直升机坠毁响应的有限元模拟

 本文概述用非线性有限元技术对直升机结构的坠毁过程进行数值模拟。所分析的结构包括飞行员座椅、座椅减震器、地板盒段和滑撬。问题被当作结构在规定初速度或脉冲载荷作用下的非线性（大变形与弹塑性）动反应。用特殊设计的单元模拟减震器及座椅滑轨,用间隙单元模拟结构与地面的撞击。     

杯杯型复合挤压两种宏观缺陷并存分析

 通过杯杯型轴对称复合挤压两种宏观缺陷并存的上限分析表达式,研究了该变形方式下两种宏观缺陷并存区域与正挤部分、反挤部分变形程度和坯料相对余厚的关系。本文的模型及结论被实验结果所证实。     

强制偏流喷管的数值仿真

采用薄层Ｎ－Ｓ方程成功地求解了强制流喷管内的三维复杂流场，对通量项和压力项用Ｖａｎ Ｌｅｅｒ发展的矢通量分裂法进行了离散，对离散方程采用线超松弛方法迭代求解，在亚音速与超音速气流共同存在的出口边界分情况进行了处理。计算结果验证了强制偏喷管具有自动补偿外界压力变化的能力，与实验结果基本吻合。     

相变光盘的介质优选及理论计算

 本文着重论述相变光盘的存储机理、介质优选、理论计算及光存储最新进展。     

高密度喷气燃料与常规喷气燃料浓度场试验研究

本文利用ＣＯ２红外气体分析仪和取样管对高密度喷燃料和常规喷气燃料在直流喷嘴下游的浓度场分布进行了测量，就气流速度，油压降和下游距离对浓度场分布的影响进行了对比研究。试验结果表明，在相同工况下，常规喷气燃料的最大浓度值比高密度喷气燃料的大；气流速度和油压变化对高密度喷气燃料最大浓度点穿透深度的影响大于对常规喷气燃料的影响。     

Satellite fault diagnosis using a bank of interacting Kalman filters

The main objective of this work is development and testing of a detection, isolation, and diagnosis algorithm based on interacting multiple model (IMM) filters for both partial (soft) and total (hard) reaction wheels faults in a spacecraft. This is shown to be accomplished under a number of different faulty mode scenarios for these actuators associated with the attitude control system (ACS) of a satellite. Various operating and faulty conditions due to changes and anomalies in the temperature, the power supply line voltage, and the loss of effectiveness of the torque and the current are considered in each reaction wheel associated with the three axes of the satellite. Once a fault mode is detected and isolated the recovery procedure can subsequently be engaged by invoking appropriate switching control strategies for the ACS. The application of a bank of interacting multiple Kalman filters for detection and diagnosis of anticipated reaction wheel failures in the ACS is described and developed. Compared with other model-based fault detection, diagnosis and isolation(FDDI) strategies developed in the control systems literature, our FDDI strategy is shown, through extensive numerical simulations, to be more accurate and robust with potential for extension to a number of other application areas.     

分轴燃气轮机大扰动动态过程计算

由我国自行设计和生产的燃气-蒸汽联合循环装置已经在东炼试运成功。其燃气轮机是用斯贝核心机改型的分轴燃气轮机。发电机组采用了双转速调节系统来代替功频调节系统,以消除气体燃料热值变化引起的工况变化。为确保甩负荷时大扰动动态过程计算的准确度,采用了以非稳态工况为起始点的数学模型,用变系数分段小偏差线性化的方法计算大扰动的动态过程,从而解决了非线性系统动态过程的计算问题。     

机动飞行时安装角对转子叶片振动的影响

提出旋转转子叶片在轴线发生平面偏转时的振动问题。在非线性曲杆理论的基础上，建立了在陀螺力作用下叶片振动的微分程及其求解方法，并进行了数值分析。结果表明，安装角在不同取值范围和不同转速范围对叶片振动的影响是完全不同的。对于无扭向叶片在低转速下，安装角对振动的影响是显著的；而在高转速下则是很微弱的。当安装角在某个较大的范围取值时，可有效地减弱该运动状态所导致的振动。     

燃气发生器中注入水蒸汽对燃烧效率和总压损失的影响

试验是在一个 WZ- 5燃气发生器上进行的 ,燃料用低热值气态燃料 (体积热值为 8172 k J/N· m3) ;水蒸汽可由燃烧室前部或从后部掺混孔处注入。试验结果表明 ,水蒸汽注入对燃烧效率影响不大而使总压损失增加。当水蒸汽流量与总空气流量之比为 10 % ,且水蒸汽从后部掺混孔处注入 ,则总压损失会增大 12 %左右 ;如果水蒸汽从前排注入 ,则总压损失会更大些。     

Probing the era of galaxy formation via TeV gamma ray absorption by the near infrared extragalactic background

We present models of the extragalactic background light (EBL) based on several scenarios of galaxy formation and evolution. We have treated galaxy formation with the Press-Schecter approximation for both cold dark matter (CDM) and cold+hot dark matter (CHDM) models, representing a moderate (z _f 3) and a late (z _f 1) era of galaxy formation respectively. Galaxy evolution has been treated by considering a variety of stellar types, different initial mass functions and star formation histories, and with an accounting of dust absorption and emission. We find that the dominant factor influencing the EBL is the epoch of galaxy formation. A recently proposed method for observing the EBL utilizing the absorption of 0.1 to 10 TeV gamma-rays from active galactic nuclei (AGN) is shown to be capable of discriminating between different galaxy formation epochs. The one AGN viewed in TeV light, Mrk 421, does show some evidence for a cutoff above 3 TeV; based on the EBL models presented here, we suggest that this is due to extinction in the source. The large absorption predicted at energies > 200 GeV for sources at z > 0.5 indicates that observations of TeV gamma-ray bursts (GRB) would constrain or eliminate models in which the GRB sources lie at cosmological distances.Now at University of Chicago, Dept. of Astronomy & Astrophysics.