基于多孔介质模型的指尖密封泄漏流动分析

将指尖密封处理为多孔介质,把压力梯度作为多孔介质动量方程中的源项,根据试验结果确定了源项中的系数,结合指尖密封的结构参数提出了用于指尖密封泄漏的多孔介质模型,利用该模型计算结果与试验结果吻合较好,证明利用该模型模拟指尖密封泄漏是可行的.流场计算结果表明:指尖密封与转子接触部分的孔隙率对泄漏影响比较大,指尖密封的承压部分主要为后挡板内径以下区域.      

涡扇发动机极值限制保护闭环控制设计

现代高性能涡扇发动机采用分段组合多变量控制计划,以发挥发动机工作在整个飞行包线范围内的气动热力设计潜力。为保证发动机在过渡态工作的安全性,控制系统中必须考虑极值限制保护控制的设计问题。为避免直接限制保护控制引发的不同控制通道切换带来的系统震荡问题,提出1种高回路稳态增益的滞后-超前频域校正间接极值限制保护控制器设计方法,在保证限制回路足够的稳态精度和抗噪声能力的同时,又避免了引入积分环节导致相角裕度损失过大的缺点。通过发动机线性模型和非线性模型的控制系统仿真,验证了所述方法设计限制控制器的有效性。     

数字通信系统中新型自动增益控制方法设计

设计了一个新型的自动增益控制(Automatic Gain Control,AGC)方法.针对某数字通信系统的需求,所设计的AGC可以充分利用ADC量化位数,并能够处理LTE多种传输模式(TM2和TM3)信号.仿真结果表明,本AGC能够同时适用于TM2和TM3信号,能够在充分利用ADC量化位数的同时避免过饱和现象,能够准确判断输入信号功率变化状态并迅速调整,从而对稳定功率的输入信号给出恒定的增益.     

Spatial variation of the supersonic thermal plasma flow downstream of the termination shock

In this paper we start from the most recently observed fact that the solar wind plasma after passage over the termination shock is still supersonic with a Mach number of about 2. To explain this unexpected phenomenon and to predict the evolution of properties of the downstream plasma flow we here consider a two-fluid proton plasma with pick-up protons as a separate suprathermal, second proton fluid. We then formulate a self-consistent system of hydrodynamical conservation equations coupling the two fluids by dynamical and thermodynamical coupling terms and taking into account the effects of newly incorporated protons due to charge exchange with the H-atoms in the heliosheath. This then allows us to predict that in the most probable case the solar wind protons will become subsonic over a distance of about 30 AU downstream of the shock. As we can also show, it may, however, happen that the plasma mixture later again reconverts to a supersonic signature and has to undergo a second shock before meeting the heliopause.     

某小型无人机中长波辐射特性测量及辐射强度反演

随着“自杀式”无人机集群的饱和式攻击在战场上发挥巨大威力,如何有效拦截是各国近年来研究的重要方向,而红外探测是最热门也是最高效的探测拦截手段之一。为此,开展某典型无人机目标中长波红外探测试验,获取典型某无人机目标辐射特性数据,完成中长波红外辐射强度反演。同时,考虑环境变化对红外探测的影响,为使用红外探测手段完成无人机目标拦截提供实测效果演示。本文研究结果可作为论证中长波对无人机目标探测差异的依据,以支撑探测体制的选择。     

多孔介质微燃烧器内的火焰驻定机理研究

为解释毫米尺度多孔介质燃烧器中火焰可在一个当量比范围内驻定的物理现象,搭建了二维非稳态数学物理模型,利用数值计算方法定性研究了氢气/空气预混气在部分填充不锈钢网的微通道内的火焰传播特性。通过分析浸没火焰及表面火焰的温度分布特点并量化燃烧室内的预热和散热发现：火焰驻定在多孔介质内的不同位置时对应的传热特性存在差异,是控制火焰传播速度在一定当量比范围内保持恒定的关键因素,而预热及散热的相对大小可作为衡量传热对火焰宏观影响的重要参数。对火焰的的总预热与总散热之比R越临近多孔介质入口边界变化越剧烈,导致浸没火焰易驻定在多孔介质的中上游区域;多孔介质对火焰的预热虽在多孔介质出口边界外减小,但与多孔介质散热之比Rp呈上升趋势,使得低流速工况下易形成表面火焰。同时,R随当量比的变化规律导致多孔介质下游火焰的稳定性相对较弱。     

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.     

导体与非导体介质翼型的缩比模型RCS数值计算分析

应用二维电磁散射有限元算法理论考虑了几组导体和非导体介质翼型的缩比计算模型,计算出缩比模型的RCS并与1:1模型进行对比.结果显示,导体翼型的缩比模型RCS计算结果与推及的二维导体外形缩比模型测量定律完全符合;非导体翼型的缩比模型在等效阻抗增大时,按缩比测量定律计算的RCS与1:1模型间的相对误差越来越大,但在等效阻抗小于0.5时缩比定律是有效的.     

CO2脉冲激光与气体相互作用实验

实验研究采用波长为10.6μm的CO2脉冲激光器,N2,He,CO2等三种纯净气体及上述气体的相互混合气作为推进工质时,通过实验舱内的冲击摆装置对抛物形光船获得的冲量耦合系数Cm进行了测量。实验发现气体工质的获得的冲量耦合系数Cm随气压增高而增大,通常气体工质的分子量越大,冲量耦合系数Cm越大;在低气压条件下,分子量较大的气体所占的比例越高,混合气获得的冲量耦合系数Cm越高;在高气压条件下,混合气体工质获得的冲量耦合系数与混合气体的种类及比例密切相关。     

扩展分支分析方法在飞行动力学中的应用

将分支分析和突变理论方法扩展后,应用于飞机全包线范围内平衡特性的连续计算和稳定性分析,提出了以扩展分支分析方法为基础的反馈参数连续调参的控制律设计方法。研究结果表明,扩展分支分析方法不仅能获得飞行性能指标,而且可确定非线性飞行动力学系统的稳定特性,是综合进行性能计算、品质分析及控制律设计的一种有效方法。