推桨式察打无人机起落架总体布置参数设计研究

现有飞机起落架总体布置参数设计的规范和要求主要适用于传统战斗机,如果按此规范和要求设计推桨式察打一体无人机起落架将带来诸多问题。从推桨式察打一体无人机的布局和飞行特点入手,通过对起落架总体布置参数的定义和内涵进行分析,提出一种适合推桨式察打无人机起落架总体参数和总体布置的设计方案,对察打一体无人机起降特点进行分析;对比“捕食者B”无人机起落架总体布置参数,验证本文设计方案的有效性。结果表明：擦地角可减小,建议不小于6°（静态,含间隙）;防倒立角可减小,建议11°～12°（静态）;停机角范围可适当减小,建议-2°～-1°;起落架总体布置方案可选择机身式、较长的外八字形起落架布置型式。     

Numerical investigation of unsteady vortex breakdown past 80°/65° double-delta wing

An improved delayed detached eddy simulation （IDDES） method based on the k-x-SST （shear stress transport） turbulence model was applied to predict the unsteady vortex breakdown past an 80o/65o double-delta wing （DDW）, where the angles of attack （AOAs） range from 30° to 40°. Firstly, the IDDES model and the relative numerical methods were validated by simulating the massively separated flow around an NACA0021 straight wing at the AOA of 60°. The fluctuation properties of the lift and pressure coefficients were analyzed and compared with the available measurements. For the DDW case, the computations were compared with such mea-surements as the mean lift, drag, pitching moment, pressure coefficients and breakdown locations. Furthermore, the unsteady properties were investigated in detail, such as the frequencies of force and moments, pressure fluctuation on the upper surface, typical vortex breakdown patterns at three moments, and the distributions of kinetic turbulence energy at a stream wise section. Two dominated modes are observed, in which their Strouhal numbers are 1.0 at the AOAs of 30°, 32° and 34° and 0.7 at the AOAs of 36o, 38° and 40°. The breakdown vortex always moves upstream and downstream and its types change alternatively. Furthermore, the vortex can be identified as breakdown or not through the mean pressure, root mean square of pressure, or even through correlation analysis.     

民用运输飞机适坠性要求浅析

全面解读了民用运输飞机适坠性要求,并对CCAR/FAR25与CS25之间差异进行剖析,总结国内外相关经验,提出适坠性后续工作方向。     

超宽带螺旋天线的小型化设计

介绍一种新型的螺旋结构天线,将平面等角螺旋天线与锥面螺旋天线结合起来,采用渐变式的巴伦平衡馈电。相比传统的平面螺旋天线,针对同样频带宽度的天线设计,这种混合型螺旋天线体积更小。利用Ansoft HFSS电磁场仿真软件对天线进行建模和仿真计算,并结合仿真结果实际制作了该螺旋天线,给出了实测结果,表明天线可以在工程实际中应用。     

The variability of the proton cosmic ray flux on the Sun’s way around the galactic center

The discovery of direct evidences for the acceleration of high energetic particles at the shell supernova remnant RXJ1713.7-3946 underlined the need to calculate the cosmic ray (CR) distribution in the Galaxy on a spatial grid fine enough to resolve the changes in the CR density due to these kind of objects. It was shown before by Büsching et al. [Büsching, I., Kopp, A., Pohl, M., Schlickeiser, R., Perrot, C., Grenier, I. Cosmic-ray propagation properties for an origin in supernova remnants. ApJ 619, 314–326, 2005] that the discrete nature (both in space and time) of super novae (SN) as sources of Galactic CR leads to CR spectra changing in space and time, resulting in a range of possible CR spectra at a given location in the Galaxy. As the most frequent SN types Ib and II are found within spiral arms, one can expect a significant difference of the range of possible spectra in and outside spiral arms. We investigate the variability of the local interstellar CR proton spectrum during the motion of the Sun in and out of spiral arms in its journey around the Galactic center. Using the code described by Büsching et al. [Büsching, I., Kopp, A., Pohl, M., Schlickeiser, R., Perrot, C., Grenier, I. Cosmic-ray propagation properties for an origin in supernova remnants. ApJ 619, 314–326, 2005], the proton CR density in the Galaxy is calculated with high spatial and temporal resolution (75 pc in galactocentric radius r and azimuth φ at the position of the Sun and 20 pc in z (perpendicular to the galactic plane), with a time step of 1 kyr), assuming stochastically distributed point sources with a probability distribution that resembles the spiral structure of our Galaxy. We find the averaged CR flux outside the spiral arm to be about 50% of that inside a spiral arm. We further find spatial and temporal variations of the CR flux inside spiral arms.     

非对称式带状线模式馈电网络

本文概要的介绍了一种新型器件——非对称式带状线模式馈电网络的基本原理,主要技术指标及其相位关系等。该器件体积小、重量轻、结构紧凑、性能稳定、用于按模式馈电的场合既方便又可靠。     

一维喷管化学反应流的吉尔方法研究

建立了一维喷管化学反应流计算模型,并进行了数值求解,给出了喷管内一维化学反应流计算结果。采用吉尔方法解决控制方程组的刚性问题获得满意效果。计算中解决了化学反应流计算中初值难于给定和喉部条件难于确定等问题。并通过对氢氧发动机喷管的分析计算,证明了这种方法的正确性。     

具有SFD及锥齿轮啮合的多转子系统稳态不平衡响应研究

研究具有锥齿轮啮合条件下,多转子-支承系统的动力响应;研究挤压油膜阻尼器对锥齿轮传动系统减振的有效性;导出计及锥齿轮啮合力的弯扭耦合传递矩阵,建立了计算包括主动轮、从动轮并带有畸形结构的多转子轴系不平衡响应的通用程序。      

2219合金TIG补焊接头亮线影像成因及其力学性能

针对2219合金TIG补焊接头X射线底片亮线影像,开展2219合金不同坡口面角TIG补焊接头组织及性能研究。通过X射线、扫描电镜及能谱仪分析接头底片亮线影像位置对应的微观形貌及成分,并通过拉伸试验评价补焊接头力学性能。结果显示:在0～20°随坡口面角α值的增大,X射线底片上亮线影像的黑度逐渐降低;Cu含量较高的α(Al)+θ非平衡共晶组织对X射线的散射与吸收作用较强,是X射线底片亮线影像的成因;坡口面角α角侧受电磁搅拌作用弱于β角侧,其固-液界面前沿的边界层宽度大于β角侧,且温度梯度及边界层内的成分过冷度均大于β角侧,促进了α角侧枝晶的生长。当β角为20°时,在0°～20°随着α角度值增大,接头的抗拉强度与延伸率逐渐增大,20°时获得了优良的室温力学性能。X射线底片上存在亮线影像的补焊接头力学性能满足型号使用要求,亮线影像结构可不按焊接缺陷处理。     

一种简便的齿轮传动优化设计方法

本文通过分析齿面接触疲劳强度和齿根弯曲疲劳强度的内在联系，引进齿形复合系数和齿数算子概念，提出了一种能直接求得齿轮传动优化参数的简便方法。将该方法用于二级或多级齿轮减速器的优化设计，其优化过程更为直观、清晰，编程更为简单、快捷。