值.      

高负荷吸附式压气机叶栅数值与实验研究

针对无通道激波单纯由强逆压梯度诱导的附面层分离进行了吸附式数值与实验研究.研究对象为某大转折角高负荷吸附式压气机叶栅,利用准三维叶栅通道计算程序（MISES）进行抽吸流场数值模拟,在确定抽吸位置后进行了风洞实验验证.结果表明:抽吸后总压损失系数大幅度降低,对于单纯由强逆压梯度诱导的附面层分离,最佳抽吸位置应该位于附面层分离之后尚未充分发展之处;在确定抽吸位置时可以根据设计状态的分离状况进行;实际中需要的抽吸流量小于计算值;在数值计算中,具体的抽吸模型还有待进一步改进和修正,以使数值模拟更加准确.      

某型航空活塞发动机进排气系统优化分析

针对高空小型飞机的动力要求,对某型航空活塞发动机的进排气系统均匀性进行了分析,建立了某型航空活塞发动机的仿真模型,分析了进排气管路结构参数对发动机性能的影响.以进气质量流量不均匀度和进气压力波动效应为评价指标,对发动机的进排气系统结构参数进行了优化.通过改变进排气歧管和总管的长度,把不均匀度降低到5%以内,最大降幅为38%,并且提高了发动机的扭矩和功率,最大提高幅度为5%.      

一种直升机自旋训练过程涡轴发动机控制规律设计与仿真

针对直升机自旋训练过程中涡轴发动机快速响应要求,提出了一种以燃油流量和导叶角为控制量的鲁棒控制规律抑制自由涡轮转速瞬态下垂.首先,通过改进UH-60直升机/T700发动机综合模型,使之能够模拟自旋进入及自旋恢复过程动态变化.其次,提出并设计一种基于燃油流量和导叶调节的涡轴发动机鲁棒控制规律,并通过典型的自旋训练过程仿真,验证了该控制规律相比仅以燃油流量为变量的控制规律,自由涡轮转速瞬态下垂量降低至3%以下,且燃油流量变化更加平缓,改善了执行机构的工作条件.     

固液火箭发动机试验燃速的计算

基于固液火箭发动机固体药柱燃速与药柱通道氧化剂质量流率的关系,推导分析得出:在2s短工作时间内或者药柱通道直径增大10%的情况下,燃烧室压力与其氧化剂质量流量成正比.因此通过试验测量的燃烧室压力可计算得到发动机转级或者关机拖尾段中的氧化剂质量流量.据此,计算发动机拖尾段消耗的燃料质量,消除发动机拖尾段燃料消耗对平均燃速的影响,可以修正常用的计算试验燃速的起止点平均法.利用此方法对两种试验推进剂组合的燃速进行了计算,原偏高的燃速值降低约20%,不同尺寸发动机的燃速符合尺寸规律,偏差在5%以内,使小尺寸发动机测得的燃速可应用到大尺寸发动机的设计中.      

Type II Solar Radio Bursts: Theory and Space Weather Implications

Recent data and theory for type II solar radio bursts are reviewed, focusing on a recent analytic quantitative theory for interplanetary type II bursts. The theory addresses electron reflection and acceleration at the type II shock, formation of electron beams in the foreshock, and generation of Langmuir waves and the type II radiation there. The theory's predictions as functions of the shock and plasma parameters are summarized and discussed in terms of space weather events. The theory is consistent with available data, has explanations for radio-loud/quiet coronal mass ejections (CMEs) and why type IIs are bursty, and can account for empirical correlations between type IIs, CMEs, and interplanetary disturbances. This revised version was published online in August 2006 with corrections to the Cover Date.     

SAE线性令牌传输总线与光纤型分布式数据接口规约的比较

SAE LTPB与ANSI FDDI两种光纤高速总线规约很适合在分布式航空电子综合系统中使用,以满足下一代高性能军用飞机系统区域内、外数据的高传递速率的需要。本文从几个方面对其作了比较,旨在为设计者选择使用提供参考。     

液体火箭发动机喷管发汗冷却研究

采用SSTk-ω湍流模型对液体火箭发动机喷管发汗冷却进行了全场耦合计算,考虑了不同孔隙率、变物性、可压缩性、多孔介质热弥散效应、微尺度流动以及传质等因素的影响,比对再生冷却分析了不同注入率对壁面温度、冷却效率以及边界层厚度的影响;结果表明平均注入率的增大使平均壁温以更大的比例降低,采用发汗冷却的喷管喉部不再是最高温的部位.将CFD计算结果分别与实验以及一维气动公式计算结果进行了比较,证实计算结果可靠.      

Solar Sources of Heliospheric Energetic Electron Events—Shocks or Flares?

Electrons with near-relativistic (E≳30 keV, NrR) and relativistic (E≳0.3 MeV) energies are often observed as discrete events in the inner heliosphere following solar transient activity. Several acceleration mechanisms have been proposed for the production of those electrons. One candidate is acceleration at MHD shocks driven by coronal mass ejections (CMEs) with speeds ≳1000 km s⁻¹. Many NrR electron events are temporally associated only with flares while others are associated with flares as well as with CMEs or with radio type II shock waves. Since CME onsets and associated flares are roughly simultaneous, distinguishing the sources of electron events is a serious challenge. On a phenomenological basis two classes of solar electron events were known several decades ago, but recent observations have presented a more complex picture. We review early and recent observational results to deduce different electron event classes and their viable acceleration mechanisms, defined broadly as shocks versus flares. The NrR and relativistic electrons are treated separately. Topics covered are: solar electron injection delays from flare impulsive phases; comparisons of electron intensities and spectra with flares, CMEs and accompanying solar energetic proton (SEP) events; multiple spacecraft observations; two-phase electron events; coronal flares; shock-associated (SA) events; electron spectral invariance; and solar electron intensity size distributions. This evidence suggests that CME-driven shocks are statistically the dominant acceleration mechanism of relativistic events, but most NrR electron events result from flares. Determining the solar origin of a given NrR or relativistic electron event remains a difficult proposition, and suggestions for future work are given.     

孔隙预置技术制备多孔C/SiC复合材料及其性能表征

以玻璃纤维为成孔剂,采用孔隙预置技术制备了发汗多孔C/SiC复合材料.对孔隙结构进行了表征,并研究了材料的力学性能和渗透行为.研究结果表明,采用孔隙预置技术能够有效地实现多孔 C/SiC材料开孔率和孔隙结构控制,该材料具有良好的力学性能和渗透性能.