全文获取类型
收费全文 | 10053篇 |
免费 | 9277篇 |
国内免费 | 1689篇 |
专业分类
航空 | 17837篇 |
航天技术 | 1078篇 |
综合类 | 213篇 |
航天 | 1891篇 |
出版年
2024年 | 109篇 |
2023年 | 220篇 |
2022年 | 345篇 |
2021年 | 389篇 |
2020年 | 501篇 |
2019年 | 1186篇 |
2018年 | 1357篇 |
2017年 | 1291篇 |
2016年 | 1324篇 |
2015年 | 1260篇 |
2014年 | 1075篇 |
2013年 | 1081篇 |
2012年 | 1040篇 |
2011年 | 983篇 |
2010年 | 987篇 |
2009年 | 1004篇 |
2008年 | 858篇 |
2007年 | 739篇 |
2006年 | 586篇 |
2005年 | 392篇 |
2004年 | 371篇 |
2003年 | 315篇 |
2002年 | 353篇 |
2001年 | 302篇 |
2000年 | 272篇 |
1999年 | 282篇 |
1998年 | 233篇 |
1997年 | 205篇 |
1996年 | 157篇 |
1995年 | 135篇 |
1994年 | 139篇 |
1993年 | 193篇 |
1992年 | 136篇 |
1991年 | 313篇 |
1990年 | 262篇 |
1989年 | 294篇 |
1988年 | 207篇 |
1987年 | 82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 0 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.
6.
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
7.
8.
相邻结点负载平衡算法具有计算简单、额外开销小的优点。但由于采用局部的观点平衡负载,限制了结点信息得到的范围,使得系统在某种情况下达不到全局平衡,本文提出了基于偏差信息的星载计算机系统负载平衡算法,它改变了结点传递的实际负载信息,使修改后的负载信息能体现出结点及其周边结点的负载形势,以此弥补了相邻结点负载平衡算法的不足,并将其应用在星载计算机系统上,首先,介绍了相邻结点负载平衡算法及其存在的不足;其次,描述了基于偏差信息的星载计算机系统负载平衡算法,最后,通过仿真实验,给出了这种算法同其它几种负载平衡算法的比较,并证明了它的正确性与可行性。 相似文献
9.
蔡续 《桂林航天工业高等专科学校学报》2006,11(2):35-37
随着高等教育事业的蓬勃发展,特别是高校后勤社会化改革不断深入,中国特色高校后勤管理理论初见端倪。文章从近几年高校后勤管理理论研究的基本情况、高校后勤管理理论研究倾向及问题两个方面,深入探讨了高校后勤管理理论研究这一主题,以期进一少促进高校后勤管理理论研究,加强理论建设,提高理论研究水平,更好地发挥理论对决策的服务功能。 相似文献
10.
介绍一种以大规模集成电路为核心组成的通用计数器的设计。该通用计数器具有输出标准信号、测量频率、测量周期、累加计数和自校等多种功能。 相似文献