全文获取类型
收费全文 | 10356篇 |
免费 | 9361篇 |
国内免费 | 1753篇 |
专业分类
航空 | 17996篇 |
航天技术 | 1169篇 |
综合类 | 296篇 |
航天 | 2009篇 |
出版年
2024年 | 117篇 |
2023年 | 240篇 |
2022年 | 357篇 |
2021年 | 447篇 |
2020年 | 545篇 |
2019年 | 1218篇 |
2018年 | 1388篇 |
2017年 | 1335篇 |
2016年 | 1332篇 |
2015年 | 1276篇 |
2014年 | 1079篇 |
2013年 | 1117篇 |
2012年 | 1053篇 |
2011年 | 993篇 |
2010年 | 984篇 |
2009年 | 1023篇 |
2008年 | 887篇 |
2007年 | 734篇 |
2006年 | 569篇 |
2005年 | 396篇 |
2004年 | 376篇 |
2003年 | 334篇 |
2002年 | 366篇 |
2001年 | 304篇 |
2000年 | 276篇 |
1999年 | 308篇 |
1998年 | 237篇 |
1997年 | 209篇 |
1996年 | 159篇 |
1995年 | 136篇 |
1994年 | 142篇 |
1993年 | 194篇 |
1992年 | 136篇 |
1991年 | 314篇 |
1990年 | 263篇 |
1989年 | 294篇 |
1988年 | 208篇 |
1987年 | 83篇 |
1986年 | 32篇 |
1983年 | 4篇 |
1981年 | 3篇 |
1972年 | 1篇 |
1962年 | 1篇 |
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
1.
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
2.
H. Thiemann R. W. Schunk 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1992,12(12):143-146
Heavy emission caused by impacting plasma ions results in a fast discharging effect of the initially large surface potentials on the dielectric solar cells. This eventually counteracts the energization process of the plasma ions to the cover glasses and leaves no significant electric fields. Thus, with an existing thermal plasma, electrons are again able to reach dielectric surfaces. Strong localized electric fields of the order of several 10 kV/cm form near the interconnector-cover glass interface. 相似文献
3.
T. J. Ponman A. M. Read 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1993,13(12):361-364
Using data from the Wide Field Camera EUV all-sky survey, we have established upper limits to the EUV flux from a sample of 30 bright, nearby, non-active spiral galaxies. These galaxies were chosen to be those most likely to be detected in the EUV on the basis of (i) low interstellar absorption within our own galaxy, (ii) brightness in other wavebands, (iii) high star formation activity, and (iv) proximity. The derived EUV upper limits are restrictive, and establish for the first time that the EUV flux escaping from galaxies does not constitute a major component of their bolometric luminosity, and in particular that it cannot be the sink for the energy injected into the interstellar medium by supernova explosions, as had been suggested following the failure to detect this power in the X-ray band. 相似文献
4.
5.
本文介绍了一种基于DWDM光接入网的波长分配算法,该算法在保证基本服务质量的前提下,通过调度共享波长降低业务请求过程中的阻塞率。文中还对该算法进行了计算机仿真实验,仿真结果表明了该算法的有效性。 相似文献
6.
7.
一种基于误差四元数的战术导弹垂直发射姿态调转控制器 总被引:3,自引:0,他引:3
针对战术导弹垂直发射姿态调转时的快速性要求,研究了垂直发射快速姿态调转的控制问题。首先基于误差四元数并结合垂直发射的具体特点,建立了战术导弹垂直发射的非线性数学模型;然后通过李亚普诺夫第二方法进行控制系统设计,得出了基于误差四元数反馈控制器。分析了系统的稳定性和鲁棒性。该控制器实现了绕欧拉特征轴的旋转,缩短了姿态调转的时间,最后通过仿真验证其有效性。 相似文献
8.
The primary objective of the Laser Interferometer Space Antenna (LISA) mission is to detect and observe gravitational waves from massive black holes and galactic binaries in the frequency range 10−4 to 10−1 Hz. This low-frequency range is inaccessible to ground-based interferometers because of the unshieldable background of local gravitational noise and because ground-based interferometers are limited in length to a few km. LISA is an ESA cornerstone mission and recently had a system study (Ref. 1) carried out by a consortium led by Astrium, which confirmed the basic configuration for the payload with only minor changes, and provided detailed concepts for the spacecraft and mission design. The study confirmed the need for a drag-free technology demonstration mission to develop the inertial sensors for LISA, before embarking on the build of the flight sensors. With a technology demonstration flight in 2005, it would be possible to carry out LISA as a joint ESA-NASA mission with a launch by 2010 subject to the funding programmatics. The baseline for LISA is three disc-like spacecraft each of which consist of a science module which carries the laser interferometer payload (two in each science module) and a propulsion module containing an ion drive and the hydrazine thrusters of the AOCS. The propulsion module is used for the transfer from earth escape trajectory provided by the Delta II launch to the operational orbit. Once there the propulsion module is jettisoned to reduce disturbances on the payload. Detailed analysis of thermal and gravitational disturbances, a model of the drag-free control and of the interferometer operation confirm that the strain sensitivity of the interferometer will be achieved. 相似文献
9.
10.