多元线性回归在坐标测量中的应用

简要介绍了多元线性回归的数学原理,重点分析了坐标测量中利用回归分析进行基本几何要素处理计算的原理、方法和预处理技巧,在此基础上介绍和讨论了形位误差的处理计算方法。     

NIM4#铯冷原子喷泉钟新一代时间频率基准

回顾了NIM4 #钟实现 5 μK冷原子云 ,74cm原子喷泉和 0 95Hz线宽Ramsey跃迁实验 ,报道了 9 19GHz微波锁定到铯原子秒定义跃迁 ,频率稳定性达到 (5 - 7)× 10 -15(15 0 0 0s)。目前我们正在进行不确定度评估 ,可望不确定度进入 10 -15量级 ,建立我国新一代时间频率基准装置。     

磁云—高速流相互作用的数值模拟

对１９７８年８月２７至２８日期间观测到的磁云与尾随高速流的相互作用进行数值模拟，基本拟合了１ＡＵ处的观测剖面。模拟结果表明，磁云－高速流系统将导致前向快，慢激波和后向快激波的形成。     

The population of massive stars in R136 from HST/FOC UV observations

New ultraviolet (1300 A, 3400 A),HST FOC observations have been used to derive the UV color-magnitude diagram (CMD) of R136, with the main scientific goal of studying the upper end of the stellar mass function at ultraviolet wavelengths where the color degeneracy encountered in visual CMDs is less severe. The CMD has been compared to a set of theoretical isochrones, which have been computed using the latest generation of evolutionary models and model atmospheres for early type stars. Wolf-Rayet stars are included. Comparison of theTheoretical andobserved CMD suggests that there are no stars brighter than M₁₃₀–11. We use the observed main sequence turn-off and the known spectroscopic properties of the stellar population to derive constraints on the most probable age of R136. The presence of WNL stars and the lack of red supergiants suggests a most likely age of 3±1 Myr. A theoretical isochrone of 3±1 Myr is consistent with the observed stellar content of R136 if the most massive stars have initial masses around 50 M.Bases on Observations with the NASA/ESA Hubble Space Telescope, obtained at the STScI, which is operated by AURA, Inc., under NASA contract NAS5-26555.Astrophysics Division, Space Science Department, ESA     

Experimental Aspects of Mid-Frequency Pulsations (f≈10–100 mHz) in the Southern Polar Cap

We review the results obtained in the frequency range of Pc3 (22-100 mHz) and Pc4 (7-22 mHz) pulsations at Italian Antarctic stations in the southern polar cap (“Mario Zucchelli”, at Terra Nova Bay, TNB, 80^˚.S; “Concordia”, the Italian/French base at Dome C, DMC, 89^˚.S). The absence of a midnight enhancement in the pulsation power suggests a negligible substorm influence at extreme latitudes, while the sharp noon enhancement, which appears only at TNB, is determined by the closer proximity of the station to cusp related phenomena. The relationship between the frequency of the band-limited signals and the interplanetary magnetic field strength, the cone angle influence, and the higher correlation of the Pc3 power with the solar wind speed in the morning hours suggest a global scenario in which upstream waves would be mainly responsible for the mid-frequency activity in the polar cap. However, the polarization pattern is odd with respect to the predictions for tailward propagating modes.     

基于N-S方程的翼型实验侧壁边界层控制

使用三维可压、雷诺平均N-S方程数值计算了NACA0012翼型在二元翼型风洞中不同迎角和马赫数状态下的压力分布,改进了划分计算网格的Hilgenstock方法,发展了一种利用N S方程计算结果,来确定翼型实验中为消除侧壁边界层干扰的抽气压力的方法。通过比较利用本文介绍的方法计算的NACA0012翼型实验侧壁抽气压力和相同状态下,在西北工业大学0.3m×0.1m二维跨音速风洞中经油流显示证明为合适的抽气压力,结果表明该方法是可行的。     

虚拟企业的知识分布与管理

文章从知识与决策权相匹配的角度解释虚拟企业分权化的原因,并提出在分权后,应采用改变激励因素、加强信息交流、建立知识共享模式、进行组织学习、实施知识管理战略等手段对分散的知识进行有效的协调和控制.     

钛合金板材激光弯曲成形的研究

 对常温下钛合金板材进行了激光弯曲成形研究。分析了激光功率、扫描速度、光斑大小对板材弯曲变形的影响,获得理想工艺参数范围为:功率1 .0～1 .2 k W、扫描速度2～3 m/min、光斑直径6～7mm。同时分析了板材厚度、宽度及扫描次数对材料弯曲变形的影响,为钛合金板材弯曲成形提供了一种新途径。     

体现裕度定制思想的轴流压气机二维特性预估方法

为实施裕度定制，本文开发了能够体现裕度定制思想的轴流压气机二维特性预估方法。精细考虑了前后缘形状、最大弯度位置等，尤其是通过考虑叶片力而全面包含掠影响是本方法的重要特色。为初步验证本方法，对NASA37和NASA67转子进行了性能预估并与试验结果进行了对比。结果表明，本方法基本可靠，可以用于裕度定制目的。     

VB6．0下级进模俯视图绘制智能化的研究

在VB6．0下研究典型级进模排样图形和其俯视图绘制的联系，利用VB6．0软件邮长圆形典型冲件级进模俯视图形设计的智能化，并给出了该软件程序运行生成的一个长圆形典型冲件级进模俯视图形。