排序方式: 共有165条查询结果,搜索用时 250 毫秒
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目前大多数卫星的监视和控制需要使用复杂的地面站,并驻有技术高超的操作手。卫星操作手必须能快速识别和诊断异常情况。许多情况下,不能完成此任务就会丢失重要信息,不能完成任务,极端情况是卫星损坏。许多负责操作卫星的政府和商业机构都面临削减预算,故要寻求用更少、技术水平较低的人员来操作卫星。这些机构寻找各种人工智能(AI)技术作为减少卫星地面控制设施人力以及技术水平的措施。至今将指出这种技术的不足,介绍利 相似文献
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伽利略系统的当前频率和信号设计方案 总被引:3,自引:0,他引:3
本文简要介绍伽利略系统最新提出的频率和信号设计方案,涉及方案设计基本要求、频率和信号基本方案、各种导航信号的调制体制、所用扩频测距伪码、性能参数、时间与坐标参考系等。 相似文献
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Tarter JC Backus PR Mancinelli RL Aurnou JM Backman DE Basri GS Boss AP Clarke A Deming D Doyle LR Feigelson ED Freund F Grinspoon DH Haberle RM Hauck SA Heath MJ Henry TJ Hollingsworth JL Joshi MM Kilston S Liu MC Meikle E Reid IN Rothschild LJ Scalo J Segura A Tang CM Tiedje JM Turnbull MC Walkowicz LM Weber AL Young RE 《Astrobiology》2007,7(1):30-65
Stable, hydrogen-burning, M dwarf stars make up about 75% of all stars in the Galaxy. They are extremely long-lived, and because they are much smaller in mass than the Sun (between 0.5 and 0.08 M(Sun)), their temperature and stellar luminosity are low and peaked in the red. We have re-examined what is known at present about the potential for a terrestrial planet forming within, or migrating into, the classic liquid-surface-water habitable zone close to an M dwarf star. Observations of protoplanetary disks suggest that planet-building materials are common around M dwarfs, but N-body simulations differ in their estimations of the likelihood of potentially habitable, wet planets that reside within their habitable zones, which are only about one-fifth to 1/50th of the width of that for a G star. Particularly in light of the claimed detection of the planets with masses as small as 5.5 and 7.5 M(Earth) orbiting M stars, there seems no reason to exclude the possibility of terrestrial planets. Tidally locked synchronous rotation within the narrow habitable zone does not necessarily lead to atmospheric collapse, and active stellar flaring may not be as much of an evolutionarily disadvantageous factor as has previously been supposed. We conclude that M dwarf stars may indeed be viable hosts for planets on which the origin and evolution of life can occur. A number of planetary processes such as cessation of geothermal activity or thermal and nonthermal atmospheric loss processes may limit the duration of planetary habitability to periods far shorter than the extreme lifetime of the M dwarf star. Nevertheless, it makes sense to include M dwarf stars in programs that seek to find habitable worlds and evidence of life. This paper presents the summary conclusions of an interdisciplinary workshop (http://mstars.seti.org) sponsored by the NASA Astrobiology Institute and convened at the SETI Institute. 相似文献
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本文简要介绍产生CCSDS的背景,其组织机构和研究成果,随后阐述制订和贯彻CCSDS的必要性和可能带来的不利影响。最后附带提一下CCSDS建议与IRIG标准的差异。已批准和正在制订的建议很多,本文不作具体介绍,请参阅随后几篇译文,由此可见一斑。 相似文献
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1988年,美国陆军工程部正式开始研究利用GPS载波相位的实时定位系统。该项研究的最终目标是在1993年做成一台实用样机,能实时获得厘米级的三维定位精度。这一目标实现了,1993年3月开始对样机进行测试。1993年8月进行了首次演示,10月进行了首次公开演示。该设备一般能在“动中”(OTF)15秒时间内分辨模糊整周数,不需要作静态初始化。任一相距20km左右的移动平台可利用该设备进行可靠而稳健的精密定位。在各种工作条件下作了试验,以评价动平台精密定位OTF解模糊的极限。本文总结了这些试验的结果。早期所作的实时试验证明三维方向的定位精度可达1—3cm。本文还介绍了最终实时系统的设计方案以及与水文监测平台的结合问题。 相似文献
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NASA下一世纪科学探索方式将基于廉价频繁的卫星发射,这些卫星将是轻型、低成本、高度自主的小卫星。通过“新世纪计划”(NMP),NASA准备创建一种新的高度综合的方法,对实现这些卫星目标的一系列技术进行开发和空间验证。要满足这些想象的任务要求,并突出降低寿命期成本的目标,对卫星设计、制造和操作各方面将提出挑战。本文集中讨论先进通信系统的体系结构和技术,这些都是NMP已明确的关键性能需求,也是空间验证计划当前选定的内容。这些系统主要分三大类:小型深空通信,极高码速率近地通信和短程通信。其应用包括:空—地链路,行星间飞行器及其着陆器和漫游年之间数据中继的航天器间链路,以及通过星间交叉链路和数据中继卫星的近地卫星通信。本文将从用途和关键性能参数(如质量、体积、效率和成本)来讨论射频(400MHz-32GHz)和光通信技术。 相似文献
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