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1.
Steven D. Howe 《Space Policy》2001,17(4):275-283
The potential benefits to humankind of space exploration are tremendous. Space is not only the final frontier but is also the next marketplace. The orbital space above Earth offers tremendous opportunities for both strategic assets and commercial development. The critical obstacle retarding the use of the space around the Earth is the lack of low cost access to orbit. Further out, the next giant leap for mankind will be the human exploration of Mars. Almost certainly within the next 30 years, a human crew will brave the isolation, the radiation, and the lack of gravity to walk on and explore the Red planet. Both of these missions will change the outlook and perspective of every human being on the planet. However, these missions are expensive and extremely difficult. Chemical propulsion has demonstrated an inability to achieve orbit cheaply and is a very high-risk option to accomplish the Mars mission. An alternative solution is to develop a high performance propulsion system. Nuclear propulsion has the potential to be such a system. The question will be whether humanity is willing to take on the challenge. 相似文献
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The Cluster mission of the European Space Agency (ESA) will allow, for the first time three-dimensional measurements in key regions of the Earth's magnetosphere to be carried out. The European Numerical Simulation Network (ENSN) aims at providing a theoretical support to the mission. We describe the achievements of the ENSN during its first period of activity 1991–1994, during which the network was funded by the European Union. In particular, the ENSN has set up (i) thematic Working Groups on the prime scientific goals of the mission, (ii) a code development Working Group to develop numerical simulation codes specifically adapted to studying magnetospheric boundaries and the corresponding scale mixing, and (iii) software models of Cluster instruments to test in a numerical simulation what the set of four instruments will measure. 相似文献
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D. Koschny V. Dhiri K. Wirth J. Zender R. Solaz R. Hoofs R. Laureijs T.-M Ho B. Davidsson G. Schwehm 《Space Science Reviews》2007,128(1-4):167-188
ESA’s Rosetta mission was launched in March 2004 and is on its way to comet 67P/Churyumov-Gerasimenko, where it is scheduled
to arrive in summer 2014. It comprises a payload of 12 scientific instruments and a Lander. All instruments are provided by
Principal Investigators, which are responsible for their operations.
As for most ESA science missions, the ground segment of the mission consists of a Mission Operations Centre (MOC) and a Science
Operations Centre (SOC). While the MOC is responsible for all spacecraft-related aspects and the final uplink of all command
timelines to the spacecraft, the scientific operations of the instruments and the collection of the data and ingestion into
the Planetary Science Archive are coordinated by the SOC. This paper focuses on the tasks of the SOC and in particular on
the methodology and constraints to convert the scientific goals of the Rosetta mission to operational timelines. 相似文献
4.
音频、视频及静态图像通信 (简称 A/ V/ SI)是空间任务 (包括无人的及载人的航天任务 )中的重要业务。对 CCSDS关于 A/ V/ SI通信业务建议进行了分析研究 ,指出 CCSDS建议的音频、视频及静态图像的质量标准、编码方法和编码参数等与 ITU - T的有关建议是相互兼容的 ,对CCSDS的 A/ V/ SI通信建议在空间任务中的应用提出了初步看法 相似文献
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基于地外天体起飞的真空羽流导流技术仿真与试验研究 总被引:1,自引:0,他引:1
针对着航天器发动机羽流导流问题,基于工程经验提出了四种典型导流装置型面(包含内凹槽形式和导流锥形式等),利用计算流体动力学/直接模拟蒙特卡罗(CFD/DSMC)耦合方法,对起飞过程中羽流导流带来的气动力和气动热效应进行了数值模拟,并对不同导流装置情况下羽流场激波、航天器表面压强和热流密度分布规律进行了分析,给出了四种导流装置的导流效果评价。最后以导流锥形式开展试验,对仿真算法进行了验证。结果表明:羽流导流并没有导致发动机燃烧不稳定;综合考虑航天器羽流和发动机安全性,大导流锥导流的方案最优;在导流锥附近的激波位置及形态和仿真一致,仿真与试验的变化趋势一致,仿真算法可信,数据规律可以作为工程参考。 相似文献
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I. Antonenko G.R. Osinski M. Battler M. Beauchamp L. Cupelli A. Chanou R. Francis M.M. Mader C. Marion E. McCullough A.E. Pickersgill L.J. Preston B. Shankar T. Unrau D. Veillette 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
Remote robotic data provides different information than that obtained from immersion in the field. This significantly affects the geological situational awareness experienced by members of a mission control science team. In order to optimize science return from planetary robotic missions, these limitations must be understood and their effects mitigated to fully leverage the field experience of scientists at mission control. 相似文献