密闭燃烧器法固体推进剂燃速测试系统

就才燃烧器法测试系统部分的硬件、软件进行了全面统一的设计,尤其是在软件部分引入了数据库管理系统,不仅使该软件能查询实验相关的数据,还使该软件具备了一定的智能,可以辅助识别推进剂燃速。     

单晶涡轮叶片三维晶体取向相关性能分析及优化

采用单晶正交各向异性弹性本构关系,分析了三维晶体取向对单晶涡轮叶片应力分布、蠕变寿命、低周疲劳寿命及叶尖径向位移的影响.结果表明,三维晶体取向对单晶叶片上述性能存在显著影响,且3个取向角之间相互耦合,偏差角对叶片性能的影响随着随机角的方位而变化,随机角对叶片性能的影响也随着偏差角的角度而不同.在此基础上,应用ISIGHT构建了单晶叶片全三维取向优化平台,以蠕变寿命、低周疲劳寿命及叶尖最大径向位移为优化目标,采用邻域培植多目标遗传算法进行了叶片三维取向优化,所得Pareto解聚集在偏差角12°的区域内.选择寿命最长的Pareto解作为最优解,相对于初始强度计算点,蠕变寿命提高6倍,低周疲劳寿命提高37倍,叶尖最大径向位移减小2.5%.      

GHOST FLUID METHOD FOR RICHTMYER-MESHKOV INSTABILITY SIMULATION

INTRODUCTIONThe energy of the Richtmyer- Meshkov in-stability is excited by the interaction between ashock wave and a contact interface across thatfluids are different.Itis very important thatcap-ture the interface in multi- material flows exact-ly.Here we will apply the ghost fluid method tosimulate two dimensional Richtmyer- Meshkovinstability.The mathematical equation used to simulatethe Ritchmyer- Meshkov instability is the com-pressible Euler equation for two ideal gases.ρρuρvE…     

推力矢量飞机平衡特性研究

通过建立推力矢量飞机数学模型，分析其平衡状态的基本特征，利用连续算法对其平衡面进行计算，以及对其仿真结果比较分析，介绍推力矢量技术的发展状况，从而全面理解推力矢量系统配置下飞机的优越机动性能。     

凸壳的结构与直径

本文是讨论线性空间和赋范线性空间中集合 E 的凸壳 conV(E)的性质,首先推出了线性空间中 ConV(E)的结构表示。进而在赋范线性空间中证明了diam(conV(E))=diam(E)。     

400Hz电流互感器校验仪的检定

介绍了用功率源法与分流法相结合对电流互感器校验仪进行检定的方法，并给出了检定结果的不确定度。该方法已应用于新研制的400Hz电流互感校验仪的检定，对于工频的电流互感器校验仪的检定也有一定的参考价值。     

Deep Impact: The Anticipated Flight Data

A comprehensive observational sequence using the Deep Impact (DI) spacecraft instruments (consisting of cameras with two different focal lengths and an infrared spectrometer) will yield data that will permit characterization of the nucleus and coma of comet Tempel 1, both before and after impact by the DI Impactor. Within the constraints of the mission system, the planned data return has been optimized. A subset of the most valuable data is planned for return in near-real time to ensure that the DI mission success criteria will be met even if the spacecraft should not survive the comet’s closest approach. The remaining prime science data will be played back during the first day after the closest approach. The flight data set will include approach observations spanning the 60 days prior to encounter, pre-impact data to characterize the comet at high resolution just prior to impact, photos from the Impactor as it plunges toward the nucleus surface (including resolutions exceeding 1 m), sub-second time sampling of the impact event itself from the Flyby spacecraft, monitoring of the crater formation process and ejecta outflow for over 10 min after impact, observations of the interior of the fully formed crater at spatial resolutions down to a few meters, and high-phase lookback observations of the nucleus and coma for 60 h after closest approach. An inflight calibration data set to accurately characterize the instruments’ performance is also planned. A ground data processing pipeline is under development at Cornell University that will efficiently convert the raw flight data files into calibrated images and spectral maps as well as produce validated archival data sets for delivery to NASA’s Planetary Data System within 6 months after the Earth receipt for use by researchers world-wide.     

强激光与高超声速球锥流场干扰数值模拟研究

本文采用有限差分技术，数值求解带能量源项与空气11组分化学动力学模型的轴对称粘性流体力学方程组，采用类氢原子理论模型计算空气对激光的吸收系数，建立了模拟强激光与超声速钝体流场干扰的计算软件，得到了高能浙江与超声速球锥流场干扰数值模拟的结果。     

校准实验室质量体系综合评判方法

采用模糊集合理论来处理校准实验室质量体系的综合评判问题.描述了建立模糊评价模型的方法,并给出了实际的应用计算.     

十一组元高温平衡、非平衡空气光谱吸收系数计算

飞行器以很高的马赫数再入大气层时 ,头部激波层、尾迹的气体辐射产生的紫外、可见、红外特征信号 ,是地面监测和反导制导系统探测、识别的主要依据 ;同时 ,头部气体层热辐射也是再入体壁面加热热流的重要源项。激波层内高温气体吸收系数是目标紫外、可见光、红外辐射特性计算、热防护计算和气动流场辐射场耦合计算的基本参数。本文分析了再入过程中高超声速稀薄气体流的非平衡现象 ,采用三温度模型 (电子能温度 Te、振动能温度 TV、转动和平动能温度 TR)来表征激波层内非平衡态的气体组份各个能级占有数分布 ,并由原子分子辐射理论直接计算 N2 ,N+ 2 ,N,N+ ,O2 ,O+ 2 ,O,O+ ,NO,NO+和 e-等 1 1种主要空气组元各种能级跃迁对辐射的贡献 ,最终得到平稀和非平衡高温空气吸收系数计算模型。计算结果可见光区与试验结果符合较好 ,紫外、红外区结果稍差