全文获取类型
收费全文 | 9589篇 |
免费 | 2303篇 |
国内免费 | 2007篇 |
专业分类
航空 | 9109篇 |
航天技术 | 1682篇 |
综合类 | 1287篇 |
航天 | 1821篇 |
出版年
2024年 | 40篇 |
2023年 | 136篇 |
2022年 | 324篇 |
2021年 | 404篇 |
2020年 | 419篇 |
2019年 | 403篇 |
2018年 | 395篇 |
2017年 | 497篇 |
2016年 | 525篇 |
2015年 | 507篇 |
2014年 | 609篇 |
2013年 | 544篇 |
2012年 | 784篇 |
2011年 | 816篇 |
2010年 | 653篇 |
2009年 | 775篇 |
2008年 | 634篇 |
2007年 | 610篇 |
2006年 | 567篇 |
2005年 | 497篇 |
2004年 | 373篇 |
2003年 | 356篇 |
2002年 | 353篇 |
2001年 | 267篇 |
2000年 | 289篇 |
1999年 | 281篇 |
1998年 | 218篇 |
1997年 | 235篇 |
1996年 | 246篇 |
1995年 | 194篇 |
1994年 | 188篇 |
1993年 | 176篇 |
1992年 | 133篇 |
1991年 | 120篇 |
1990年 | 111篇 |
1989年 | 94篇 |
1988年 | 101篇 |
1987年 | 19篇 |
1986年 | 5篇 |
1984年 | 1篇 |
排序方式: 共有10000条查询结果,搜索用时 110 毫秒
11.
用数值方法模拟双锥,圆柱,椭球、圆锥和倒圆锥五类等质量异形铝粒子五种高宽比共25种粒子对半无限铝靶的超高速撞击侵蚀,撞击速度为4km/s,给出了坑深、坑径、坑形参数和坑体积随粒子形状及高宽比的变化曲线。结果与非圆球异形粒子超高速撞击侵蚀计算有重要参考价值。 相似文献
12.
本文是近年来在微波聚焦热疗人体深部癌病灶研究工作推动下完成的。文中给出了光学及电磁学界感兴趣的某些结果。在人体分层媒质前的一有限口径处,置一时谐电流分布,在每一分层内的微波传输场及反射场可利用传输矩阵及并矢格林函数给出计算结果。 相似文献
13.
Mercury’s unusually high mean density has always been attributed to special circumstances that occurred during the formation of the planet or shortly thereafter, and due to the planet’s close proximity to the Sun. The nature of these special circumstances is still being debated and several scenarios, all proposed more than 20 years ago, have been suggested. In all scenarios, the high mean density is the result of severe fractionation occurring between silicates and iron. It is the origin of this fractionation that is at the centre of the debate: is it due to differences in condensation temperature and/or in material characteristics (e.g. density, strength)? Is it because of mantle evaporation due to the close proximity to the Sun? Or is it due to the blasting off of the mantle during a giant impact? In this paper we investigate, in some detail, the fractionation induced by a giant impact on a proto-Mercury having roughly chondritic elemental abundances. We have extended the previous work on this hypothesis in two significant directions. First, we have considerably increased the resolution of the simulation of the collision itself. Second, we have addressed the fate of the ejecta following the impact by computing the expected reaccretion timescale and comparing it to the removal timescale from gravitational interactions with other planets (essentially Venus) and the Poynting–Robertson effect. To compute the latter, we have determined the expected size distribution of the condensates formed during the cooling of the expanding vapor cloud generated by the impact. We find that, even though some ejected material will be reaccreted, the removal of the mantle of proto-Mercury following a giant impact can indeed lead to the required long-term fractionation between silicates and iron and therefore account for the anomalously high mean density of the planet. Detailed coupled dynamical–chemical modeling of this formation mechanism should be carried out in such a way as to allow explicit testing of the giant impact hypothesis by forthcoming space missions (e.g. MESSENGER and BepiColombo). 相似文献
14.
空间能量粒子探测方法研究 总被引:1,自引:0,他引:1
阐述了空间能量粒子探测的原理和方法。介绍了国外在能量粒子探测方面所采用的半导体望远镜测量法、电场加速法、磁偏转法等方法,分析了它们各自的优缺点。就制约能量粒子探测技术发展的关键因素进行了讨论。并以此为基础,结合我国实际情况提出了一种新的探测方法。 相似文献
15.
Space-Wise,Time-Wise,Torus and Rosborough Representations in Gravity Field Modelling 总被引:1,自引:0,他引:1
The decade of the geopotentials started July 2000 with the launch of the German high-low SST mission CHAMP. Together with the joint NASA-DLR low-low SST
mission GRACE and the ESA gradiometry mission GOCE an unprecedented wealth of geopotential data becomes available over the
next few years.
Due to the sheer number of unknown gravity field parameters (up to 100 000) and of observations (millions), especially the
latter two missions are highly demanding in terms of computational requirements. In this paper several modelling strategies
are presented that are based on a semi-analytical approach. In this approach the set of normal equations becomes block-diagonal
with maximum block-sizes smaller than the spherical harmonic degree of resolution. The block-diagonality leads to a rapid
and powerful gravity field analysis tool.
Beyond the more-or-less conventional space-wise and time-wise formulations, the torus approach and Rosborough's representation
are discussed. A trade-off between pros and cons of each of the modelling strategies will be given.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
16.
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
17.
空战机动动作库设计方式研究 总被引:13,自引:0,他引:13
具体阐述了两类常见空战动作库的设计 :典型战术动作库和基本操作动作库 ,详细分析了这两类空战机动动作库的不足 ,最后提出了改进动作库设计的具体意见和建议。 相似文献
18.
19.
20.
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