穿孔泡沫夹层复合材料低速冲击性能试验研究

针对普通泡沫夹层复合材料层间性能较弱的问题，提出在泡沫上预先打孔的方法，在泡沫芯材中形成胶钉从而提高泡沫夹层材料的力学性能，并对穿孔泡沫夹层复合材料的低速冲击性能进行了研究。通过手糊和真空辅助成形工艺制备穿孔泡沫夹层复合材料试验件，对其进行不同能量的低速冲击试验，记录接触力、冲头位移和能量吸收率等力学响应，并采用目视检测和超声C扫无损检测两种方法确定冲击损伤的范围，探究胶钉密度、打孔深度和泡沫槽宽等变量对穿孔泡沫夹层复合材料低速冲击阻抗性能的影响。试验结果表明，随着冲击能量的增加，最大接触力、最大冲头位移和残余变形均增加，凹坑深度和内部损伤面积也增大，同时结构的能量吸收率也有所提高；适当地增加胶钉密度和泡沫槽宽能提高穿孔泡沫夹层材料的低速冲击阻抗性能，而泡沫孔深度对其冲击性能的影响较小。     

基于二维紧凑型四阶格子模型的激波管流动模拟

为了提高格子的稳定性，使用Hermite展开方法，构建了新的二维四阶紧凑型格子模型，即D2Q37A。比较了D2Q37A和与Philippi给出的紧凑型格子模型(D2Q37B)的稳定性。在相同的碰撞频率下，与D2Q37B相比，D2Q37A可以模拟初始密度比更高的一维激波管流动。这表明D2Q37A与现有格子模型相比，具有更好的稳定性。详细给出了适用于高阶格子模型的边界条件实现方式。此边界条件实现方式保留了体现LBM（lattice Boltmann method）粒子特性的迁移 碰撞机制。用以上给出的格子模型和边界条件处理方式模拟激波管流动，得到的模拟结果和解析解吻合得很好。这表明所给出的边界处理方式是可行的。此边界格式同样可以用于其他类型的流动和边界。      

Robust extension of the simple sea-surface irradiance model to handle cloudy conditions for the global ocean using satellite remote sensing data

Sea-surface solar radiation (abbreviated as photosynthetically available radiation, PAR) in the visible wavelength (400–700 nm) is an essential parameter to estimate marine primary productivity and understanding phytoplankton dynamics, upper ocean physics and biogeochemical processes. Although many remote-sensing models were developed to estimate daily PAR (DPAR) from ocean colour data, these models often produce biases in the DPAR products under cloudy-sky and complex atmospheric conditions due to the lack of parameterization to deal with the cloud cover conditions and insufficient in-situ DPAR data. This study presents an Extended Sea-surface Solar Irradiance Model (ESSIM) for estimating DPAR over the global ocean. The ESSIM uses the direct and diffuse components from the Simple sea-surface Solar Irradiance Model (SSIM) along with a new parameter to handle cloudy conditions. The ESSIM produced DPAR products with greater accuracy under both clear and cloudy conditions. Its performance was tested on the time-series MODIS-Aqua images and compared with the concurrent in-situ data and the results from two global models. Results showed that the DPAR values produced by ESSIM agree with in-situ data better than the global models for all-sky conditions (with a mean relative error of 11.267 %; a root mean square error of 5.563 Em^?2day^?1; and a mean net bias of 2.917 Em^?2day^?1). The ESSIM performed slightly better than the SSIM for clear conditions and the Frouin's Operational Algorithm (FOA) for all-sky conditions. As the new parameterization accounts for cloudy conditions, the ESSIM produced more accurate results for cloud cover conditions across latitudes (up to 60°). The time-series Level-3 binned MODIS-Aqua data (global gridded) also demonstrated that the ESSIM improved the accuracy of DPAR products and produced spatially and temporally consistent DPAR products over the global ocean regardless of the seasons and sky conditions.     

