全文获取类型
收费全文 | 15950篇 |
免费 | 10084篇 |
国内免费 | 2646篇 |
专业分类
航空 | 20764篇 |
航天技术 | 2753篇 |
综合类 | 1263篇 |
航天 | 3900篇 |
出版年
2024年 | 121篇 |
2023年 | 265篇 |
2022年 | 482篇 |
2021年 | 571篇 |
2020年 | 672篇 |
2019年 | 1277篇 |
2018年 | 1481篇 |
2017年 | 1422篇 |
2016年 | 1439篇 |
2015年 | 1468篇 |
2014年 | 1441篇 |
2013年 | 1390篇 |
2012年 | 1412篇 |
2011年 | 1382篇 |
2010年 | 1481篇 |
2009年 | 1457篇 |
2008年 | 1268篇 |
2007年 | 1085篇 |
2006年 | 880篇 |
2005年 | 654篇 |
2004年 | 535篇 |
2003年 | 508篇 |
2002年 | 561篇 |
2001年 | 479篇 |
2000年 | 467篇 |
1999年 | 525篇 |
1998年 | 484篇 |
1997年 | 399篇 |
1996年 | 345篇 |
1995年 | 297篇 |
1994年 | 290篇 |
1993年 | 304篇 |
1992年 | 247篇 |
1991年 | 389篇 |
1990年 | 324篇 |
1989年 | 339篇 |
1988年 | 259篇 |
1987年 | 118篇 |
1986年 | 57篇 |
1985年 | 22篇 |
1984年 | 13篇 |
1983年 | 13篇 |
1982年 | 13篇 |
1981年 | 24篇 |
1979年 | 2篇 |
1978年 | 3篇 |
1976年 | 2篇 |
1974年 | 3篇 |
1972年 | 2篇 |
1965年 | 3篇 |
排序方式: 共有10000条查询结果,搜索用时 31 毫秒
1.
2.
针对红外与可见光图像融合中特征损失严重、显著目标不突出的问题,提出了一种低秩表示分解与深度神经网络相结合的图像融合算法。首先,对源图像进行潜在低秩表示分解(DLatLRR),得到相应的低秩部分、显著部分及稀疏噪声。然后,分别采用16层的VGG Net模型和联合特征加权算法对低秩部分与显著部分进行融合,舍弃二者的稀疏噪声。最后,对融合得到的低秩部分和显著部分进行图像重建,得到最终的融合图像。实验结果表明:与其他算法进行比较,所提算法能够对图像的深层次细节特征进行融合,突出场景中的感兴趣区域,且融合图像的相关差异和、结构相似性、线性相关度等多种客观指标均有所提升,提升最大值分别为0.73、0.15、0.11,噪声产生率的最大缩减值为0.041 2。 相似文献
3.
Yongjie Ding Jia Boyang Hezhi Sun Liqiu Wei Wuji Peng Peng Li Daren Yu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(3):837-843
Discharge characteristics of a non-wall-loss Hall thruster were studied under different channel lengths using a design based on pushing a magnetic field through a double permanent magnet ring. The effect of different magnetic field intensities and channel lengths on ionization, efficiency, and plume divergence angle were studied. The experimental results show that propellant utilization is improved for optimal matching between the magnetic field and channel length. While matching the magnetic field and channel length, the ionization position of the neutral gas changes. The ion flow is effectively controlled, allowing the thrust force, specific impulse, and efficiency to be improved. Our study shows that the channel length is an important design parameter to consider for improving the performance of non-wall-loss Hall thrusters. 相似文献
4.
5.
摘要: 为满足未来脉冲星导航和空间天文观测任务对X射线望远镜的载荷需求,Wolter I光学系统的研制正逐渐成为新的研究热点,电铸镍方案是当前国内外X射线光学系统镜筒制造的主要技术方案.文章对电铸镍X射线光学系统制造工艺、国内外研制现状、未来应用需求进行了介绍和整理,梳理了电铸镍X射线光学系统研制遇到的关键技术和难点,提出了后续研究发展建议,以促进中国在 X射线脉冲星自主导航、空间探测领域的快速发展. 相似文献
6.
Yu Jiang Hexi Baoyin Hengnian Li 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(5):1371-1385
We investigate the orbital stability close to the unique L4-point Jupiter binary Trojan asteroid 624 Hektor. The gravitational potential of 624 Hektor is calculated using the polyhedron model with observational data of 2038 faces and 1021 vertexes. Previous studies have presented three different density values for 624 Hektor. The equilibrium points in the gravitational potential of 624 Hektor with different density values have been studied in detail. There are five equilibrium points in the gravitational potential of 624 Hektor no matter the density value. The positions, Jacobian, eigenvalues, topological cases, stability, as well as the Hessian matrix of the equilibrium points are investigated. For the three different density values the number, topological cases, and the stability of the equilibrium points with different density values are the same. However, the positions of the equilibrium points vary with the density value of the asteroid 624 Hektor. The outer equilibrium points move away from the asteroid’s mass center when the density increases, and the inner equilibrium point moves close to the asteroid’s mass center when the density increases. There exist unstable periodic orbits near the surface of 624 Hektor. We calculated an orbit near the primary’s equatorial plane of this binary Trojan asteroid; the results indicate that the orbit remains stable after 28.8375?d. 相似文献
7.
主要介绍了刹车装置性能试验台的实现机理、采用的方案,有助于增进对液压试验台设计和可编程控制器PLC应用方面的了解。 相似文献
8.
本文简要地介绍了电子工作台的特点和使用方法,结合我们设计具体模拟电子线路的实践,说明了电子工作台在模拟电子技术中的应用。 相似文献
9.
10.
T C Yang M Mei K A George L M Craise 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1996,18(1-2):149-158
Energetic heavy ions are present in galactic cosmic rays and solar particle events. One of the most important late effects in risk assessment is carcinogenesis. We have studied the carcinogenic effects of heavy ions at the cellular and molecular levels and have obtained quantitative data on dose-response curves and on the repair of oncogenic lesions for heavy particles with various charges and energies. Studies with repair inhibitors and restriction endonucleases indicated that for oncogenic transformation DNA is the primary target. Results from heavy ion experiments showed that the cross section increased with LET and reached a maximum value of about 0.02 micrometer2 at about 500 keV/micrometer. This limited size of cross section suggests that only a fraction of cellular genomic DNA is important in radiogenic transformation. Free radical scavengers, such as DMSO, do not give any effect on induction of oncogenic transformation by 600 MeV/u iron particles, suggesting most oncogenic damage induced by high-LET heavy ions is through direct action. Repair studies with stationary phase cells showed that the amount of reparable oncogenic lesions decreased with an increase of LET and that heavy ions with LET greater than 200 keV/micrometer produced only irreparable oncogenic damage. An enhancement effect for oncogenic transformation was observed in cells irradiated by low-dose-rate argon ions (400 MeV/u; 120 keV/micrometer). Chromosomal aberrations, such as translocation and deletion, but not sister chromatid exchange, are essential for heavy-ion-induced oncogenic transformation. The basic mechanism(s) of misrepair of DNA damage, which form oncogenic lesions, is unknown. 相似文献