“蚌式”进气道附面层扫除特性风洞试验

以某低、高速风洞为平台,设计搭建了“蚌式”进气道附面层扫除特性测量试验系统,进行了不同流量系数和来流马赫数下进气道鼓包表面附面层扫除特性的风洞试验,通过对试验数据的整理、计算和对比分析同型号的飞行试验结果,研究了“蚌式”进气道鼓包表面附面层扫除特性。研究结果表明:在相同的来流马赫数下,随着流量系数的增大,鼓包表面附面层的扫除能力逐渐减弱;在亚声速工况的绝大多数流量范围内,鼓包表面压力系数沿鼓包中心线对称分布、压力梯度变化明显,且在不同截面沿主流方向具有增大的特征,鼓包构型对附面层扫除效果较强;超声速工况下具有明显附面层扫除能力的流量范围明显小于亚声速工况,进气道唇口形成的弓形激波是影响鼓包表面不同位置压力梯度变化的主要因素,进而决定着附面层扫除特性。在接近来流马赫数18及以上飞行工况下,附面层的扫除能力减弱,附面层分离加强,进而会造成较大的进气压力损失和畸变。     

微型燃气轮机燃烧室燃烧特性实验

针对燃气轮机低污染排放要求,在为使用气体燃料设计的低排放微型燃气轮机燃烧室单头部实验件上进行了燃烧特性实验,对比分析了燃料喷口位置、数量,值班级与主燃级燃料分配比例和不同空气流量分配方式时的燃烧效率和污染物排放特性。结果表明:改变燃料喷口的位置、数量可以改变燃料与空气的混合特性,对燃烧特性产生较大的影响;值班级与主燃级燃料流量分配比例的变化,会导致各燃烧区当量比的变化,主燃级燃烧区当量比降低至08以下有利于降低污染物排放;通过改变燃烧室空气流量分配方式,可以降低主燃级燃烧区的当量比,使NOx排放降低至272 mg/m3,燃烧效率达到986%。但用于掺混的空气流量的降低会使出口温度分布系数由021升高至024。     

高长径比银纳米线的制备及其透明导电薄膜性能

为改善产品长径比,本文在经典多元醇法的基础上,经过常压滴注路线和密闭溶剂热路线分别制备银纳米线。详细讨论了反应时间、反应气氛及反应物投料比等相关参数对银纳米线的产率和长径比的影响。发现密闭溶剂热法在缓解环境污染的同时降低了生长过程中的扰动,所得银纳米线平均直径约55 nm,长度约65μm,长径比接近1 200。以之制备的透明导电薄膜的方阻仅6Ω,波长550 nm下透光度为78. 6%,品质因数(FOM)高达246,优于常压滴注路线。     

预燃式等离子体射流点火器工作特性实验研究

为解决发动机点火包线小于飞行包线的实际问题,提供等离子体点火技术在航空发动机中的工程应用新思路,论文设计了一种预燃式等离子体射流点火器,实验研究了放电特性和射流特性。结果表明,预燃式等离子体射流点火器与空气等离子体射流点火器相比,在提升射流能量降低电源功率方面有着较大的优势,电流相同时通入甲烷在较大流量时可减小驱动电源功率,总流量为44L/min时,减幅可达14.99%;同时预燃式等离子体射流较空气等离子体射流稳定,且射流长度增加,扩大了点火面积,有利于点火。     

大涵道比涡扇发动机风扇/ 增压级试验件结构 设计及验证

某大涵道比风扇/增压级试验件为1级风扇加3级增压级结构,为实现风扇/增压级部件特性录取,结构设计在满足气动设计要求的基础上,重点考虑了合理性和可靠性问题,采用理论结合工程经验的方法完成了转子支撑、静子连接和轴承润滑及密封等难点设计,兼顾大涵道比风扇/增压级结构及气动特点,采用宽弦风扇叶片设计、榫头/榫槽圆弧榫连及装配式风扇转子流路板结构。顺利完成试验件研制工作,经试验验证,压比、效率等性能参数达到或超过设计指标。     

