动量轮维纳过程退化建模与寿命预测

针对动量轮寿命预测无失效数据问题,利用有漂移的维纳过程对其轴承温度建立性能退化模型,同时,考虑由于加工工艺、制造误差等因素所造成的不确定性,利用随机变量来描述其漂移参数和扩散参数,并结合自助法获取纠偏估计.根据所建模型仿真了轴承温度维纳过程的样本路径,最后,对动量轮进行随机失效阈值情形的寿命预测和剩余寿命预测.该模型为...     

改性BMI树脂固化过程的温度控制优化

针对以改性双马来酰亚胺树脂(BMI)为基体的树脂膜熔渗(RFI)成型工艺,以三维热传导方程与固化动力学模型为控制方程,采用有限元/有限差分方法对所得方程进行离散求解。为了衡量固化质量,提出了两个新的控制参数,并用于最优固化温度控制工艺的模拟。数值结果表明,构件内部温度与固化度均高于表面,而固化保持温度和起始时间会对构件中温度和固化度的均匀性产生较大影响。数值模拟结果对固化过程的优化设计有重要的指导意义。     

真空导入模塑工艺树脂流动行为研究进展

综述了近年来真空导入模塑工艺树脂流动行为的研究进展,结合自己的研究成果系统地评述了真空导入模塑工艺中树脂的流动模型及机理、流动行为的数值模拟和流动行为的监测控制,并在此基础上对真空导入模塑工艺树脂流动行为的研究前景进行了展望。     

双轴涡喷发动机脉冲停供油时动态过程的数值模拟

在数值模拟双轴涡喷发动机脉冲停供油时动态工作过程中, 考虑到脉冲停供油会引起燃烧效率和涡轮效率恶化, 从而偏离特性图上所示值, 且因实验较难获得上述效率修正关系, 因此提出用实测的高、低压转速曲线代替上述效率做为数值模拟的已知条件。应用这一方法模拟了某型发动机脉冲停供油时的动态过程, 数值结果与实验值基本符合, 并获得该动态过程燃烧效率数据。      

The primordial Helium-4 abundance determination: systematic effects

By extrapolating to O/H = N/H = 0 the empirical correlations Y–O/H and Y–N/H defined by a relatively large sample of 45 Blue Compact Dwarfs (BCDs), we have obtained a primordial ⁴Helium mass fraction Y _p=0.2443±0.0015 with dY/dZ=2.4±1.0. This result is in excellent agreement with the average Y _p=0.2452±0.0015 determined in the two most metal-deficient BCDs known, I Zw 18 (Z /50) and SBS 0335–052 (Z /41), where the correction for He production is smallest. The quoted error (1) of 1% is statistical and does not include systematic effects. We examine various systematic effects including collisional excitation of hydrogen lines, ionization structure and temperature fluctuation effects, and underlying stellar Hei absorption, and conclude that combining all systematic effects, our Y _p may be underestimated by 2–4%. Taken at face value, our Y _p implies a baryon-to-photon number ratio =(4.7^+1.0 _–0.8)×10^–10 and a baryon mass fraction _b h ² ₁₀₀=0.017±0.005 (2), consistent with the values obtained from deuterium and Cosmic Microwave Background measurements. Correcting Y _p upward by 2–4% would make the agreement even better.     

变温热源回热式布雷顿循环的功率密度特性

用有限时间热力学方法分析变温热源条件下不可逆回热式布雷顿循环的功率密度特性，计人工质与高、低温测换热器的热阻损失，压气机、涡轮机的不可逆压缩和膨胀损失和管路系统中的压力损失，导出了功率密度与压比间的解析式，并通过数值计算将对应于最大功率密度时的一些参数与对应圩最大功率时的同样参数进行了比较。     

连续玻璃纤维增强热塑性复合材料工艺及力学性能的研究

选择三种国产高性能热塑性树脂 ,聚醚砜、酞侧基聚醚砜、酞侧基聚醚酮和高强玻璃纤维粗纱 ,采用连续预浸渍技术和高温、高压成型工艺 ,确定出合理的工艺参数 ,分别制备了树脂基体试件和单向板试件 ,并对其进行了相关力学性能试验研究。通过扫描电镜对单向板试件断口进行了分析     

Falkner-Skan流空间演化的二次稳定性研究

依据Floquet理论建立三维亚谐扰动的控制方程，研究Falkner-Skan流的二次稳定性问题。采用高精度的谱方法进行数值模拟，结合边界层特性有效地配置边界条件，引入不同类型压力梯度，研究在压力梯度下的二维有限振幅的Tollmien-Schlichting（TS）波对三维亚谐扰动的产生、发展和演化的作用和影响。结果表明，顺压梯度的存在可以减缓二次不稳定的发生和演化，而逆压梯度却加速了二次不稳定性。     

Helium-3: Status and Prospects

We report on our continuing efforts to determine 3He abundances in H II regions and planetary nebulae. Our detections of 3He in some PNe show that some stars produce large amounts of 3He. However the H II region abundances show no evidence for this production. From our sample of > 40 H II regions, the subsample which should yield the most reliable abundances has 3He/H abundances which scatter between 1-2 × 10-5. There is no trend with either galactocentric distance or metallicity. Even if we do not understand the underlying mechanisms, we see empirically that stars neither produce nor destroy 3He in a major way. We thus suggest that the level of the "3He Plateau" (3He/H = 1.5 _-0.5 ^+1.0 × 10^-5) is a reasonable estimate for the primordial 3He.     

Galactic Evolution of D and 3He

The most recent chemical evolution models for D and 3He are reviewed and their results compared with the available data.Models in agreement with the major galactic observational constraints predict deuterium depletion from the Big Bang to the present epoch smaller than a factor of 3 and therefore do not allow for D/H primordial abundances larger than 5 × 10-5. Models predicting higher D consumption do not seem to be able to reproduce other observed features of our galaxy (e.g. SFR, abundances, abundance ratios and/or gradients of heavier elements, metallicity distribution of G-dwarfs).Observational and theoretical 3He abundances can be reconciled with each other if the majority of low mass stars experience in the red giant phase a deep mixing allowing the consumption of most of the 3He produced during core-hydrogen burning.