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31.
Air route network optimization,one of the essential parts of the airspace planning,is an effective way to optimize airspace resources,increase airspace capacity,and alleviate air traffic con gestion.However,little has been done on the optimization of air route network in the fragmented airspace caused by prohibited,restricted,and dangerous areas (PRDs).In this paper,an air route network optimization model is developed with the total operational cost as the objective function while airspace restriction,air route network capacity,and non-straight-line factors (NSLF) are taken as major constraints.A square grid cellular space,Moore neighbors,a fixed boundary,together with a set of rules for solving the route network optimization model are designed based on cellular automata.The empirical traffic of airports with the largest traffic volume in each of the 9 flight information regions in mainland China is collected as the origin-destination (OD) air port pair demands.Based on traffic patterns,the model generates 35 air routes which successfully avoids 144 PRDs.Compared with the current air route network structure,the number of nodes decreases by 41.67%,while the total length of flight segments and air routes drop by 32.03% and 5.82% respectively.The NSLF decreases by 5.82% with changes in the total length of the air route network.More importantly,the total operational cost of the whole network decreases by 6.22%.The computational results show the potential benefits of the model and the advantage of the algorithm.Optimization of air route network can significantly reduce operational cost while ensuring operation safety. 相似文献
32.
对H5飞机经过了计算、论证、试飞,在此基础上提出了一种既安全又能充分发挥飞机飞行性能,同时又使动作程序化的调油方法--规划调油法。用这种调油就可以大大地减少飞行员操纵飞机进的注意力分散,更利于集中精力操纵飞机,以保证飞行的安全。 相似文献
33.
Neta A. Bahcall 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
The spatial distribution of a complete redshift sample of nearby rich clusters of galaxies is studied. Strong superclustering, extending to very large scales (100h−1Mpc), is observed in the cluster distribution. In particular, we determined and discuss below the following studies:I. The spatial correlation function of rich clusters of galaxies.II. The construction of a complete catalog of superclusters and a study of their growth (percolation).III. The finding of large-scale superclusters surrounding the giant galaxy void in Bootes.IV. The finding of a 300 Mpc void of rich clusters of galaxies.All the above studies provide evidence for the existence of large-scale structure in the universe, and reveal some of its characteristics. These findings are of importance to models of the formation of galaxies and structure in the universe. 相似文献
34.
风扇/增压级带间隙三维粘性流场数值模拟 总被引:8,自引:0,他引:8
使用三维数值模拟软件NUMECA(Numerical Mechanics Application)对双涵道风扇/增压级带转子叶尖间隙的粘性流场进行了三维定常流动数值模拟,获得了其设计转速下的流场特性.结果显示,随着外涵背压的升高,风扇顶部激波后阻塞区周向和轴向尺寸增大,激波变形加剧,继续提高外涵压比,则外涵效率和进出口流量下降.内涵背压的升高,使内涵各转子叶片顶部的泄漏流动影响范围向上游扩散.内涵背压过高,效率和进出口流量同样会有下降的趋势.同时通过和实验结果的比较表明,数值模拟软件模拟的风扇/增压级的三维定常粘性流场能够较真实的反映出转子叶尖间隙泄漏流场的结构特征,以及间隙对流场参数的影响. 相似文献
35.
合理采购并在多个航站之间合理配置航材数量对于民用飞机的经济运行十分重要,而航材预测与配置研究形成的理论算法内容相对复杂。为推动这些算法程序能够有效投入工程应用,基于 Java 语言,并整合Matlab、Python 语言编写的算法程序,开发多语言混合编程的民用飞机航材预测与配置平台。首先,介绍平台中集成的航材预测与配置的支持向量机算法和边际分析算法,并叙述混合编程的实现方式;然后,阐述平台设计的详细内容,并对混合编程的实现方式及不同程序语言间参数类型的转换方法进行说明;最后,运用实际工程数据对平台的功能进行使用测试。结果表明:平台的人机界面友好、操作简便,较好地实现了航材预测与航材配置功能,能够为相关理论算法通过平台技术满足工程需要提供借鉴和思路。 相似文献
36.
