下颔式进气道实验研究

为了验证下颔式进气道 /前机身一体化设计方案的合理性及其进气道性能 ,对下颔式进气道 /前机身一体化设计方案进行了实验研究。测出了进气道总压恢复系数、畸变指数随流量系数、攻角、侧滑角的变化规律。结果表明 ,进气道性能较好 ,进气道 /发动机匹配良好。最后提出了下颔式进气道的进一步改进措施     

GE90-70双机热备冗余控制系统在进排气调压系统中的应用

本文介绍了进排气调压系统测控改造的总体结构、通信网络、软件设计和系统功能。该系统以GE90—70的可编程控制器（PLC）为基础,将Ethernet和现场总线Genius相结合进行数据通信,采用下位机编程软件Cimplieity Machine Edition、上位机组态软件Cimplicity HMI编制设计软件系统,使整个系统具有较好的可靠性和可扩展性。能实现进排气压力调节的工况显示和过程控制。实际运行表明,该系统结构先进,控制可靠,配置灵活,可进一步提高高空台试验效率,降低试验风险。     

NiCoP合金包覆空心微珠粉体的制备

采用粉体化学镀技术，以AgNO3取代常见的贵金属盐PdCl2作为活化剂，H2PO2^-取代Sn^2 作为还原剂，在空心微珠表面包覆NiCoP合金。利用扫描电镜、能谱分析仪分析包覆层的形貌和成分。结果表明NiCoP合金均匀包覆在空心微珠表面。并提出了这种改进工艺的一种可能的机理。     

飞机机身腹部与两侧进气道性能比较试验研究

通过高低速风洞试验,对比迎角和侧滑角对机身腹部和机身两侧进气的进气道气动性能的影响。试验结果表明:在超音速来流状态下,当迎角增加到5°时,腹部进气道的气动性能改善,而两侧进气道的气动性能几乎不变;在亚音速来流状态下,当迎角从6°逐渐增加到所试验的值(高亚音速为12°,低速为30°),两侧进气道的气动性能逐渐明显变差,而腹部进气道的气动性能对迎角并不敏感,基本能保持无迎角时的性能;在高低速来流状态下,两种型式进气道的气动性能对所试验的侧滑角β(小于6°或9°)均不敏感。      

气固紊流剪切流中颗粒弥散的拉格朗日模拟

本文提出了一种对于气固两相紊流剪切流中圆形固体颗粒弥散的拉格朗日拟计算方法，其中考虑了颗粒间的磁撞对流体相和颗料相的影响，应用该方法对一气固紊流剪切流场进行了模拟计算，并对有、无颗粒间磁撞情况下的模拟计算结果与Lavieville用大涡模拟方法的研究结果进行了比较，并进行了讨论。     

腹下无隔道大偏距跨声速S弯进气道气动特性的实验研究(英文)

An investigation on the ventral diverterless high offset S-shaped inlet is carried out at Mach numbers from 0.600 to 1.534, angles of attack from -4° to 9.4°, and yaw angles from 0° to 8°. Results indicate： （1） a large region of low total pressure exists at the lower part of the inlet exit caused by the counter-rotating vortices in the S-shaped duct; （2） the performances of the inlet at Mach number 1.000 reach almost the highest, so the propulsion system could work efficiently in terms of aerodynamics; （3） the total pressure recovery increases slowly at first and then remains unvaried as the Mach number rises from 0.6 to 1.0, however, it does in an opposite manner in the conventional diverter-equipped S-shaped inlet; （4） the performances of the inlet are generally insensitive to angles of attack from -4° to 9.4° and yaw angles from 0° to 8° at Mach number 0.850, and angles of attack from -2° to 6° and yaw angles from 0° to 5° at Mach number 1.534.     

基于混合多目标粒子群算法的飞行器气动布局设计

 为了提高多目标优化算法求解非劣解集的效率,在多目标粒子群算法的基本框架中引入了Pareto过滤算子、小生境技术和模拟退火算法,建立了全新的混合多目标粒子群算法。该算法具有运算收敛快,所得非劣解集分布均匀、广泛的特点。将其应用于求解以升阻比和效用体积最大化为目标的再入式高超声速飞行器气动布局多目标优化设计模型,将计算结果与原始多目标粒子群算法的计算结果进行对比,体现出本文提出的混合多目标粒子群算法能够更加有效地求解复杂多目标优化设计问题的非劣解集,从而为多目标决策提供有力的支持。     

S形进气道流动控制数值模拟研究

采用CFD技术,结合试飞数据,对某S形进气道进行了加涡流发生器的流动控制数值模拟研究.着重分析了三个不同位置加涡流发生器后,进气道内部二次流的发展;之后比较了不加涡流发生器及不同位置加涡流发生器时进气道出口总压恢复、畸变等情况.结果表明涡流发生器明显地影响着进气道内部二次流的发展变化,涡流发生器对进气道出口周向稳态总压畸变有较大程度改善,但是对于提高总压恢复效果不明显.     

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.     

隐身外形飞行器用埋入式进气道的设计与风洞实验研究

本文为隐身外形飞行器用埋入式进气道发展了一套设计方法。该方法的理论基础是埋入式进气道进气机理和气动S弯概念,其关键技术包含通道中心线设计、横截面面积变化规律设计以及横截面形状设计等,各技术可以方便地用数学方法加以描述,整个方法易于编程实现。并结合一种隐身外形无人机提出了埋入式进气道方案,通过实验得到了此类隐身外形飞行器用埋入式进气道的气动特性。结果表明,所提出的埋入式进气道方案可行,所设计的模型进气道性能良好,所发展的设计方法合理。同时验证了埋入式进气道进气机理的正确性,也表明隐身外形飞行器与埋入式进气道的组合方案具有十分光明的应用前景。