基于学习的并行免疫量子进化算法

提出了基于学习的多宇宙并行免疫量子进化算法,算法中将种群分成若干个独立的子群体,称为宇宙。并给出了多宇宙的并行拓扑结构,其中各宇宙独立演化．宇宙内采用免疫量子进化算法,宇宙间采用基于学习机制的移民、模拟量子纠缠的种群交叉等信息交互方式．使得进化算法具有更好的种群多样性,更快的收敛速度和全局寻优能力。仿真实验结果表明该算法比串行的免疫量子进化算法运算效率更高。     

爆炸解体空间碎片的空间密度分布

利用NASA爆炸解体模型研究了由爆炸解体而产生的空间碎片的分布情况,并通过对大种群空间碎片进行快速轨道演化,获得了所有历史上爆炸解体而产生的空间碎片在当前时刻的分布情况,为建立空间碎片环境工程模型提供了一部分参考数据。文中对后续的研究工作具有一定的参考价值。     

高职院校教师教学能力演变规律与突破机制研究

"三教"是今后高职院校教育教学重点关注的领域,尤其是教师的教学能力提升方面,不仅关系到人才培养质量,更成为高职教育改革亟需突破的重点.以高职院校教师教学能力大赛政策为例,挖掘教师能力演变规律,探索教学突破机制,并提出团队配置精细化、教学设计精致化、课堂授课精品化及课程问题解决精益化等建议.     

一种面向运载火箭自动对接的三维测量场构建方法

旋转激光自动经纬仪系统(R-LATs)是一种基于前方角度交汇的分布式大尺寸测量系统。各激光扫描基站的布局位置直接影响着测量区域内的测量精度和应用性能。从测量区域的测量不确定度量化着手,利用蒙特卡罗法获取各点的测量不确定度,以测量区域的最大不确定度作为主要优化目标,利用差分进化算法自动寻优,更简单有效地实现了面向运载火箭自动对接的R-LATs系统布站优化。最后进行了运载火箭对接测量场的实际应用验证。应用结果表明:该方法能有效优化激光扫描基站布局,提高系统测量精度,满足实际应用需求。     

A plastic strain energy method exploration between machined surface integrity evolution and torsion fatigue behaviour of low alloy steel

To explore the evolution mechanism of multistage machining processes and torsional fatigue behaviour based on strain energy for the first time and provide process optimization of axis parts of low alloy steel for service performance, four multistage machining processes were applied to the 45Cr Ni Mo VA steel, including the Rough Turning process(RT), RT+ the Finish Turning process(FRT), FRT+ the Grinding process(GFRT) and RT+ the Finish Turning process on dry cutting condition(FRT0). The result s...     

Observations of the atmospheres and winds of O-stars,LBVs and Wolf-Rayet stars

This review summarises recent studies of O-stars, Luminous Blue Variables (LBVs) and Wolf-Rayet (WR) stars, emphasising observations and analyses of their atmospheres and stellar winds yielding determinations of their physical and chemical properties. Studies of these stellar groups provide important tests of both stellar wind theory and stellar evolution models incorporating mass-loss effects. Quantitative analyses of O-star spectra reveal enhanced helium abundances in Of and many luminous O-supergiants, together with CNO anomalies in OBN and Ofpe/WN9 stars, indicative of evolved objects. Enhanced helium, and CNO-cycle products are observed in several LBVs, implying a highly evolved status, whilst for the WR stars there is strong evidence for the exposition of CNO-cycle products in WN stars, and helium-burning products in WC and WO stars. The observed wind properties and mass-loss rates derived for O-stars show, in general terms, good agreement with predictions from the latest radiation-driven wind models, although some discrepancies are apparent. Several LBVs show similar mass-loss rates at maximum and minimum states, contrary to previous expectations, with the mechanism responsible for the variability and outbursts remaining unclear. WR stars exhibit the most extreme levels of mass-loss and stellar wind momenta. Whilst alternative mass-loss mechanisms have been proposed, recent calculations indicate that radiation pressure alone may be sufficient, given the strong ionization stratification present in their winds.     

The massive star distribution in the Galaxy and the Magellanic Clouds

The numbers and distribution of Population I O-type stars and Wolf-Rayet stars are reviewed. The numbers of known WR stars in the Galaxy, the LMC and the SMC are 185, 114, and 9, respectively. Distances and galactic distributions determined by various authors are compared. The single star and binary distributions are discussed in the light of evolutionary studies.     

A spectroscopic analysis of B stars in the SMC cluster NGC 330

Medium resolution (2A/px) but high s/n spectra of approximately twenty of the brightest blue stars in the young open cluster NGC 330 in the SMC have been analyzed in order to determine their atmospheric parameters and the evolutionary status. Stellar parameters are determined by comparison with LTE and NLTE model atmosphere calculations and an HR diagram constructed. Luminosities of the sample stars lie in the range 4.0L _*/L )<5.0 and spectral types between O9 and late-B. The stars in our sample appear to define 4 groups: main-sequence B-stars (B2-B4), B-supergiants (B4) in a blue-loop phase of evolution, a small number of blue stragglers (O9-B0 near main-sequence stars) and a group of luminous giants (B1-B2) which reside in the so-called post main-sequence gap of the HR diagram. Furthermore, we have confirmed spectroscopically the very high incidence of Be stars in this cluster. Finally the almost complete absence of metal lines (at this resolution) is in keeping with the expected very low metallicity of the SMC.     

基于适当控制翼型演化历程的气动设计方法

本文提出一种翼型设计的新方法,它基于适当控制翼型演化历程,采用求解非定常流动控制方程的方法,实现了翼型反问题的高效求解.同时在笛卡尔坐标系中应用Level-Set函数,避免了贴体动网格的采用,从而大大减少了所需计算工作量.