水下强声波脉冲引发的空化气泡运动和声辐射

通过建立由等离子体声源、PCB压力传感器和高速相机等构成的实验测量系统,研究了强声波脉冲引发的空化气泡运动和二次声辐射。通过实验,观察到了强声波脉冲特有的波形结构,空化气泡的成长、膨胀和坍缩过程以及气泡坍缩时辐射的声信号。其次,利用Gilmore方程和Bernoulli方程,从理论上对空化气泡的运动和声辐射进行了数值模拟和分析。研究结果表明：（1）在强声波脉冲正压区的作用下,空化气泡将受到压缩并围绕＂准平衡态半径＂振荡;在强声波脉冲负压区的作用下,空化气泡将出现膨胀、坍缩和回弹的物理过程。（2）空化气泡坍缩时周期性辐射的声脉冲持续时间极短,具有＂冲击波＂的特点。     

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.      

燃油射流横流穿透深度试验和数值模拟

采用激光粒子成像测速仪(PIV),试验研究了不同动量比下燃油射流在横向空气流中的穿透深度特性。同时,采用数值计算方法,对射流穿透特性进行了模拟,并将试验和计算结果,分别与已有的经验关系式,及考虑气动韦伯数影响修改后的关系式进行对比。结果表明:燃油射流上边界深度与幂指数关系式较吻合;采用VOF两相流模型能较准确地模拟出燃油射流的喷雾核心深度;修改后的关系式与不同燃油-空气动量比范围下的喷雾核心深度较吻合;燃油-空气动量比和气动韦伯数,是影响燃油射流横流穿透深度的主要参数。     

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.     

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.     

民用飞机初始库存量的预测模型及优化方法研究

以民用飞机可靠性数据为依据,对ABJ21飞机备件进行合理的分类,并建立了相应的初始库存量预测模型,对ARJ21飞机初始库存量需求进行定量的计算和优化分析,在一定条件下达到了制造商的节约成本和满足一定可用度的双重要求。