全文获取类型
收费全文 | 1736篇 |
免费 | 351篇 |
国内免费 | 310篇 |
专业分类
航空 | 1394篇 |
航天技术 | 453篇 |
综合类 | 181篇 |
航天 | 369篇 |
出版年
2024年 | 2篇 |
2023年 | 27篇 |
2022年 | 58篇 |
2021年 | 76篇 |
2020年 | 88篇 |
2019年 | 100篇 |
2018年 | 105篇 |
2017年 | 96篇 |
2016年 | 82篇 |
2015年 | 77篇 |
2014年 | 110篇 |
2013年 | 108篇 |
2012年 | 137篇 |
2011年 | 128篇 |
2010年 | 150篇 |
2009年 | 150篇 |
2008年 | 117篇 |
2007年 | 132篇 |
2006年 | 95篇 |
2005年 | 73篇 |
2004年 | 61篇 |
2003年 | 44篇 |
2002年 | 54篇 |
2001年 | 35篇 |
2000年 | 44篇 |
1999年 | 35篇 |
1998年 | 32篇 |
1997年 | 27篇 |
1996年 | 24篇 |
1995年 | 26篇 |
1994年 | 19篇 |
1993年 | 14篇 |
1992年 | 23篇 |
1991年 | 8篇 |
1990年 | 14篇 |
1989年 | 11篇 |
1988年 | 9篇 |
1987年 | 3篇 |
1984年 | 3篇 |
排序方式: 共有2397条查询结果,搜索用时 312 毫秒
981.
982.
Bernard M. Rabin Kirsty L. Carrihill-Knoll Barbara Shukitt-Hale 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
On exploratory class missions astronauts will be exposed to a variety of heavy particles (HZE particles) which differ in terms of particle energy and particle linear energy transfer. The present experiments were designed to evaluate how these physical characteristics of different particles affect cognitive performance, specifically operant responding. Following exposure to 28Si, 48Ti, 12C and 16O particles at the NASA Space Radiation Laboratory rats were tested for their ability to respond appropriately to changes in reinforcement schedules using an operant task. The results showed that the effectiveness of different particles in disrupting cognitive performance, defined as the lowest dose that produced a performance decrement, varied as a function of the energy of the specific particle: for comparisons between different energies of the same particle (e.g., 56Fe) the effectiveness of the particle was directly proportional to particle linear energy transfer, whereas for comparisons between different particles (e.g., 56Fe and 16O) effectiveness was inversely proportional to particle linear energy transfer. The results are discussed in terms of the mechanisms that influence the effectiveness of different particles and energies and in terms of their implications for analyzing the possible risks to astronauts of decrements in cognitive performance following exposure to HZE particles on long-duration exploratory class missions. 相似文献
983.
984.
采用压敏漆(PSP)测量技术研究了尾迹对涡轮动叶气膜冷却效率的影响,测试叶片带有11排圆柱形气膜孔。获得了不同质量流量比和尾迹斯特劳哈尔数(Sr=0,0.12,0.36)条件下全表面气膜冷却效率分布的试验数据,结果表明:随着尾迹Sr数的增加,叶片前缘区域径向平均气膜冷却效率最大降低幅度达36.5%,吸力面径向平均气膜冷却效率最大降低幅度达53.5%,压力面径向平均气膜冷却效率最大降低幅度达24.2%;尾迹对前缘和吸力面气膜冷却效率的影响大于压力面;随着质量流量比增加,尾迹的影响减小;在进行涡轮动叶表面气膜冷却结构设计时,不考虑尾迹效应会增加设计风险。 相似文献
985.
O. Grigoryan K. Kudela H. Rothkaehl V. Sheveleva 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(1):81-85
We continue to analyze the distribution of electron fluxes with energy 30–500 keV under the radiation belts at low and middle latitudes (L = 1.2–1.9) using experimental data obtained onboard ACTIVE satellite. Special attention is given to altitudinal distribution of electron fluxes and detailed analysis of these electron formations. We observe three main regions of electron flux registration that seem to exist constantly under the radiation belts. These regions are: magneto-conjugated to SAA region (in the north hemisphere), local zone of low intense electron flux accumulation to the west of SAA, and extensive region in the north hemisphere to the east. The analysis of experimental data obtained from ACTIVE satellite (orbit height 500–2500 km) shows that electron fluxes are registered in the wide altitude range up to 1100 km. It is shown that these formations have complicated initial structure with two regions of flux maximums: at L = 1.3 and L = 1.6–1.8. We compare particle data with low frequency (LF) data (ARIEL-4 satellite) and high frequency (HF) data (CORONAS-I satellite). Also we discuss the possible mechanisms of the appearance of these formations under the radiation belts. 相似文献
986.
传递对准姿态匹配的优化算法 总被引:1,自引:0,他引:1
推导了4种传递对准姿态匹配算法,分析了这4种姿态匹配算法的优缺点,证明并验证了其中的“最优姿态匹配法”在姿态匹配算法中的最优性。首先介绍了传统的“姿态角匹配法”及其改进算法,即“姿态矩阵匹配法”,接着引入了量测失准角的概念,经过理论推导,提出了利用量测失准角进行传递对准姿态匹配的“量测失准角匹配法”。上述3种姿态匹配算法都是在子惯导安装角是小量的条件下推导而获得的,只能适用于安装角是小量的条件,具有一定的局限性。基于此,对“量测失准角匹配法”进行了完善,推导出了一种可在多挂点下使用的现代姿态匹配算法——最优姿态匹配法。从理论上证明了4种姿态匹配算法的相互关系。最后,采用“速度+姿态”匹配方案进行的传递对准仿真结果表明:4种姿态匹配算法具有相同的估计精度;推导的“最优姿态匹配法”在保证精度的同时,可应用于子惯导安装角是任意角度的情况,具有更广的应用范围。 相似文献
987.
988.
外商投资企业通常通过转让定价进行避税,转让定价问题不能仅从名义税负的高低来思考,一切影响企业成本和收益的因素都可以引起外商投资企业做出理性的转让定价避税方式和方向选择。通过对珠海市外商投资企业纳税能力和税收流失规模的评估,认为应从完善外部环境和转让定价的调整及稽查方面入手提高转让定价避税的成本,解决外资企业税收流失问题。 相似文献
989.
M.A. Abdu C.G.M. BrumI.S. Batista J.H.A. SobralE.R. de Paula J.R. Souza 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
The F layer critical frequency (foF2) as measured by Digisondes in the equatorial and low latitude locations in Brazil is analyzed to investigate the seasonal and solar flux controls of the intensity of the equatorial ionization anomaly (EIA) in the equinoctial month of March. The analysis also included the total electron content (TEC) as measured by a GPS receiver operated at the EIA crest location. The foF2 data set covered a period of large solar flux variation from 1996 to 2003, while the GPS TEC data was for a period in 2002–2003 when the solar flux parameter F10.7 underwent large variations, permitting in both cases an examination of the solar flux effects on these parameters. The seasonal variation pattern in TEC shows a maximum in equinoctial months and a minimum in June solstice, with similar variations for foF2. The solar flux dependence of the TEC is a maximum during equinoxes, especially for post-sunset TEC values at times when the latitudinal distribution is controlled by the equatorial evening plasma fountain processes. Significant variations with local time are found in the degree of solar flux dependence for both the TEC and EIA. The EIA intensity shows large dependence on F10.7 during post-sunset to midnight hours. These results are discussed in comparison with their corresponding IRI representations. 相似文献
990.