全文获取类型
收费全文 | 3406篇 |
免费 | 716篇 |
国内免费 | 603篇 |
专业分类
航空 | 2395篇 |
航天技术 | 739篇 |
综合类 | 680篇 |
航天 | 911篇 |
出版年
2024年 | 12篇 |
2023年 | 37篇 |
2022年 | 117篇 |
2021年 | 124篇 |
2020年 | 124篇 |
2019年 | 97篇 |
2018年 | 97篇 |
2017年 | 105篇 |
2016年 | 117篇 |
2015年 | 156篇 |
2014年 | 225篇 |
2013年 | 229篇 |
2012年 | 231篇 |
2011年 | 258篇 |
2010年 | 275篇 |
2009年 | 231篇 |
2008年 | 229篇 |
2007年 | 215篇 |
2006年 | 199篇 |
2005年 | 165篇 |
2004年 | 101篇 |
2003年 | 102篇 |
2002年 | 106篇 |
2001年 | 119篇 |
2000年 | 123篇 |
1999年 | 104篇 |
1998年 | 117篇 |
1997年 | 104篇 |
1996年 | 86篇 |
1995年 | 78篇 |
1994年 | 69篇 |
1993年 | 88篇 |
1992年 | 51篇 |
1991年 | 61篇 |
1990年 | 58篇 |
1989年 | 32篇 |
1988年 | 38篇 |
1987年 | 18篇 |
1986年 | 15篇 |
1985年 | 4篇 |
1983年 | 1篇 |
1982年 | 5篇 |
1980年 | 1篇 |
1965年 | 1篇 |
排序方式: 共有4725条查询结果,搜索用时 218 毫秒
741.
742.
针对小卫星研制中出现的一些非常规动力学问题进行研究,并提出解决办法。针对小卫星组件最大冲击谱量级超出常规冲击试验规范谱的分析与验证困难,通过研究提出了能够分析评估组件高量级冲击的方法。针对小卫星随机振动下强度设计方法还存在较大误差,分析了系统模态质量比与模态频率在一定频段的影响规律,认为忽略模态质量耦合会带来误差,提出了考虑模态质量耦合的准静态载荷计算方法。最后,针对小卫星整星开展了减振研究,分析了正弦和随机减振效果,对于对称安装减振系统,提出了减振系统的主频率计算公式。 相似文献
743.
Lin Quan Bing Cai Xiong Hu Qingchen Xu Ling Li 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(2):715-721
During solar flares, the X-ray radiation suddenly increases, resulting in an increase in the electron density of the atmospheric D region and a strong absorption of short-wave radio waves. Based on Langfang medium frequency (MF) radar, this paper analyzed the variation characteristics of D region in the lower ionosphere from 62 km to 82 km. The analysis focused on multiple C-level and M-level solar flare events before and after the large-scale flare event at 11:53 (UT) on September 6, 2017. The results show that it is difficult to detect the electron density over 70 km in Langfang during solar flares, but the electron density value can be obtained as low as 62 km, and the stronger the flare intensity, the lower the detectable electron density height. Besides, the equal electron density height, the received power of X and O waves will also be significantly reduced during the flares, and the reduction of equal electron density height has a weak linear relationship with flare intensity. 相似文献
744.
Jing-Fan Gao Li-Xin Guo Zheng-Wen Xu Hai-Sheng Zhao Jie Feng 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(9):2234-2244
Ionospheric inhomogeneous plasma produced by single point chemical release has simple space-time structure, and cannot impact radio wave frequencies higher than Very High Frequency (VHF) band. In order to produce more complicated ionospheric plasma perturbation structure and trigger instabilities phenomena, multiple-point chemical release scheme is presented in this paper. The effects of chemical release on low latitude ionospheric plasma are estimated by linear instability growth rate theory that high growth rate represents high irregularities, ionospheric scintillation occurrence probability and high scintillation intension in scintillation duration. The amplitude scintillations and the phase scintillations of 150?MHz, 400?MHz, and 1000?MHz are calculated based on the theory of multiple phase screen (MPS), when they propagate through the disturbed area. 相似文献
745.
Fuyu Sun Jianping Zhou Zheyao Xu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(1):189-206
This study proposes a new simulation platform named Simulation Integrated Management (SIM) for the analysis of parallel and distributed systems. The platform eases the process of designing and testing both applications and architectures. The main characteristics of SIM are flexibility, scalability, and expandability. To improve the efficiency of project development, new models of early-warning satellite system were designed based on the SIM platform. Finally, through a series of experiments, the correctness of SIM platform and the aforementioned early-warning satellite models was validated, and the systematical analyses for the orbital determination precision of the ballistic missile during its entire flight process were presented, as well as the deviation of the launch/landing point. Furthermore, the causes of deviation and prevention methods will be fully explained. The simulation platform and the models will lay the foundations for further validations of autonomy technology in space attack-defense architecture research. 相似文献
746.
747.
Yue Wang Shijie Xu Mengping Zhu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The full dynamics of spacecraft around an asteroid, in which the spacecraft is considered as a rigid body and the gravitational orbit–attitude coupling is taken into account, is of great value and interest in the precise theories of the motion. The spectral stability of the classical relative equilibria of the full spacecraft dynamics around an asteroid is studied with the method of geometric mechanics. The stability conditions are given explicitly based on the characteristic equation of the linear system matrix. It is found that the linearized system decouples into two entirely independent subsystems, which correspond to the motions within and outside the equatorial plane of the asteroid respectively. The system parameters are divided into three groups that describe the traditional stationary orbit stability, the significance of the orbit–attitude coupling and the mass distribution of the spacecraft respectively. The spectral stability of the relative equilibria is investigated numerically with respect to the three groups of system parameters. The relations between the full spacecraft dynamics and the traditional spacecraft dynamics, as well as the effect of the orbit–attitude coupling, are assessed. We find that when the orbit–attitude coupling is strong, the mass distribution of the spacecraft dominates the stability of the relative equilibria; whereas when the orbit–attitude coupling is weak, both the mass distribution and the traditional stationary orbit stability have significant effects on the stability. We also give a criterion to determine whether the orbit–attitude coupling needs to be considered. 相似文献
748.
J.S. Xu X.J. LiY.W. Liu M. Jing 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Based on measurements of ground-based GPS station network, differences of the mid-latitude ionospheric TEC in the east and west sides of North America, South America and Oceania have been analyzed in this paper. Results show that for nearly all seasons from 2001 to 2010 and in both sides of the longitudes with zero declination, there exist systematic differences for the mid-latitude ionospheric TEC in the regions mentioned above and the features of these differences markedly depend upon the local time but less depend upon seasons and the level of solar activity. Theory analysis shows that the longitude variations of both declination and zonal thermospheric winds are one of important factors to cause differences of the mid-latitude ionospheric TEC in both sides of the longitudes with zero declination. 相似文献
750.
表层采样是月球采样探测的重要方式,样品智能确认有助于提升工作效率与复杂问题处理能力。结合月球表层采样铲挖工作过程,分析了铲挖过程中臂载相机图像的特点,模仿有人参与识别过程,提出了层次解耦的月球样品智能识别流程,利用深度学习方法构建了一类深度卷积识别网络,完整地描述了图像、特征、标记在网络中的正反传递关系,并在月球表层采样地面试验中进行了验证,结果表明该方法对不同光照、不同背景、不同过程、不同形态的样品,具有较好的泛化识别能力,误识别率优于8.1%,平均单幅识别时间约0.7 s。 相似文献