全文获取类型
收费全文 | 5302篇 |
免费 | 1089篇 |
国内免费 | 956篇 |
专业分类
航空 | 3780篇 |
航天技术 | 1730篇 |
综合类 | 610篇 |
航天 | 1227篇 |
出版年
2024年 | 49篇 |
2023年 | 118篇 |
2022年 | 209篇 |
2021年 | 301篇 |
2020年 | 325篇 |
2019年 | 461篇 |
2018年 | 567篇 |
2017年 | 435篇 |
2016年 | 391篇 |
2015年 | 349篇 |
2014年 | 255篇 |
2013年 | 271篇 |
2012年 | 370篇 |
2011年 | 428篇 |
2010年 | 282篇 |
2009年 | 254篇 |
2008年 | 312篇 |
2007年 | 287篇 |
2006年 | 326篇 |
2005年 | 212篇 |
2004年 | 174篇 |
2003年 | 127篇 |
2002年 | 96篇 |
2001年 | 109篇 |
2000年 | 79篇 |
1999年 | 77篇 |
1998年 | 80篇 |
1997年 | 74篇 |
1996年 | 71篇 |
1995年 | 65篇 |
1994年 | 81篇 |
1993年 | 30篇 |
1992年 | 26篇 |
1991年 | 12篇 |
1990年 | 11篇 |
1989年 | 12篇 |
1988年 | 9篇 |
1987年 | 9篇 |
1986年 | 1篇 |
1984年 | 1篇 |
1981年 | 1篇 |
排序方式: 共有7347条查询结果,搜索用时 15 毫秒
1.
2.
本文首先分析了当前直升机在运用CAD/CAE/CAM技术进行研制中存在的一些问题,接着提供了解决的方法,介绍了PDM的概念、构成、主要功能。最后简述了PDM技术在直升机研制中的作用,以及企业在实施PDM当中应注意的一些问题。 相似文献
3.
4.
经营机制创新是中小型外贸企业摆脱困境的必由之路。针对目前面临的主要问题,从外部环境及企业自身经营机制缺陷方面对中小型外贸企业生存环境进行分析,并从实现经营机制创新角度探讨改善现状的方法,力图找出中小型外贸企业经营机制创新的突破点。 相似文献
5.
A numerical procedure for the calculation of the transonic dip of airfoils in the time domain is presented. A viscous-inviscid aerodynamic interaction method is taken to calculate the unsteady aerodynamic loads. In the present case the integral boundary layer equations are coupled with the Transonic Small Disturbance (TSD) Potential Equation. The coupling between structural motion and aerodynamic loads is carried out using State Space equation. It is solved by State Transition Matrix technique. Results are presented for NACA 64A010 and NLR 7301 airfoils with structural data from Isogai and DLR, respectively. Comparisons show good agreement with other numerical results. Certain deviations of experimental data taken from literature need more insight in the detailed test conditions. 相似文献
6.
ected g 《桂林航天工业高等专科学校学报》2006,(2)
with primary goat embryonic fibroblast showed no difference from traditional feederlayer-based culture method used in mouse and human. The putative primary EG colonies were multilayer clumps ofcompact cel 相似文献
7.
运用理论分析方法和实测试验方法,探讨了梁在塑性动态断裂过程中,其塑性铰转动因子的变化规律,提出了断裂过程中塑性铰几何转动因子的概念及其确定方法,并以3点弯曲梁理论分析解为例,计算了梁在塑性动态断裂过程中,其塑性铰转动因子的变化规律。该计算结果与3点弯曲梁动态断理解实验实测相一致。理论分析进一步明确了梁的塑性铰转动因子具有几何与物理两种不同的本质含意,并可直接用于修正梁的塑性动态断裂的理论分析解。 相似文献
8.
应用奇异摄动法分析横侧小扰动运动的动稳定性问题,将四阶问题分解为小根、大根和复根模态,它对应于经典理论中的螺旋、滚转和荷兰滚模态,并给出了动态反应过程的解。 相似文献
9.
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
10.
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