共查询到20条相似文献,搜索用时 46 毫秒
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本文总结了英国希斯罗机场发展综合交通枢纽的经验,并在此基础上探讨了枢纽功能发挥与场站选址和衔接网络等技术属性之间的关系和一般性规律,以期对我国综合交通枢纽的建设发展提供有益借鉴。伦敦共有5个机场,希斯罗机场、盖特威克机场、斯坦斯特德机场、伦敦城市机场和卢顿机场。希斯罗机场提供洲际、欧洲、国内航班服务,其他4个机场主要提供国内和欧洲航班服务。希斯罗机场2010年旅客吞吐量达到6500万人,货运量达147万吨,是英国乃至欧洲最重要的机场。 相似文献
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在知识经济快速发展和经济全球化的背景下,国内外的大型机场地区及其进场交通沿线地区已经成为城市空间发展的主要区域之一。以由轨道交通为主体的综合进场交通走廊为增长轴,以机场综合交通枢纽为增长极的开发模式也将成为一种新兴的城市综合开发模式。 相似文献
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近年来,高铁等轨道交通迅猛发展,对传统航空运输造成冲击,同时带来了航空枢纽发展理念的革新。机场的功能已经由单纯为航空运输提供服务的终端逐步转变为航空运输与轨道交通、公路运输等方式一体化的综合交通枢纽。这是世界大型枢纽机场发展的潮流,同样也是白云机场航空枢纽建设发展的方向。 相似文献
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以济宁曲阜机场为例,结合菏泽机场规划,说明了济宁曲阜机场存在机场位置与旅游景区位置发生偏离、对济宁城市空间扩展引导不足、限制菏泽机场规划、影响济宁综合交通枢纽建设以及机场容量无法满足旅客量增长等问题,这些问题具有一定的普遍意义,希望能促进规划和决策者对军民合用这一机场建设方式采取更为谨慎的态度. 相似文献
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对我国支线机场建设与发展的思考 总被引:1,自引:0,他引:1
机场作为航空运输和城市的重要基础设施,是综合交通运输体系的重要组成部分。经过几十年的建设和发展,我国机场总量初具规模,机场密度逐渐加大,机场服务能力逐步提高,现代化程度不断增强,为保证我国航空运输持续快速、健康协调发展,以及完善国家综合交通体系发挥了重要作用。但是,在不断加快机场建设速度的同时,机场体系结构和功能定位不尽合理, 相似文献
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我国正在加快推进综合交通运输体系建设,在此过程中,民航的发展将呈现新的趋势。未来,低成本航空将成为顺应综合运输体系构建的必然选择,传统航空枢纽将向综合交通枢纽转变,航空货运将与快递业融合发展,民航规划也将与其他交通规划形成互动体系。 相似文献
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介绍了半实物仿真中三轴转台的设备参数修正方法,根据此结果对影响转台精度的频率特性进行测试,并从理论上给出转台框架误差的分析结果。 相似文献
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介绍了美国波音公司实施精益企业的历史、所取得的成绩及今后的发展,论述了精益原理、精益生产系统的组成要素及其实施. 相似文献
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Paola Testa 《Space Science Reviews》2010,157(1-4):37-55
Studies of element abundances in stars are of fundamental interest for their impact in a wide astrophysical context, from our understanding of galactic chemistry and its evolution, to their effect on models of stellar interiors, to the influence of the composition of material in young stellar environments on the planet formation process. We review recent results of studies of abundance properties of X-ray emitting plasmas in stars, ranging from the corona of the Sun and other solar-like stars, to pre-main sequence low-mass stars, and to early-type stars. We discuss the status of our understanding of abundance patterns in stellar X-ray plasmas, and recent advances made possible by accurate diagnostics now accessible thanks to the high resolution X-ray spectroscopy with Chandra and XMM-Newton. 相似文献
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中国公务机市场风生水起3月28日,空中客车公司在京召开"空中客车公务机中国媒体说明会",空客公务及私人航空部副总裁Francois Chazelle出席。时隔仅两天,波音公务机公司总裁 相似文献
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Eva K. Grebel WM James Roberts Jean-Marie Will Klaas S. De Boer 《Space Science Reviews》1993,66(1-4):65-68
A substantial fraction (typically 10%) of Galactic B stars consists of Be stars. While Galactic Be stars have been fairly well investigated, very little is known about the Be star content of the Magellanic Clouds (MCs). We present a refined method of Be star identification by CCD photometry and apply it to four young clusters and associations in the MCs. We find NGC 330 in the SMC to be exceptionally rich in Be stars, while the fraction is clearly lower in the similarly aged LMC clusters NGC 2004 and NGC 1818. NGC 2044, a very young region in the LMC, contains almost no Be stars. Among very early-type B stars in the investigated MC clusters we find the largest number of Be stars, while in the Milky Way this is shifted to somewhat later types. In the LMC, there may be a second frequency peak around B6.Based on observations obtained at the 2.2m MPIA telescope at ESO, La Silla, Chile, partly on time granted by the MPIA, Heidelberg. 相似文献
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Yoji Kondo 《Space Science Reviews》1989,50(1-2):79-84
Recent satellite observations of close binary systems show that practically all binaries exhibit evidence of mass flow and that, where the observations are sufficiently detailed, a fraction of the matter flowing out of the mass-losing component is accreted by the companion and the remainder is lost from the binary system. The mass flow is not conservative. During the phase of dynamic mass flow, the companion star becomes immersed in optically-thick plasma and the physical properties of that star elude close scrutiny. 相似文献
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Yoji Kondo 《Space Science Reviews》1989,49(3-4):79-84
Recent satellite observations of close binary systems show that practically all binaries exhibit evidence of mass flow and that, where the observations are sufficiently detailed, a fraction of the matter flowing out of the mass-losing component is accreted by the companion and the remainder is lost from the binary system. The mass flow is not conservative. During the phase of dynamic mass flow, the companion star becomes immersed in optically-thick plasma and the physical properties of that star elude close scrutiny. 相似文献