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Elisa Maria Alessi Gerard Gómez Josep J. Masdemont 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
The purpose of this work is to compute transfer trajectories from a given Low Earth Orbit (LEO) to a nominal Lissajous quasi-periodic orbit either around the point L1 or the point L2 in the Earth–Moon system. This is achieved by adopting the Circular Restricted Three-Body Problem (CR3BP) as force model and applying the tools of Dynamical Systems Theory. 相似文献
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垂直返回重复使用运载火箭技术分析 总被引:3,自引:0,他引:3
结合SpaceX公司近期进行的多次猎鹰火箭一子级垂直着陆返回技术试验,对比分析垂直返回重复使用运载火箭两种返回方式的工程应用价值。首先,建立运载火箭一子级动力返回段弹道设计动力学模型。随后,提出基于H-V飞行剖面分段返回弹道设计方法。然后针对“返回原场”(RTLS)和“不返回原场”(NRTLS)两种垂直返回方式,构建综合考虑上升段与返回段的推进剂耦合作用的一体化弹道优化设计策略。最后,通过数值仿真,对比分析了两种返回方式下的火箭运载能力。结果表明,采用“不返回原场”方式的运载能力损失仅占“返回原场”方式的一半,具有较好的工程应用价值。 相似文献
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Yuan Ren Jinjun Shan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
With the development of lunar exploration, a lunar global positioning system (LGPS) is demanded for both on-ground and in-flight lunar exploration missions. The traditional configuration of constellation requires at least eighteen satellites to cover the whole lunar surface continuously. In this paper, the configurations of the libration point orbits (LPOs) constellations are investigated. By using the constellations on the Earth–Moon L1 and L2 LPOs, the basic functions of the LGPS can be realized by using eight to fourteen satellites. First, the LPO and the combinations of LPOs, which can be used in the constellations of the LGPS, are investigated. The criteria and procedures of the configuration design are introduced. Second, the configurations of LPOs constellations are investigated in the Earth–Moon circular-restricted three-body problem (CR3BP). The size of the LPOs and the distribution of the satellites on these LPOs are determined by using an exhaustive algorithm and a global optimization method, respectively. The key performance parameters of these constellations are computed. Third, the constellations with good performance in the CR3BP are redesigned in the more accurate Earth–Moon based Sun-perturbed bicircular four-body problem (B4BP). Moreover, in order to avoid the ground coverage problem caused by the perturbation of the Sun, some modifications are implemented, and the configuration of the no blind area LGPS in the B4BP is obtained. 相似文献
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Michal Kačmařík Pavla Skřivánková 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
This paper discusses GPS (Global Position System) meteorology. The research presented is based on a comparison of values of precipitable water vapour PWV, based on GPS measurements using final and predicted ephemerides of satellite orbits. We analysed recent year’s improvement in predicting ephemerides. We compared the data outputs from a radiosonde using GPS receiver measurements directly from the meteorological station from which the radiosondes were launched. The results indicate a high quality of the predicted ephemerides. This finding makes predicted ephemerides highly usable for near real-time estimations of PWV. To use PWV in meteorological forecast applications, this high speed of PWV values supply is necessary. 相似文献
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Lawrence D. Huebner R. Marshall Smith John R. Campbell Terry L. Taylor 《Acta Astronautica》2009,65(11-12):1706-1716
The Ares I–X Flight Test Vehicle is the first in a series of flight test vehicles that will take the Ares I Crew Launch Vehicle design from development to operational capability. Ares I–X is scheduled for a 2009 flight date, early enough in the Ares I design and development process so that data obtained from the flight can impact the design of Ares I before its Critical Design Review. Decisions on Ares I–X scope, flight test objectives, and FTV fidelity were made prior to the Ares I systems requirements being baselined. This was necessary in order to achieve a development flight test to impact the Ares I design. Differences between the Ares I–X and the Ares I configurations are artifacts of formulating this experimental project at an early stage and the natural maturation of the Ares I design process. This paper describes the similarities and differences between the Ares I–X Flight Test Vehicle and the Ares I Crew Launch Vehicle. Areas of comparison include the outer mold line geometry, aerosciences, trajectory, structural modes, flight control architecture, separation sequence, and relevant element differences. Most of the outer mold line differences present between Ares I and Ares I–X are minor and will not have a significant effect on overall vehicle performance. The most significant impacts are related to the geometric differences in Orion Crew Exploration Vehicle at the forward end of the stack. These physical differences will cause differences in the flow physics in these areas. Even with these differences, the Ares I–X flight test is poised to meet all five primary objectives and six secondary objectives. Knowledge of what the Ares I–X flight test will provide in similitude to Ares I—as well as what the test will not provide—is important in the continued execution of the Ares I–X mission leading to its flight and the continued design and development of Ares I. 相似文献
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针对火箭控制系统姿态网络设计,提出了一种采用遗传算法和模拟退火算法混合的算法进行姿态网络自动设计的方法。该算法实现了已知校正网络幅频特性曲线的幅频向量,通过系统辨识和寻优搜索,可以计算出该网络的传递函数。本文对该算法进行了试验验证,证明该方法可行并优于单纯的模拟退火算法和遗传算法。 相似文献