Ground-based investigations on phase-moving phenomenon with space sublimation cooling for lunar exploration missions

The lunar surface is a typical vacuum environment, and its harsh heat rejection conditions bring great challenges to the thermal control technology of the exploration mission. In addition to the radiator, the sublimator is recommended as one of the promising options for heat rejection. The sublimator makes use of water to freeze and sublimate in a porous medium, rejecting heat to the vacuum environment. The complex heat and mass transfer process involves many physical phenomena such as the freezing and sublimation phase change of water in the porous medium and the movement of the phase-change interface. In this paper, the visualized ground-based experimental approaches of space sublimation cooling were presented to reveal the moving law of three-phase point and the growth phenomenon of ice-peak and icicle in microchannels under vacuum conditions. The visualized experiments and results prove that the freezing ice is divided into the porous ice-peak and the transparent icicle. As the sublimation progresses, the phase-change interface moves downward steadily, the length of the ice-peak increases, but the icicle decreases. The visualized experiments of space sublimation cooling in the capillary have guiding significance to reveal the sublimation cooling mechanism of water in the sublimator for lunar exploration missions.     

航空滚动轴承振动特征的故障灵敏度分析与融合技术

针对工程中航空滚动轴承实时状态监测的需要，提出了基于标准化欧氏距离的多特征融合评估方法。首先，进行了航空滚动轴承故障模拟试验，引入了故障灵敏度的定量评价指标，对融合前后特征的故障灵敏度进行了分析；在此基础上，将所提方法与主分量分析、支持向量数据描述和支持向量分布估计方法相比较；最后，进行了轴承疲劳加速试验，将所提融合方法应用于航空滚动轴承状态监测。试验表明:相比于主分量分析、支持向量数据描述和支持向量分布估计，基于标准化欧氏距离的融合值的故障灵敏度更高；其对不同类型、不同阶段的航空滚动轴承故障更加灵敏，相比于有效值更适合作为航空滚动轴承状态监测的指标。      

非结构嵌套网格中的一种改进型径向基函数插值方法

非结构混合网格拓扑关系相对复杂,在嵌套边界区域进行流场信息插值传递容易有精度的损失。利用已知的解析函数作为插值样本,对线性插值(LINE)、距离倒数权重插值(WA)、逆二次径向基函数插值(IQ)、Wendland暞sC2径向基函数插值四种方法的精度进行对比,筛选出精度较高的C2径向基函数;提出一种改进的C2径向基函数插值方法,通过调整径向基函数的作用半径来控制插值矩阵条件数,进而消除使用径向基函数插值在嵌套边界区域出现的数值奇性问题;选用MD30P/30N 多段翼与三维AEDC典型外挂物分离模型对该插值方法进行验证。结果表明:改进后的径向基函数插值方法能够有效消除嵌套边界区域数值奇性,同时计算收敛速率更快,插值精度更高。     

航空发动机需求管理方法研究

为在全生命周期内保证"用户和其他利益攸关者"的需求被充分理解和执行,提出以产品分解结构PBS为基础,构建航空发动机需求管理的瀑布型模型。将复杂的航空发动机需求管理工作模块化,制定以产品符合性为目标的需求管理流程,并以该流程为依托提出航空发动机的需求管理方法。该方法提升了全生命周期内的需求管理能力,为航空发动机产品的成功研制提供了有力保障。     

航空发动机主轴轴承状态监测研究现状与发展趋势

航空发动机主轴轴承承受着高温、高速、重载、贫油、断油等极端工况,其疲劳、磨损等失效问题严重影响发动机的可靠性.因此,对航空发动机主轴轴承的使用状态进行有效精确监测极为重要.对航空发动机主轴轴承工况特点、主要失效模式和失效机制进行了梳理;针对主轴轴承的状态监测方法和技术,总结并对比分析了现有主轴轴承振动、滑油状态、声音、...