考虑配平特性的超声速客机低声爆气动布局优化研究

降低声爆水平是下一代超声速运输机研制需要解决的关键问题之一。低声爆优化通常使飞行器布局向着机翼后掠角增大、机翼沿机身方向分布范围增大的趋势发展,给飞行器的配平和低速特性带来不利影响。以某超声速客机基本构型为研究对象,建立基于类别/形状函数的翼身组合体参数化建模方法;基于超声速线化理论分析外形几何参数对声爆水平的影响。在此基础上,分别针对机身轮廓、机翼平面形状以及扭转角分布对该构型进行低声爆优化和俯仰力矩特性优化,并采用CFD 方法对优化结果进行校核。结果表明：与基准构型相比,在不显著增加俯仰力矩的基础上,优化构型的阻力降低了19 cts,近场过压显著降低,地面声爆响度降低5.1 PLdB。     

The Primordial Helium-4 Abundance from Observations of a Large Sample of Blue Compact Dwarf Galaxies

We use a sample of 45 low-metallicity H II regions in blue compact dwarf (BCD) galaxies to determine the primordial helium abundance YP with a precision better than 5%. We have carefully investigated the physical effects which may make the He I line intensities deviate from their recombination values such as collisional and fluorescent enhancements, underlying He I stellar absorption and absorption by Galactic interstellar Na I. By extrapolating the Y vs. O/H and Y vs. N/H linear regressions to O/H = N/H = 0, we obtain YP = 0.244±0.002 and 0.245±0.001, respectively, higher than previous determinations (YP = 0.230 - 0.234). Part of the difference comes from the fact that previous investigators have not taken into account underlying He I stellar absorption, especially in the NW component of the BCD I Zw 18 which, because of its extremely low metallicity plays a key role in the determination of YP. We derive a slope dY/dZ = 2.3±1.0, considerably smaller than those derived before. With this smaller slope and taking into account the errors, chemical evolution models with an outflow of well-mixed material can be built for star-forming dwarf galaxies which satisfy all the observational constraints. Our YP gives _bh ₅₀ ² = 0.058±0.007,f consistent with the lower limit set by dynamical measurements and X-ray observations of clusters of galaxies. It is also consistent, within the framework of standard big bang nucleosynthesis theory, with measurements of primordial 7Li in galactic halo stars and with the D/H abundance measured in absorption systems toward quasars by Burles and Tytler (1997).     

Experimental investigation and correlation development of jet impingement heat transfer with two rows of aligned jet holes on an internal surface of a wing leading edge

Extensive experimental studies on the heat transfer characteristics of two rows of aligned jet holes impinging on a concave surface in a wing leading edge were conducted, where50000 Rej 90000, 1.74 H/d 27.5, 66° a 90°, and 13.2 r/d 42.03. The finding was that the heat transfer performance at the jet-impingement stagnation point with two rows of aligned jet holes was the same as that with a single row of jet holes or the middle row of three-row configurations when the circumferential angle of the two jet holes was larger than 30°. The attenuation coefficient distribution of the jet impingement heat transfer in the chordwise direction was so complicated that two zones were divided for a better analysis. It indicated that: the attenuation coefficient curve in the jet impingement zone exhibited an approximate upside-down bell shape with double peaks and a single valley; the attenuation coefficient curve in the non-jet impingement zone was like a half-bell shape, which was similar to that with three rows of aligned jet holes; the factors,including Rej, H/d and r/d, affected the attenuation coefficient value at the valley significantly.When r/d was increased from 30.75 to 42.03, the attenuation rates of attenuation coefficient increased only by 1.8%. Consequently, experimental data-based correlation equations of the Nusselt number for the heat transfer at the jet-impingement stagnation point and the distributionof the attenuation coefficient in the chordwise direction were acquired, which play an important role in designing the wing leading edge anti-icing system with two rows of aligned jet holes.     

基于软件工程思想方法的CAI课件开发

介绍了软件工程思想方法，运用软件工程思想方法基于瀑布模型分析了CAI课件开发过程，实践创作开发了基于Web的多媒体《概率论与数理统计》CAI课件。     

Numerical Simulation of a Swept Wing Hot-air Anti-icing System

对后掠翼热气防冰系统的表面温度进行了数值仿真研究.用欧拉方法计算局部水收集系数,外部对流换热系数用附面层积分法计算,蒙皮导热和内部换热用计算流体力学(CFD)方法计算,用基于FLUENT的用户自定义函数(UDF)方法将外部换热、蒙皮导热和内部换热三者耦合求解,实现了热流边界条件的自动加载和温度的自动更新.通过对ARJ21-700机翼防冰系统性能的计算,说明所研究的计算方法能对三维后掠翼热气防冰系统作出总体性能的评估和局部性能的评价,为自然结冰条件下飞机的飞行试验提供依据,从而大大降低飞行试验风险.     