疲劳开裂结构等效分析谱构造方法

为了解决外场疲劳裂纹排故中结构疲劳载荷谱数据不全或过于复杂的问题,提出了一种适用于飞机外场疲劳开裂结构的等效分析谱构造方法。该方法以细节疲劳额定值(DFR)法和结构细节有限元分析为基础,构建地—空—地最大应力与结构疲劳寿命的变化曲线,进而通过寿命反推,获取适用的地—空—地损伤比,以此构建等效分析谱,谱型为等幅谱。通过应用实例,将该方法构造的载荷谱与实测谱进行了对比,确认了该方法的正确性和有效性。     

反推状态下大涵道比涡扇发动机气动稳定性预测与评估

为了预测与评估反推状态下,反推气流再吸入对大涵道比涡扇发动机气动稳定性的影响,采用反推气流扰流流场三维CFD数值模拟、发动机整机稳定性计算分析以及反推状态下发动机进气畸变台架试验相结合的方法,开展了反推气流对大涵道比涡扇发动机气动稳定性影响的研究。通过三维CFD数值模拟手段,捕获了反推状态下发动机进口流场的畸变程度。在此基础上,通过采用稳定性计算程序预测了发动机的气动稳定性,并进一步通过发动机台架试验,验证了预测结果。CFD计算结果表明,随着相对来流马赫数的减小,反推气流被发动机重新吸入的可能性不断增大,当相对来流马赫数减小到0.05时,外侧发动机进口的流场畸变情况变得最为严重。进气畸变情况下的整机稳定性计算分析以及发动机台架试验结果表明,在所考核的目标状态,若只存在因反推气流再吸入引起的进口流场畸变,是不会导致发动机失稳的。     

Enhancing buckling capacity of a rectangular plate under uniaxial compression by utilizing an auxetic material

Auxetic materials have previously been shown to enhance various performances due to its unusual property of becoming fatter when uniaxially stretched and thinner when uniaxially com-pressed (i.e., the materials exhibit a negative Poisson’s ratio). The current study focuses on assessing the potential of an auxetic material to enhance the buckling capacity of a rectangular plate under uniaxial compression. The in-plane translational restraint along the unloaded edges that was often neglected in open literature is taken into consideration in our buckling model proposed in this study. The closed-form expressions for the critical buckling coefficient of the rectangle are provided and the predicted results agree well with those determined by the finite element method. Further-more, the results indicate that the buckling performance of a rectangular plate under uniaxial com-pression can be significantly improved by replacing the traditional material that has a positive Poisson’s ratio with an auxetic material when there is in-plane translation restraint along the unloaded edges.     

航空后续备件周转比例计算

首先根据航空后续备件消耗的特点,将后续备件分为四类:有寿件、可修件、消耗件和低耗件;对于前三类分别建立了计算模型,对于低耗件,提出了专家估算方法。经实际验证,本文提供的方法可以达到满意的结果。     

Indicators of black-hole mass and Eddington accretion ratio from QSO X-ray and UV spectra

The evolution of luminous QSOs is linked to the evolution of massive galaxies. We know this because the relic black-holes found locally have masses dependent on the properties of the host galaxy’s bulge. An important way to explore this evolution would be to measure dependences of black-hole masses and Eddington accretion ratios over a range of redshifts, i.e., with cosmological age. For low redshift QSOs (and their lower luminosity Seyfert galaxy counterparts) it has been possible to infer black-hole masses from the luminosities and velocity dispersions of their host-galaxy bulges. These masses agree with those virial black-hole masses calculated from the Doppler widths of the broad Hβ emission lines. The latter method can then be extended to more distant and luminous QSOs, up to redshifts of 0.6 with ground-based optical observations. We discuss ways to extend these explorations to higher redshifts – up to 3 using the widths of QSOs’ broad UV emission lines, and in principle, and to redshifts near 4 from ground-based infrared observations of rest-frame Hβ at 2.5 μm. We discuss the possibility of investigating the accretion history of the higher redshift QSOs using measures of Eddington accretion ratio – the soft X-ray spectral index and the eigenvectors of Principal Components Analyses of QSOs’ UV emission-line spectra.