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近年来,售后服务模式的变化促进了航空航天业的快速转变. 航空公司和运营商希望从发动机制造商(OEM)得到更多的支持,由此导致两种商业模式产生了更多的一致性,OEM最终想得到的是能与客户长期的合作.除了在设计时提出各种要求,OEM还需要客户在接收了发动机后,继续与之合作以了解用户的需求. 相似文献
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<正>为了节约维修成本、保证飞机的高可用性,低成本航空公司的机队类型简单,且愿意与OEM签署全面的维修协议,将维修的责任转移给OEM。这一方面的确可使其自身集中更多的精力用于航线运营,另一方面也极大地促进OEM在设计阶段就更注重产品的全寿命期使用成本。 相似文献
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航空电子设备的支援方式正在发生变化.航空公司在接收装有最新数字式航电设备的新飞机的同时,还要继续运营一些安装了老的航电设备的飞机.随着新一代航电设备的日益复杂化,OEM(制造商)不愿意提供这些设备的专有数据,减少了航空公司选择非OEM维修的可能性,而OEM在向客户提供全寿命期支援时,也很难满足各航空公司独特的运营需求. 相似文献
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Lee Ann Shay 《航空维修与工程》2019,(7)
<正>2018年,《航空周刊》和AeroD ynamic咨询公司首次联合开展了《对OEM客户服务满意度的调查》,在给OEM的工作带来一定压力的同时,也为OEM在售后服务方面的改进指出了明确的方向,反响很好。今年,这一调查仍在继续并得出了一些不一样的结果,如空客的整体得分较去年有所提高、巴航工业的 相似文献
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<正>随着OEM产能的提升,对零部件供应商的需求越来越大。因此,零部件供应商都在努力扩大产能,不仅致力于现有能力的提升,还在持续寻找新部件生产的商机。随着各大OEM产能的提升, OEM新生产任务对零部件供应市场的需求不断扩大,致使各级部件供应商也纷纷看到了远超过市场增长本身的发展空间。例如,全球知名的反推装置复合材 相似文献
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大约4年前,加拿大航空技术公司(ACTS)与铬合金公司结为战略合作伙伴,在CF34发动机的维修中采用由铬合金公司生产的PMA件,以减少大修成本. 相似文献
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Massive stars are crucial building blocks of galaxies and the universe, as production sites of heavy elements and as stirring agents and energy providers through stellar winds and supernovae. The field of magnetic massive stars has seen tremendous progress in recent years. Different perspectives—ranging from direct field measurements over dynamo theory and stellar evolution to colliding winds and the stellar environment—fruitfully combine into a most interesting and still evolving overall picture, which we attempt to review here. Zeeman signatures leave no doubt that at least some O- and early B-type stars have a surface magnetic field. Indirect evidence, especially non-thermal radio emission from colliding winds, suggests many more. The emerging picture for massive stars shows similarities with results from intermediate mass stars, for which much more data are available. Observations are often compatible with a dipole or low order multi-pole field of about 1 kG (O-stars) or 300 G to 30?kG (Ap/Bp stars). Weak and unordered fields have been detected in the O-star ζ Ori A and in Vega, the first normal A-type star with a magnetic field. Theory offers essentially two explanations for the origin of the observed surface fields: fossil fields, particularly for strong and ordered fields, or different dynamo mechanisms, preferentially for less ordered fields. Numerical simulations yield the first concrete stable (fossil) field configuration, but give contradictory results as to whether dynamo action in the radiative envelope of massive main sequence stars is possible. Internal magnetic fields, which may not even show up at the stellar surface, affect stellar evolution as they lead to a more uniform rotation, with more slowly rotating cores and faster surface rotation. Surface metallicities may become enhanced, thus affecting the mass-loss rates. 相似文献
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崔晨耕 《西安航空技术高等专科学校学报》2010,28(1)
电能质量的电压跌落问题正日益被关注,为此对动态电能质量中电压跌落问题进行研究,分析电压跌落的原因、传播过程及对电力系统的危害,并在此基础上对电压跌落进行了分类,提出了评估指标及应对电压跌落问题的措施。 相似文献
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在今年2月的美国空军峰会空中作战研讨会上,美国空军高层领导人就他们目前面临的经费紧张、F-35项目拖期、机队老龄化以及维修和部队培训等问题发表讲话。其中有造势的成分,也有真实的看法和计划。 相似文献
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Rumi Nakamura 《Space Science Reviews》2006,124(1-4):91-101
Consequences of the solar wind input observed as large scale magnetotail dynamics during substorms are reviewed, highlighting
results from statistical studies as well as global magnetosphere/ionosphere observations. Among the different solar wind input
parameters, the most essential one to initiate reconnection relatively close to the Earth is a southward IMF or a solar wind
dawn-to-dusk electric field. Larger substorms are associated with such reconnection events closer to the Earth and the magnetotail
can accumulate larger amounts of energy before its onset. Yet, how and to what extent the magnetotail configuration before
substorm onset differs for different solar wind driver is still to be understood. A strong solar wind dawn-to-dusk electric
field is, however, only a necessary condition for a strong substorm, but not a sufficient one. That is, there are intervals
when the solar wind input is processed in the magnetotail without the usual substorm cycle, suggesting different modes of
flux transport. Furthermore, recent global observations suggest that the magnetotail response during the substorm expansion
phase can be also controlled by plasma sheet density, which is coupled to the solar wind on larger time-scales than the substorm
cycle. To explain the substorm dynamics it is therefore important to understand the different modes of energy, momentum, and
mass transport within the magnetosphere as a consequence of different types of solar wind-magnetosphere interaction with different
time-scales that control the overall magnetotail configuration, in addition to the internal current sheet instabilities leading
to large scale tail current sheet dissipation. 相似文献
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大手笔的购机行为和传统航空公司纷纷着手设立廉航子公司的现象,使得廉航成为2011年全球航空运输业的热点。通过关注各地区有重要影响并发展稳健的主要廉航,观察其航线的发展现状、规律,以及地区特色,可以更好地掌握全球廉航的发展趋势。 相似文献