全文获取类型
收费全文 | 8886篇 |
免费 | 1592篇 |
国内免费 | 1365篇 |
专业分类
航空 | 6247篇 |
航天技术 | 2335篇 |
综合类 | 1031篇 |
航天 | 2230篇 |
出版年
2024年 | 62篇 |
2023年 | 212篇 |
2022年 | 301篇 |
2021年 | 429篇 |
2020年 | 468篇 |
2019年 | 594篇 |
2018年 | 691篇 |
2017年 | 563篇 |
2016年 | 567篇 |
2015年 | 489篇 |
2014年 | 549篇 |
2013年 | 493篇 |
2012年 | 634篇 |
2011年 | 726篇 |
2010年 | 482篇 |
2009年 | 435篇 |
2008年 | 555篇 |
2007年 | 553篇 |
2006年 | 515篇 |
2005年 | 420篇 |
2004年 | 344篇 |
2003年 | 256篇 |
2002年 | 193篇 |
2001年 | 200篇 |
2000年 | 146篇 |
1999年 | 143篇 |
1998年 | 143篇 |
1997年 | 108篇 |
1996年 | 91篇 |
1995年 | 103篇 |
1994年 | 104篇 |
1993年 | 54篇 |
1992年 | 52篇 |
1991年 | 50篇 |
1990年 | 37篇 |
1989年 | 42篇 |
1988年 | 25篇 |
1987年 | 7篇 |
1986年 | 2篇 |
1984年 | 4篇 |
1981年 | 1篇 |
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
21.
美国科技文献资源体系建设及启示 总被引:4,自引:0,他引:4
介绍了美国联邦政府和国家航空般天局(NASA)科技文献信息资源体系建设,科技信息纲领的内涵、宗旨、任务、目标,实施科技信息纲领的工作程序、组织管理机构,科技信息产品和服务,以及美国国家技术信息服务中心(NTIS)和航空航天科技信息中心(CASI)的运作情况,论述了美国科技文献信息资源在推动科技进步中的作用,并在研究分析的基础上给出了结论。 相似文献
22.
The fastest pulsar and the slowest nova; the oldest galaxies and the youngest stars; the weirdest life forms and the commonest
dwarfs; the highest energy particles and the lowest energy photons. These were some of the extremes of Astrophysics 2006.
We attempt also to bring you updates on things of which there is currently only one (habitable planets, the Sun, and the Universe)
and others of which there are always many, like meteors and molecules, black holes and binaries. 相似文献
23.
本文介绍了一种非常规的高速轴振动抑制方法,主要是用振源分析技术,通过确诊设备故障原因来分析影响轴振动的主要因素,调节机器的系统刚度,再通过理论计算修订安装参数,制定设备故障处理对策,在涟源钢铁集团有限公司一万氧压机组上的实践取得了相当满意的效果,很有推广价值。 相似文献
24.
Martin A. Lee 《Space Science Reviews》2007,130(1-4):221-229
Gradual solar energetic particle (SEP) events are evidently accelerated by coronal/interplanetary shocks driven by coronal
mass ejections. This talk addresses the different factors which determine the composition of the accelerated ions. The first
factor is the set of available seed populations including the solar wind core and suprathermal tail, remnant impulsive events
from preceding solar flares, and remnant gradual events. The second factor is the fractionation of the seed ions by the injection
process, that is, what fraction of the ions are extracted by the shock to participate in diffusive shock acceleration. Injection
is a controversial topic since it depends on the detailed electromagnetic structure of the shock transition and the transport
of ions in these structured fields, both of which are not well understood or determined theoretically. The third factor is
fractionation during the acceleration process, due to the dependence of ion transport in the turbulent electromagnetic fields
adjacent to the shock on the mass/charge ratio. Of crucial importance in the last two factors is the magnetic obliquity of
the shock. The form of the proton-excited hydromagnetic wave spectrum is also important. Finally, more subtle effects on ion
composition arise from the superposition of ion contributions over the time history of the shock along the observer’s magnetic
flux tube, and the sequence of flux tubes sampled by the observer. 相似文献
25.
When a micro-debris or a micrometeoroid impacts a spacecraft surface, a large number of secondary particles, called ejecta, are produced. These particles can contribute to a modification of the debris environment: either locally by the occurrence of secondary impacts on the components of complex and large space structures, or at great distance by the formation of a population of small orbital debris. This paper describes firstly, the ejecta overall production, and secondly, the lifetime and the orbital evolution of the particles. Finally the repartition of ejecta in LEO is computed. Some results describing the population as a function of size and altitude are presented. 相似文献
26.
Mauro Orlandini 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2742-2746
Broad-band spectra of accreting X-ray binary pulsars can be fitted by a phenomenological model composed of a power law with a high energy rollover above 10 keV, plus a blackbody component with a temperature of few hundred eV. While, at least qualitatively, the hard tail can be explained in terms of (inverse) Compton scattering, the origin of the soft component cannot find a unique explanation. Recently, a qualitative picture able to explain the overall broad-band spectrum of luminous X-ray pulsars was carried out by taking into account the effect of bulk Comptonization in the accretion column. After a review of these recent theoretical developments, I will present a case study of how different modeling of the continuum affect broad features, in particular the cyclotron resonance features in Vela X-1. 相似文献
27.
A.G. Lyne 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2716-2720
A recent multibeam pulsar survey of the outer Galactic plane at Parkes has discovered the first-known double-pulsar binary, a very compact double neutron star system in which both stars are observable as radio pulsars. In this review, we briefly describe the discovery and the studies which have been enabled by the unique properties of the system. These range from the most precise confirmation yet of the theory of general relativity, with the possibility of even more new tests and the measurement of second-order post-Newtonian effects, to studies of the magnetospheres and emission properties of the two pulsars. The discovery also results in a significant increase in the expected rate of occurrence of the mergers of double neutron star systems, and hence the rate of detection of such events by the new ground-based gravitational wave detectors. 相似文献
28.
Nazar R. Ikhsanov Chul-Sung Choi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2901-2902
The state of subsonic propeller is intermediate between the states of supersonic propeller and accretor in the evolutionary tracks of magnetized compact stars. The rotational rate of a star at this stage decelerates due to the interaction between its magnetosphere and the surrounding hot, quasi-static plasma envelope. The magnetospheric radius is smaller than the corotation radius and the boundary of the magnetosphere is stable with respect to interchange instabilities. The rate of the mass flux from the inner radius of the envelope to the stellar surface is limited by the rate of plasma diffusion into the magnetic field of the star. As a result, the subsonic propeller would appear as a low-luminosity accretion-powered pulsar with a soft X-ray spectrum. 相似文献
29.
本文研究的是四维飞行性能管理系统的核心环节-飞机在终端区域内的四维下降技术,首先探讨了基于常值航迹角的定常M数/指示空速下降飞行技术,论述了其高度剖面的构成与特点,通过尤拉积分方法求解飞机运动方程,实现了高度冲面的解算。其次开发了对速度剖面的迭代过程,选取原则及方法。本文在进行理论分析的同时,还开发了满意的仿真软件,一了其应用价值。 相似文献
30.
光学中心偏测量仪软件研制 总被引:3,自引:0,他引:3
文章介绍了北京空间机电研究所自行研制的光学中心偏测量仪的软件设计思路、工作原理 ,并对一些关键技术进行了讨论。 相似文献