排序方式: 共有11条查询结果,搜索用时 187 毫秒
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基于单一产品数据源的BOM管理 总被引:18,自引:2,他引:16
如何管理产品生命周期中的各种物料项清单BOM(Bill of Material)是产 品数据管理的关键,其核心是产品生命周期中BOM的全局数据模型,即BOM之间关系的建立和 维护.借鉴波音公司提出的单一产品数据源SSPD(Single Source of Product Data)思 想,从分析产品生命周期中BOM的演化过程出发,提出了BOM演变原理,并在此基础上,提出 了一种基于SSPD统一管理BOM的框架模型. 相似文献
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飞行器围绕小行星的轨道运动 总被引:1,自引:0,他引:1
分析了飞行器围绕小行星轨道运动的特点,介绍了所建立的表述这一问题的理论基础。采用三种不同方法从几个侧面揭示了这一问题的本质特征。给出了所完成的研究这一问题的进展、结果和相互联系,其中包括轨道摄动、共振运动和周期轨道运动。这一问题的核心和难点是轨道的稳定性问题。 相似文献
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S. M. Giuliatti Winter O. C. Winter 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,33(12):2298-2302
The system formed by the F ring and two close satellites, Prometheus and Pandora, has been analysed since the time that Voyager visited the planet Saturn. During the ring plane crossing in 1995 the satellites were found in different positions as predicted by the Voyager data. Besides the mutual effects of Prometheus and Pandora, they are also disturbed by a massive F ring. Showalter et al. [Icarus 100 (1992) 394] proposed that, the core of the ring has a mass which corresponds to a moonlet varying in size from 15 to 70 km in radius which can prevent the ring from spreading due to dissipative forces, such as Poynting–Robertson drag and collisions. We have divided this work into two parts. Firstly we analysed the secular interactions between Prometheus–Pandora and a massive F ring using the secular theory. Our results show the variation in eccentricity and inclination of the satellites and the F ring taking into account a massive ring corresponding to a moonlet of different sizes. There is also a population of dust particles in the ring in the company of moonlets at different sizes [Icarus 109 (1997) 304]. We also analysed the behaviour of these particles under the effects of the Poynting–Robertson drag and radiation pressure. Our results show that the time scale proposed for a dust particle to leave the ring is much shorter than predicted before even in the presence of a coorbital moonlet. This result does not agree with the confinement model proposed by Dermott et al. [Nature 284 (1980) 309]. In 2004, Cassini mission will perform repeated observations of the whole system, including observations of the satellites and the F ring environment. These data will help us to better understand this system. 相似文献
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Tai-Yin Huang Michael Hickey 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(9):1478-1487
Secular variations of OH airglow (8,3) band and of the intensity-weighted temperature induced by a gravity wave packet at three latitudes in the northern hemisphere in the Mesosphere/Lower Thermosphere region are investigated using a 2-D, time-dependent, fully nonlinear OH chemistry–dynamics model. A net-cycled average survives due to wave transience and dissipation. The integrated OH (8,3) volume emission rates show a 20 percent increase induced by the wave packet. The corresponding intensity-weighted temperature shows an initial increase up to 2 percent then a gradual decrease for the remainder of the simulation time by the same wave packet. These secular variations could be mistaken as long-period or short-period waves in the airglow observations. Therefore, care must be taken when analyzing the data from observations. 相似文献
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用Hamilton方法研究地球自转的长期减慢 总被引:1,自引:0,他引:1
本文用Hamilton方法研究了弹性地球在日月引潮力势作用下产生形变后对地球自转速率的影响,考虑了潮汐形变的相位延迟,选择地球模型PREM参数进行了计算,理论上求得地球自转长期减慢值为-5.711×10(-22)rad/s2,与观测结果符合很好.结果表明,对地球自转长期减慢起主要影响是扇谐潮,由月亮引潮力势产生的影响远比太阳重要. 相似文献
旋转孔与腔组成的孔腔系统为航空发动机空气系统的重要组成部分,其瞬态响应过程可能诱发短时危险过渡态载荷。为研究旋转孔腔的瞬态演化规律,以旋转孔前的容腔为研究重点,建立了带旋转孔的容腔CFD计算模型,分析了孔腔系统的瞬态演化过程,并基于旋转孔的稳态流动特性建立了带旋转孔容腔的瞬态1-D模型,对瞬态演化过程进行了仿真。通过对比瞬态1-D模型的结果和CFD结果,发现采用前者能基本模拟容腔的瞬态演化过程,基本满足工程需要,并完成了瞬态1-D模型结果产生偏差的原因分析。 相似文献
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在轨编目物体数目与日俱增,为保证载人航天任务的顺利完成,必须对可能威胁任务轨道的空间目标进行碰撞检测。本文分析了美国航天司令部开发的SGP4近地轨道预报模型,引入其中的摄动力长期项公式。通过模型比对可知,引入摄动力长期项的计算结果与解析法SGP4结果接近,而且摄动力的长期项对轨道根数的影响可以表示为关于时间的函数,结合天球投影可以迅速找出2个物体分别过轨道交线的时间,因此该方法能够保证碰撞预警的精度与速度。仿真结果验证了该方法的快速有效性。 相似文献
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Michael Ovchinnikov Georgi V. Smirnov Irina Zaramenskikh 《Acta Astronautica》2009,65(11-12):1826-1830
This paper examines the possibility of regular orbital corrections for a satellite controlled by an impulsive force applied along the induction vector of the local geomagnetic field. The main purpose of the correcting considered in the paper is to eliminate the drift in secular variation of the relative orbital parameters over the orbital period. The obtained results are applied to the formation flying problem. The developed method is tested using numerical simulation. 相似文献