排序方式: 共有23条查询结果,搜索用时 0 毫秒
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The design of interplanetary trajectories based on patched circular restricted three body models is gradually becoming a valuable alternative to the classical patched conic approach. The main advantage offered by such a model is the possibility to exploit the manifold dynamics to move naturally far from or toward a body. Generally, propulsive maneuvers are required to match these structures. Low-thrust arcs offer the possibility to have a significant propellant mass reduction when moving from manifold to manifold. The aim of this paper is to present a methodology to design low-thrust trajectories between two planetary orbits connecting the manifolds of two circular three body systems. The approach is based on a grid search on the main parameters governing the solution to identify those trajectories moving within the manifold images on given Poincarè sections. The value of the Jacoby constant of the target libration point periodic orbit is chosen as stop condition for the thrusting phases. Ballistic arcs follow up to the proper Poincarè section intersection. A grid search for an Earth to Venus transfer is presented as test case. 相似文献
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介绍江西国防科技工业单位的三级计量技术机构进行国防计量认可复查的情况 ,指出了存在的问题 ,并对问题的解决提出了建议 相似文献
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空间目标编目测量资源调度是一个复杂的系统问题。首先对测量资源调度要素进行分析,然后在对调度需求分解的基础上,给出一个基于CSP(约束满足问题)模型的随机搜索编目调度算法。该算法在目标数量多、任务数据量大、复杂度高的任务环境下,求解快速、稳定。最后对调度软件实现中的核心问题——数据结构组织方式进行了阐述,基于合理的数据结构,调度算法得以高效实现。 相似文献
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从解算弹道的逐点多站最小二乘算法得到的弹道精度出发,给出了一个全测速多站系统的最优布站数学模型,并通过大量试算选定了具有良好收敛性的数值算法.初步的计算表明:对全测速多站系统,其最优布站方案与现有布站方案在弹道精度上有着显著的差别;在最优布站方案下可确保逐点多站最小二乘算法具有良好的数值稳定性,并得到满足精度要求的外测弹道. 相似文献
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对中国高模量碳纤维应用中工艺性能问题的分析 总被引:2,自引:0,他引:2
文章简述了航天器结构对高模量碳纤维需求,对中国高模量碳纤维品质稳定性、工艺稳定性等内容进行了简要评述,着重对中国高模量碳纤维工艺性能做了分析,并对加强中国高模量碳纤维批生产提出了建议. 相似文献
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介绍HBM-3000型门式布氏硬度计的电器控制系统的电器原理及手动与自动操作程序以及在调整与修理过程中发现的问题和解决的方法 相似文献
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Pini Gurfil Sofia Belyanin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,42(8):1313-1317
The Gyldén–Meshcherskii Problem (GMP) extends the classical two-body problem of Newton and Kepler by considering time-varying gravitating masses, an important extension of the two-body problem for modeling cometary motion and cosmological phenomena. In this paper, we consider the GMP in a specialized setup, the setup of gauge theory. We show that the variational equations, modeling the effect of the mass time variation on the orbital elements, can be derived by fixing a gauge of a particular form that is different from the Lagrange gauge. Thus, the orbital elements modeling the effect of a time-varying secondary mass are non-osculating. This implies that the trajectory of a celestial body whose mass is continuously changing cannot be approximated by a series of Keplerian orbits. Finally, we provide the first-order averaged equations written in terms of non-osculating elements. 相似文献
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