37.
目前,企业社会责任运动从西方向全世界扩散和渗透,日益为人们所认可和接受,成为一种国际潮流,对企业自身的可持续发展以及国际贸易的进步都具有重要的意义。在“文化与有效性模型”等相关理论模型的基础上,简析国际企业社会责任运动的新趋势,并重点阐述其对中国企业文化的深刻而具有长远意义的作用,指出在企业、政府、社会的大力支持下,中国企业文化要向与国际企业社会责任运动相融合的方向前进,才具有生命力。 相似文献
38.
研究模型振动对风洞实验结果的影响对于修正风洞实验数据和加深空气动力学的理解具有重要的现实意义。基于κ-ω的SST两方程湍流模型,在时间域求解雷诺平均N—S方程,研究了模型振动在不同迎角下流场和气动力的变化规律。结果表明:模型振动在小迎角条件下对气动力测量结果几乎没有影响,但在大迎角存在一定分离的条件下,可以引起分离涡的非线性演化,导致气动力平均值的改变,从而引起风洞气动力测量值的分散性。结论从物理机理上解释了大迎角风洞实验的重复性和数据分散性。 相似文献
39.
V.B. Baranov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
An interface between the fully ionized hydrogen plasma of the solar wind (SW) and the partially ionized hydrogen gas flow of the local interstellar medium (LISM) is formed as a region where there is a strong interaction between these two flows. The interface is bounded by the solar wind termination shock (TS) and the LISM bow shock (BS) and is separated on two regions by the heliopause (HP) separating the solar wind and charged component of the LISM (plasma component below). The BS is formed due to the deceleration of the supersonic LISM flow relative to the solar system. Regions of the interface between the TS and HP and between the HP and BS were in literature named as the inner and outer heliosheaths, respectively. An investigation of the structure and physical properties of the heliosheath is at present especially interested due to the fact that Voyager-1 and Voyager-2 have crossed the TS in December 2004 (Burlaga, L.F., Ness, N.F., Acuna, M.Y., et al. Crossing the termination shock into the the heliosheath. Magnetic fields. Science 309, 2027–2029, 2005; Fisk, L.A. Journey into the unknown beyond. Science 309, 2016–2017, 2005; Decker, R.B., Krimigis, S.M., Roelof, E.C., et al. Voyager 1 in the foreshock, termination shock and heliosheath. Science 309, 2020–2024, 2005; Stone, E.C., Cummings, A.C., McDonald, F.B., et al. Voyager 1 explores the termination shock region and the heliosheath beyond. Science 309, 2017–2020, 2005) and in September 2007 (Jokipii, J.R. A shock for Voyager 2. Nature 454, 38–39, 2008; Gurnett, D.A., Kurth, W.S. Intense plasma waves at and near the solar wind termination shock. Nature 454, 78–80, 2008. doi: 10.1038/nature07023; Wang, L., Lin, R.P., Larson, D.E., Luhmann, J.G. Domination of heliosheath pressure by shock-accelerated pickup ions from observations of neutral atoms. Nature 454, 81–83, 2008. doi: 10.1038/nature07068.14; Burlaga, L.F., Ness, N.F., Acuna, M.H., et al. Magnetic fields at the solar wind termination shock. Nature 454, 75–77, 2008. doi: 10.1038/nature07029; Richardson, J.D., Kasper, J.C., Wang, C., et al. Cool heliosheath plasma and deceleration of the upstream solar wind at the termination shock. Nature 454, 63–66, 2008. doi: 10.1038/nature07024; Stone, E.C., Cummings, A.C., McDonald, F.B., et al. An asymmetric solar wind termination shock. Nature 454, 71–74, 2008. doi: 10.1038/nature07022; Decker, R.B., Krimigis, S.M., Roelof, E.C., et al. Mediation of the solar wind termination shock by non-thermal ions. Nature 454, 67–70, 2008. doi: 10.1038/nature 07030), respectively, and entered to the inner heliosheath. 相似文献
40.