航空发动机低压转子系统的“可容模态”设计及实验验证

建立了带弹性支承和阻尼器的航空发动机低压柔性转子动力学模型,进行了模态计算以及临界转速处的响应计算。在考虑临界转速约束与“临界跟随”现象约束的条件下,综合模态不平衡影响因子、弹支应变能占比以及套齿连接结构稳定性构造了可容度评价函数,建立了低压转子系统的“可容模态”优化设计方法。设计并搭建了低压转子实验系统,从模态测试实验、阻尼器减振实验以及长时间“共振”实验,验证了设计方法的可靠性。研究结果为计算的临界转速与实际测量的临界转速最大误差为3.86%,阻尼器在1阶与2阶临界转速处的减振比最大可达45.6%,实验转子系统在1阶与2阶临界转速处各完成了长达412.5 s和429.8 s的“共振”实验,共振过程中转子系统各通道振动单峰值稳定在100μm以内,且无次谐波产生。表明了所建立的航空发动机低压转子系统“可容模态”优化设计方法是可行的。     

第3代新型低碳高合金钢弧齿锥齿轮失效分析

在中央传动调试试验中发生主动弧齿锥齿轮轮齿断裂故障,并连带其他部件产生不同程度损伤。主动弧齿锥齿轮整个圆周的接触印痕偏向小端一侧、靠近齿底,从动弧齿锥齿轮接触印痕分布在小端齿顶部位,印痕已不完整、局部超出工作面。为了排除15Cr₁₄Co₁₂Mo₅Ni₂钢弧齿锥齿轮试验中发生的断裂故障,对齿轮进行宏观检查、断口分析、组织检查、硬度测试、成分分析、啮合印痕仿真分析与验证,确定了故障齿轮断裂的性质和产生原因。结果表明：主动弧齿锥齿轮为高周疲劳断裂,疲劳起源于小端面与齿凸面根部转接棱角部位,与材质与冶金缺陷无关;在工作过程中存在异常咬合是导致该齿轮产生早期疲劳开裂的主要原因。建议优化齿面加工参数,提高齿轮工作过程中的咬合质量,从而避免此类故障再次发生。     

基于位姿可达空间的太空机械臂容错路径规划

为了使太空机械臂在关节锁定故障后仍能继续完成后续任务,提出一种基于位姿可达空间的太空机械臂容错路径规划方法。基于牛顿-拉夫逊法计算太空机械臂关节人为限位,完成满足任务需求的退化工作空间求解,通过构造姿态可达度指标,在退化工作空间的基础上建立故障机械臂基坐标系下的位姿可达空间。通过在代价函数中增加最小奇异值代价项改进传统A^*算法,基于改进A^*算法在所建立的位姿可达空间内完成太空机械臂容错路径规划。所提方法综合了位姿可达空间与改进A^*算法各自的优势,实现了关节锁定故障太空机械臂同时满足避奇异与位姿可达要求的轨迹搜索。通过建立7自由度太空机械臂运动学模型开展数值仿真研究,仿真结果验证了所提容错路径规划方法的有效性。     

小天体软着陆中的地面特征区域提取与跟踪算法

考虑到自主导航过程中的特征区域检测与跟踪问题,提出了一种新的跟踪算法。该算法是基于DIMES框架。首先,对在软着陆过程中拍摄的行星表面图像进行亮度均衡化,对处理后的图像进行二值化;然后,对二值化特征区域进行模板匹配找出高度相关位置点;最后,根据特征区域之间的几何关系确定特征区域的搜索范围,再分别提取这些相关点所代表区域的特征向量,并且与模板的特征向量进行相似性分析从而找到相似性最大的位置点。通过两组小行星表面图片进行分析验证得到了较好的效果。     

基于电子倍增CCD的微光成像遥感器焦面电路设计

文章介绍了一种以EMCCD为探测器件的星载遥感器焦面电路实现方案。利用FPGA基于VHDL语言设计了驱动时序发生模块,运用直接数字频率合成技术、LVDS总线传输技术和大幅值信号放大技术构建了EMCCD硬件驱动电路。为满足卫星在线配置的需求,电路设置了遥控遥测接口模块。在EMCCD读出模块和焦面电源模块设计中提出了一定的降噪方法。最后,对EMCCD焦面电路样机进行测试,证实了该设计的有效性和可行性。