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941.
本文所讨论的B-SURF三维CAD系铣包括3-D几何设计与外形数值计算、3-D图形变换及处理、数控绘图与数控加工自动编程等部分,能实现CAD/CAM方面的十个功能。该系统以造型能力较强的重节点非均匀B样条方法为基础,并把重节点的信息应用到后置处理中去,以充分体现出该方法的优越性。系统具有一定的通用性,可用于无人机、轻小型飞机、汽车及其它具有复杂外形产品的几何设计与制造。 相似文献
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为了适应飞机舱门密封件研制周期较短以及正向设计的发展趋势,基于Abaqus-Isight软件对飞机舱门密封件进行仿真分析和优化设计,同时校准了材料参数,提出了两种对飞机舱门密封件的优化设计方法,通过对比得到更优的密封件结构。通过试验得到橡胶与织物的材料参数,基于Abaqus-Isight对材料参数进行校核,通过试验得到的压缩试验曲线对材料参数进行修正,得到与成品试验拟合度更高的材料参数;基于Abaqus-Isight对飞机舱门密封件进行DOE正交试验优化设计,将产品结构参数作为变量,压缩力、接触压力、摩擦损耗能作为优化目标,可以得到局部最优结构;将DOE正交试验结果拟合得到近似模型,通过Isight的近似模型算法得到全局最优结构,综合评估采用近似模型算法能够得到更为优异的结果。 相似文献
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Wei Wang Yihua YanMaohai Huang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
Very low frequency interferometry among two astronomical experiments has been proposed and accepted for further study for the second phase of China’s lunar exploration programme (the Chang’E Programme), which is envisaged to operate a lander and a rover on the surface of the moon. This experiment is an interferometer experiment in the very low frequency (VLF, f < 15 MHz) regime of radio frequencies with at least degree-level angular resolution. The goals include observing solar storm activities, Coronal Mass Ejections, Auroral Kilometric Radiation, and planetary radiation in the solar system, studying the origin of Cosmic Rays, spectral properties of pulsars, surveying ionized hydrogen in the Galaxy, and exploring coherent radio emissions. 相似文献
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Dan-Dan Liu Tao Yu Jing-Song Wang Cong Huang Wei-Xing Wan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Neural networks (NNs) have been applied to ionospheric predictions recently. This paper uses radial basis function neural network (RBF-NN) to forecast hourly values of the ionospheric F2 layer critical frequency(foF2), over Wuhan (30.5N, 114.3E), China. The false nearest neighbor method is used to determine the embedding dimension, and the principal component analysis (PCA) is used to reduce noise and dimension. The whole study is based on a sample of about 26,000 observations of foF2 with 1-h time resolution, derived during the period from January 1981 to December 1983. The performance of RBF-NN is estimated by calculating the normalized root-mean-squared (NRMSE) error, and its results show that short-term predictions of foF2 are improved. 相似文献
945.
X. Wang J.K. ShiG.J. Wang Y. Gong 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Monthly median values of foF2, hmF2 and M(3000)F2 parameters, with quarter-hourly time interval resolution for the diurnal variation, obtained with DPS4 digisonde at Hainan (19.5°N, 109.1°E; Geomagnetic coordinates: 178.95°E, 8.1°N) are used to investigate the low-latitude ionospheric variations and comparisons with the International Reference Ionosphere (IRI) model predictions. The data used for the present study covers the period from February 2002 to April 2007, which is characterized by a wide range of solar activity, ranging from high solar activity (2002) to low solar activity (2007). The results show that (1) Generally, IRI predictions follow well the diurnal and seasonal variation patterns of the experimental values of foF2, especially in the summer of 2002. However, there are systematic deviation between experimental values and IRI predictions with either CCIR or URSI coefficients. Generally IRI model greatly underestimate the values of foF2 from about noon to sunrise of next day, especially in the afternoon, and slightly overestimate them from sunrise to about noon. It seems that there are bigger deviations between IRI Model predictions and the experimental observations for the moderate solar activity. (2) Generally the IRI-predicted hmF2 values using CCIR M(3000)F2 option shows a poor agreement with the experimental results, but there is a relatively good agreement in summer at low solar activity. The deviation between the IRI-predicted hmF2 using CCIR M(3000)F2 and observed hmF2 is bigger from noon to sunset and around sunrise especially at high solar activity. The occurrence time of hmF2 peak (about 1200 LT) of the IRI model predictions is earlier than that of observations (around 1500 LT). The agreement between the IRI hmF2 obtained with the measured M(3000)F2 and the observed hmF2 is very good except that IRI overestimates slightly hmF2 in the daytime in summer at high solar activity and underestimates it in the nighttime with lower values near sunrise at low solar activity. 相似文献
946.
Hongliang Xu Jinling Wang Xingqun Zhan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Integrity is the ability of Global Navigation Satellite Systems (GNSS) to detect faults in measurements and provide timely warnings to users and operators when the navigation system cannot meet the defined performance standards, which is of great importance for safety of life critical applications. Compared with both Receiver Autonomous Integrity Monitoring (RAIM) and ground based GNSS Integrity Channel (GIC) methods which are widely adopted nowadays, the Satellite Autonomous Integrity Monitoring (SAIM) method can be used to monitor orbit/ephemeris and clock errors, and has advantages in monitoring orbit and clock quality and providing instantaneous responses when faults happen. 相似文献
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