页轮干式磨削Ti6Al4V合金

进行了Ti6A14V合金锆刚玉页轮和碳化硅页轮的磨削性能试验研究,分析了磨削用量对磨削力、磨削温度和磨削表面完整性的影响。磨削力通过KISTLER9265B测力仪测定,磨削表面温度由NIUSB-621X信号采集系统测得,磨削表面形貌和金相组织由HiroxKH-7700型体视显微仪和Quanta200型扫描电镜（SEM）观察,表面粗糙度由Mahr Perthometer M1粗糙度仪测得,表层显微硬度通过HVS—1000硬度计测定。研究结果表明：页轮磨削钛合金工件表面没有发生烧伤现象,磨削热影响区厚度小于50μm,锆刚玉页轮比碳化硅页轮更适合干式磨削钛合金。     

TC4钛合金激光焊中工艺参数对气孔生成量的影响

文摘研究了TC4钛合金激光焊接在平焊、横焊两种位置下工艺参数对气孔生成量的影响。结果表明:平焊时,气孔生成量随激光功率、离焦量的增大先减小后增大,随焊接速度的增大先增大后减小;横焊时,气孔生成量随激光功率的增大而增大,随焊接速度的增大而减小,随离焦量的增大先减小后增大。利用正交试验方法得到的优化工艺参数进行焊接,气孔生成量大幅减少,在两种位置下均可得到内部质量良好的焊缝。     

信息系统群演化的综合环境SEE的研究

旨在通过对系统构架各视角的研究，开发一个信息系统综合演化环境，从而提供针对各类系统演化特征的通用的解决方案，并利用方法论的手段规范、指导和维护系统(群)的演化活动。本文首先论述了大型系统中各个系统和组件变化及改进活动中存在的问题，分析相关的研究及面临的挑战，从而提出系统群演化的概念。然后文章概括了系统群演化的特征，提出解决以上问题的思想方法，即开发“信息系统群演化的综合环境(Synthetic environment of evolution，SEE)”，将各种演化活动纳入规范，指导系统群的演化活动；在此基础上，进一步就实现SEE的关键技术给出了描述及运用的范例。     

MPEG-4视频DCT量化模块的FPGA实现

介绍了一种采用FPGA技术实现MPEG-4 ASP级视频DCT量化模块的设计方案。该模块包括二维DCT／IDCT、量化／反量化和帧内直流／交流(DC／AC)预测。用VHDL进行描述并通过模拟试验表明,该模块可在880个时钟周期内处理完一个宏块的数据,工作频率达到40MHZ。文章采用全硬件实现方法,提出了各模块的硬件电路结构设计,减少了电路规模。     

2-氯-4,6-二硝基-1,3-苯二酚萃取热力学研究

采用萃取平衡实验法,研究了用有机溶剂萃取水相中2-氯-4,6-二硝基-1,3-苯二酚的萃取热力学性质。考察了选用乙酸乙酯作萃取剂,苯、甲苯、环己烷和正庚烷作稀释剂时对萃取水相中2-氯-4,6-二硝基-1,3-苯二酚的影响。结果表明,萃合物的结构与稀释剂的种类有关,并且2-氯-4,6-二硝基-1,3-苯二酚在有机相中的分配系数随稀释剂介电常数的增大而增大。通过研究温度对萃取过程的影响,证实了乙酸乙酯从水相中萃取2-氯-4,6-二硝基-1,3-苯二酚的过程是一个放热过程,表观热效应ΔH=-10.088 kJ/mol。     

大型复杂航天器结构有限元模型的验证策略研究

大型复杂航天器结构有限元模型的合理性和准确性在航天器研制过程中具有重要意义, 它是开展星箭耦合分析以及力学环境条件设计等工作的基础。首先综合有限元建模、模 态试验、相关分析和模型修正等技术构造了一套系统的航天器结构有限元模型试验验证策略 ;然后,针对我国新一代大型卫星平台——东方红四号卫星开展了整星有限元模型的试验 验证研究,其中整星模态试验以及模型修正等研究工作属首次在东方红四号卫星平台上成功 实施。修正后有限元模型对整星主模态频率预测误差小于5％,模态置信准则大于0.6,预 示精度达到工程要求。
     

基于均匀化方法的轴编C/C复合材料性能预测

把均匀化理论与有限元法相结合,应用于轴棒法多维编织C/C复合材料的性能预测,通过对该材料有效模量的计算和实验验证,表明本方法可以得到较准确的材料刚度性能,为该材料的设计提供了性能预测方法.     

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).     

着陆姿态对地外天体表层采样的影响研究

表层采样技术是获得地外天体特性的重要手段,是完成地外天体采样任务的一项关键技术。文章结合4自由度表层采样装置的特点,建立了表层采样装置的逆运动学模型,分析了极限着陆姿态下表层采样装置安装位置在当地参考坐标系中的变化,并针对一次封装与二次封装过程中表层采样装置的位置和姿态要求,明确了末端采样器姿态补偿方法,提出了着陆姿态对表层采样影响的分析算法。仿真结果表明,该算法能有效分析着陆姿态对表层采样的影响,可为表层采样装置适应性设计提供支持。     

A systematic approach to nonlinear rotorcraft model identification

The development of a powerful parameter estimation routine and its integration into the simulation environment HOST is described. With this tool approaches are being made towards new strategies of mathematical modeling, aimed at providing highly accurate and nevertheless run-time efficient simulation models. The identification routine is capable of optimizing parameterized models in both dynamic time domain simulation and static (e.g. trim state variation) conditions. Examples of both cases are presented to emphasize the improvement in the system response prediction and to demonstrate the abilities of the identification techniques in combination with the nonlinear simulation platform. This article reviews the activities and achievements accomplished by the DLR Institute of Flight Research and the ONERA Systems Control and Flight Dynamics Department during the last few years in the research on rotorcraft flight dynamics modeling and model identification. Future activities that require extensive high fidelity modeling are in the scope of the current and coming modeling activities that include the use of the presented methods and software technologies.