全文获取类型
收费全文 | 572篇 |
免费 | 200篇 |
国内免费 | 68篇 |
专业分类
航空 | 121篇 |
航天技术 | 370篇 |
综合类 | 9篇 |
航天 | 340篇 |
出版年
2024年 | 2篇 |
2023年 | 16篇 |
2022年 | 31篇 |
2021年 | 51篇 |
2020年 | 36篇 |
2019年 | 59篇 |
2018年 | 49篇 |
2017年 | 36篇 |
2016年 | 44篇 |
2015年 | 36篇 |
2014年 | 99篇 |
2013年 | 47篇 |
2012年 | 53篇 |
2011年 | 53篇 |
2010年 | 45篇 |
2009年 | 36篇 |
2008年 | 38篇 |
2007年 | 28篇 |
2006年 | 30篇 |
2005年 | 9篇 |
2004年 | 17篇 |
2003年 | 7篇 |
2002年 | 5篇 |
2001年 | 3篇 |
1999年 | 2篇 |
1998年 | 2篇 |
1997年 | 2篇 |
1995年 | 1篇 |
1994年 | 1篇 |
1986年 | 1篇 |
1981年 | 1篇 |
排序方式: 共有840条查询结果,搜索用时 203 毫秒
91.
92.
93.
94.
美国火星表面探测使命述评(下) 总被引:2,自引:2,他引:2
从1975年8月发射(1976年7月着陆火星)的海盗-1探测器以来,美国已成功执行了6次火星表面探测使命,即海盗-1与海盗-2轨道器/着陆器,"火星探路者"(MPF)着陆器/巡游车,"勇气"与"机遇"火星探测巡游车(MER),以及"凤凰"着陆器;而推迟到2011年发射的火星科学实验室(MSL)将火星着陆技术与表面巡游车技术推向一个新的高度。从"海盗"着陆器到MSL"好奇心"巡游车、美国历经三种火星着陆系统与三代火星表面巡游车技术的发展。三种着陆系统为着陆腿着陆系统("海盗"与"凤凰"),气囊着陆系统(MPF与MER),以及空中吊机着陆系统(MSL)。三代巡游车为MPF"旅居者"巡游车、MER"勇气"与"机遇"巡游车,以及MSL"好奇心"巡游车。现在,美国在火星进入、降落与着陆(EDL)运作与表面避障移动方面,已达到技术成熟与先进的水平,满足安全着陆与表面移动探测的要求。文章阐述美国上述七项火星表面探测使命的立项背景、科学目标与有效载荷、飞行系统组成,以及飞行运作程序;分析美国火星着陆技术与表面巡游车技术的发展。 相似文献
95.
深空辐射环境及其效应的分析与比较 总被引:1,自引:0,他引:1
深空辐射环境对深空探测活动将带来严重的威胁。文章首先对深空辐射环境及效应进行了分析,接着对月球、火星、木星和土星等不同星体的辐射环境及效应进行了详细的探讨及比较。文章得到的结论可为深空探测器的设计和航天员的防护设计提供重要的指导与帮助。 相似文献
96.
97.
从协同化、体系化、一体化适应未来战争的信息化,跨域化、高速化、多用化适应未来战争的立体多维化,自主化、平台化、小型化适应未来战争的无人智能化3个方面概述了未来战略新常态下武器装备对自主导航控制的需求,进而对自主导航控制这一概念进行了简要概述.从精确打击入手,阐述了惯性技术对自主导航的重要性,提出惯性技术是自主导航控制的核心.最后,从惯性器件、惯性传感技术、惯性测试、新功能材料、新兴算法和软件技术等方面分析总结了惯性技术的发展趋势,并对我国惯性技术的发展提出了一些建议. 相似文献
98.
99.
Balázs Zábori Attila Hirn Pál Bencze 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The main point of the paper is to use the simultaneous measurements of the energetic particle flux by TriTel and those of electron density by a Langmuir probe to study the question of to what extent solar electromagnetic and corpuscular radiation (galactic cosmic rays, particle precipitation from the radiation belts) are responsible for the ionization of the atmosphere. The electron density measured by the Langmuir probe is the sum of the ionization produced by the solar electromagnetic radiation and that due to the corpuscular radiation. The ionization produced by the solar electromagnetic radiation may be computed. The flux of energetic particles in an energy range may be determined by taking the difference between the threshold energy of the TriTel telescopes and the energy corresponding to the local cut-off rigidity. As the ESEO satellite will have a quasi-polar and circular orbit, the cut-off rigidity will change from low to high latitudes, thus enabling the assignment of different energy bands for the telescopes. Thus, it will be possible to determine which energy bands of particle produce ionization at different latitudes. 相似文献
100.
M. Nelson W.F. DempsterJ.P. Allen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(5):675-683
Development of reliable and robust strategies for long-term life support for planetary exploration must be built from real-time experimentation to verify and improve system components. Also critical is incorporating a range of viable options to handle potential short-term life system imbalances. This paper revisits some of the conceptual framework for a Mars base prototype which has been developed by the authors along with others previously advanced (“Mars on Earth®”) in the light of three years of experimentation in the Laboratory Biosphere, further investigation of system alternatives and the advent of other innovative engineering and agri-ecosystem approaches. Several experiments with candidate space agriculture crops have demonstrated the higher productivity possible with elevated light levels and improved environmental controls. For example, crops of sweet potatoes exceeded original Mars base prototype projections by an average of 46% (53% for best crop) ultradwarf (Apogee) wheat by 9% (23% for best crop), pinto bean by 13% (31% for best crop). These production levels, although they may be increased with further optimization of lighting regimes, environmental parameters, crop density etc. offer evidence that a soil-based system can be as productive as the hydroponic systems which have dominated space life support scenarios and research. But soil also offers distinct advantages: the capability to be created on the Moon or Mars using in situ space resources, reduces long-term reliance on consumables and imported resources, and more readily recycling and incorporating crew and crop waste products. In addition, a living soil contains a complex microbial ecosystem which helps prevent the buildup of trace gases or compounds, and thus assist with air and water purification. The atmospheric dynamics of these crops were studied in the Laboratory Biosphere adding to the database necessary for managing the mixed stands of crops essential for supplying a nutritionally adequate diet in space. This paper explores some of the challenges of small bioregenerative life support: air-sealing and facility architecture/design, balance of short-term variations of carbon dioxide and oxygen through staggered plantings, options for additional atmospheric buffers and sinks, lighting/energy efficiency engineering, crop and waste product recycling approaches, and human factor considerations in the design and operation of a Mars base. An “Earth to Mars” project, forging the ability to live sustainably in space (as on Earth) requires continued research and testing of these components and integrated subsystems; and developing a step-by-step learning process. 相似文献