全文获取类型
收费全文 | 360篇 |
免费 | 48篇 |
国内免费 | 23篇 |
专业分类
航空 | 122篇 |
航天技术 | 112篇 |
综合类 | 7篇 |
航天 | 190篇 |
出版年
2024年 | 1篇 |
2023年 | 4篇 |
2022年 | 9篇 |
2021年 | 12篇 |
2020年 | 8篇 |
2019年 | 15篇 |
2018年 | 12篇 |
2017年 | 5篇 |
2016年 | 4篇 |
2015年 | 10篇 |
2014年 | 19篇 |
2013年 | 23篇 |
2012年 | 27篇 |
2011年 | 22篇 |
2010年 | 16篇 |
2009年 | 12篇 |
2008年 | 11篇 |
2007年 | 20篇 |
2006年 | 23篇 |
2005年 | 29篇 |
2004年 | 20篇 |
2003年 | 25篇 |
2002年 | 11篇 |
2001年 | 21篇 |
2000年 | 6篇 |
1999年 | 14篇 |
1998年 | 10篇 |
1997年 | 10篇 |
1996年 | 5篇 |
1995年 | 5篇 |
1994年 | 4篇 |
1993年 | 6篇 |
1992年 | 4篇 |
1991年 | 3篇 |
1990年 | 1篇 |
1989年 | 1篇 |
1988年 | 1篇 |
1987年 | 2篇 |
排序方式: 共有431条查询结果,搜索用时 109 毫秒
71.
Sriram Saran Anup DasShiv Mohan Manab Chakraborty 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The surface layer of the Moon preserves vital evidences of lunar impact and cratering processes due to the absence of any Aeolian and fluvial erosion processes acting on it. By examining these evidences, which are recorded throughout the evolutionary history of the Moon, several basic aspects of lunar science can be understood, and this has direct relevance to the surfaces of other airless bodies within the solar system. In this study, rock abundance data obtained from Thermal Infrared (TIR) observations and radar Circular Polarization Ratio (CPR) data sets obtained from polarimetric SAR observations were correlated at some sample sites on the lunar surface. Preliminary results yielded qualitative and quantitative estimates for surface rock abundances. Except at distal ejecta deposits of young, bright craters a general correlation was observed between the two datasets. Mixed results were observed from the impact melt flows where the situation is complex due to the possible subsurface-volume and volume-subsurface interactions of the radar waves. But the flow features were clearly separated from the interior and ejecta regions of their parent craters in terms of CPR and rock abundances. The extent and distributions of pyroclastic deposits and dark haloed regions could not be distinctly identified at the resolution of datasets utilized. Near Gerasimovich D crater, the Diviner Radiometer has provided the first TIR observations of a newly discovered impact melt flow which was not visible in the optical imagery. This facilitated the first ever quantitative comparisons of the radar CPR and rock abundance values near such a region. Also, significant differences in spatial patterns between the radar and rock concentration data sets were observed, owing to the differences in the sensitivity of the two observations. 相似文献
72.
73.
74.
Saurabh Das Ashish K. Shukla Animesh Maitra 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
The microstructure of rain has been studied with observations using a vertical looking Micro Rain Radar (MRR) at Ahmedabad (23.06°N, 72.62°E), a tropical location in the Indian region. The rain height, derived from the bright band signature of melting layer of radar reflectivity profile, is found to be variable between the heights 4600 m and 5200 m. The change in the nature of rain, classified on the basis of radar reflectivity, is also observed through the MRR. It has been found that there are three types of rain, namely, convective, mixed and stratiform rain, prevailing with different vertical rain microstructures, such as, Drop Size Distribution (DSD), mean drop size, rain rate, liquid water content and average fall speed of the drops at different heights. It is observed that the vertical DSD profile is more inhomogeneous for mixed and stratiform type rain than for convective type rain. It is also found that the large number of drops of size <0.5 mm is present in convective rain whereas in stratiform rain, drops concentration is appreciable up to 1 mm. A comparison of measurements taken by ground based Disdrometer and that from the 200 m level obtained from MRR shows good agreement for rain rate and DSD at smaller rain rate values. The results may be useful for understanding rain structures over this region. 相似文献
75.
文章讨论了星载降水测量雷达(SPR)重频设计要求和约束条件,并以GPMKuPR系统参数为例,研究了SPR重频设计的约束条件,提出和分析了几种重频设计方案。仿真结果表明一种自适应重频技术完全满足系统要求,并能获得最多脉冲积累数。 相似文献
76.
叙述分析处理连续波(CW)信号的重要性,并介绍测定CW信号频率特征的方法。讨论了运行载体上的CW信号频率的调制特性和多普勒频移以及侦收系统噪声对测定信号频率的影响。 相似文献
77.
78.
79.
《中国航空学报》2021,34(2):252-264
The technique of imaging a target with a complicated motion using an Inverse Synthetic Aperture Radar (ISAR) system is an effective tool in the field of radar signal processing. After the translational compensation, the received signal reflected from the target can take the form of a multi-component Polynomial Phase Signal (m-PPS), and the high quality ISAR image can be provided via the combination between the estimated parameters of the m-PPS and the Range Instantaneous-Doppler technique (RID). For a target with a high maneuvrability, the occurrence of scatterers Migration Through Resolution Cell (MTRC), caused by the rotational movement could be appearing. That is why the variation in the amplitude of the echo during the time of observation cannot be neglected. The purpose of this study is the parameters estimation of the m-PPS signal with order three in the case of the Time Varying Amplitude (TVA). The Improved-version of the Product High-order Ambiguity Function (IPHAF) with TVA is proposed to improve the quality of the ISAR image compared with traditional techniques based on a constant amplitude; the experimental outcomes confirm that the new IPHAF-TVA method presented in this study is an effective technique to make the ISAR image very clear. 相似文献
80.
基于分层介质模型的HF雷达高度计火星回波仿真研究 总被引:1,自引:0,他引:1
火星次表层中的水探测是当前深空探测领域中的热门问题之一. 高频(HF)雷达高度计具有较强的穿透能力, 且能同时实现距离和功率测量, 是火星次表层探测的重要手段. 介绍了高频雷达高度计系统的原理和设计, 通过分析高度计电磁脉冲与多层光滑介质之间的相互作用, 得出其回波功 率随时间变化的模型, 并考虑了表面粗糙度对表面回波功率的影响. 选用典型的火星分层介质模型, 对其介电常数特性和高度计回波波形 进行了仿真. 仿真结果表明, 采用高频雷达高度计系统可实现对火星次表 层介电特性垂直廓线的反演, 对火星中水的识别具有重要 作用. 相似文献