全文获取类型
收费全文 | 5129篇 |
免费 | 649篇 |
国内免费 | 484篇 |
专业分类
航空 | 2673篇 |
航天技术 | 1452篇 |
综合类 | 435篇 |
航天 | 1702篇 |
出版年
2024年 | 15篇 |
2023年 | 47篇 |
2022年 | 108篇 |
2021年 | 165篇 |
2020年 | 129篇 |
2019年 | 112篇 |
2018年 | 182篇 |
2017年 | 181篇 |
2016年 | 171篇 |
2015年 | 170篇 |
2014年 | 245篇 |
2013年 | 233篇 |
2012年 | 252篇 |
2011年 | 311篇 |
2010年 | 330篇 |
2009年 | 374篇 |
2008年 | 329篇 |
2007年 | 259篇 |
2006年 | 195篇 |
2005年 | 204篇 |
2004年 | 147篇 |
2003年 | 182篇 |
2002年 | 196篇 |
2001年 | 186篇 |
2000年 | 137篇 |
1999年 | 140篇 |
1998年 | 109篇 |
1997年 | 111篇 |
1996年 | 112篇 |
1995年 | 108篇 |
1994年 | 86篇 |
1993年 | 55篇 |
1992年 | 73篇 |
1991年 | 43篇 |
1990年 | 38篇 |
1989年 | 51篇 |
1988年 | 31篇 |
1987年 | 26篇 |
1986年 | 30篇 |
1985年 | 77篇 |
1984年 | 41篇 |
1983年 | 27篇 |
1982年 | 40篇 |
1981年 | 76篇 |
1980年 | 18篇 |
1978年 | 10篇 |
1977年 | 14篇 |
1976年 | 11篇 |
1975年 | 14篇 |
1974年 | 17篇 |
排序方式: 共有6262条查询结果,搜索用时 15 毫秒
361.
362.
363.
无陀螺捷联惯导系统仅利用加速度计就可完成惯性测量与导航,然而采用积分法解算载体的角速度时误差积累严重,发散迅速。文章采用一种常用的九加速度计配置方案,设计一种积分法补偿算法,并针对其初始时段误差过大的问题提出了一种组合算法。仿真验证能有效地抑制解算误差的发散,提高了解算精度。 相似文献
364.
365.
Structure of a two-phase flow of boiling water at low-head adiabatic efflux through the laval nozzle
The critical flow conditions and structural forms of a two-phase flow that is formed during water efflux from the region of moderate and low pressures into a rarefied medium are analyzed. The difference in the structural forms of a flow realized at the low-head efflux from the structure of a flow occurring in the fluid flow with moderate and high initial pressures is established. The critical pressure differential characterizing the establishment of the maximum flowrate is determined and the decisive influence of turbulence on the vapor phase generation and flow conditions of a two-phase medium is shown. 相似文献
366.
Yuri N. Kulikov Helmut Lammer Herbert I. M. Lichtenegger Thomas Penz Doris Breuer Tilman Spohn Rickard Lundin Helfried K. Biernat 《Space Science Reviews》2007,129(1-3):207-243
Because the solar radiation and particle environment plays a major role in all atmospheric processes such as ionization, dissociation,
heating of the upper atmospheres, and thermal and non-thermal atmospheric loss processes, the long-time evolution of planetary
atmospheres and their water inventories can only be understood within the context of the evolving Sun. We compare the effect
of solar induced X-ray and EUV (XUV) heating on the upper atmospheres of Earth, Venus and Mars since the time when the Sun
arrived at the Zero-Age-Main-Sequence (ZAMS) about 4.6 Gyr ago. We apply a diffusive-gravitational equilibrium and thermal
balance model for studying heating of the early thermospheres by photodissociation and ionization processes, due to exothermic
chemical reactions and cooling by IR-radiating molecules like CO2, NO, OH, etc. Our model simulations result in extended thermospheres for early Earth, Venus and Mars. The exospheric temperatures
obtained for all the three planets during this time period lead to diffusion-limited hydrodynamic escape of atomic hydrogen
and high Jeans’ escape rates for heavier species like H2, He, C, N, O, etc. The duration of this blow-off phase for atomic hydrogen depends essentially on the mixing ratios of CO2, N2 and H2O in the atmospheres and could last from ∼100 to several hundred million years. Furthermore, we study the efficiency of various
non-thermal atmospheric loss processes on Venus and Mars and investigate the possible protecting effect of the early martian
magnetosphere against solar wind induced ion pick up erosion. We find that the early martian magnetic field could decrease
the ion-related non-thermal escape rates by a great amount. It is possible that non-magnetized early Mars could have lost
its whole atmosphere due to the combined effect of its extended upper atmosphere and a dense solar wind plasma flow of the
young Sun during about 200 Myr after the Sun arrived at the ZAMS. Depending on the solar wind parameters, our model simulations
for early Venus show that ion pick up by strong solar wind from a non-magnetized planet could erode up to an equivalent amount
of ∼250 bar of O+ ions during the first several hundred million years. This accumulated loss corresponds to an equivalent mass of ∼1 terrestrial
ocean (TO (1 TO ∼1.39×1024 g or expressed as partial pressure, about 265 bar, which corresponds to ∼2900 m average depth)). Finally, we discuss and
compare our findings with the results of preceding studies. 相似文献
367.
It is widely accepted that diffusive shock acceleration is an important process in the heliosphere, in particular in producing
the energetic particles associated with interplanetary shocks driven by coronal mass ejections. In its simplest formulation
shock acceleration is expected to accelerate ions with higher mass to charge ratios less efficiently than those with lower
mass to charge. Thus it is anticipated that the Fe/O ratio in shock-accelerated ion populations will decrease with increasing
energy above some energy. We examine the circumstances of five interplanetary shocks that have been reported to have associated
populations in which Fe/O increases with increasing energy. In each event, the situation is complex, with particle contributions
from other sources in addition to the shock. Furthermore, we show that the Fe/O ratio in shock-accelerated ions can decrease
even when the shock is traveling through an Fe-rich ambient ion population. Thus, although shock acceleration of an Fe-rich
suprathermal population has been proposed to explain large Fe-rich solar particle events, we find no support for this proposal
in these observations. 相似文献
368.
形状记忆合金偏心埋入到复合材料层板中可以构成可变形复合材料,并且其在航空航天、工业生产中具有广泛的应用前景.可变形复合材料的主要性能受到形状记忆合金的特性以及制备工艺的制约,可采用单向弯曲、推挽结构和扭曲结构等方法进行设计.通过对形状记忆合金的记忆处理及表面处理,根据形状记忆合金的铺入方式设计,可以制备可变形复合材料试件,这种方法可以为工业生产提供技术参考. 相似文献
369.
370.
硬支承动平衡机通用微机化电测系统的研究 总被引:2,自引:0,他引:2
论述了一种以IBM-PC为主机的微机化通用硬支承动平衡机电测系统的实现方法。系统采用了先进的硬软件结合技术,寻求达到高精度、多功能、易操作和低成本的总体目标。为了满足不同用户的需求,系统具有多种支承方式、多种显示方式、多种补偿方式、多次启动平均、多面校正计算、多和打印方式以及自动标定和留言服务等功能. 相似文献