全文获取类型
收费全文 | 373篇 |
免费 | 22篇 |
国内免费 | 24篇 |
专业分类
航空 | 39篇 |
航天技术 | 339篇 |
综合类 | 13篇 |
航天 | 28篇 |
出版年
2024年 | 2篇 |
2023年 | 8篇 |
2022年 | 6篇 |
2021年 | 20篇 |
2020年 | 18篇 |
2019年 | 16篇 |
2018年 | 17篇 |
2017年 | 1篇 |
2016年 | 4篇 |
2015年 | 6篇 |
2014年 | 35篇 |
2013年 | 41篇 |
2012年 | 18篇 |
2011年 | 46篇 |
2010年 | 26篇 |
2009年 | 43篇 |
2008年 | 39篇 |
2007年 | 4篇 |
2006年 | 8篇 |
2005年 | 5篇 |
2004年 | 6篇 |
2003年 | 2篇 |
2002年 | 5篇 |
2001年 | 3篇 |
2000年 | 6篇 |
1999年 | 2篇 |
1998年 | 4篇 |
1997年 | 6篇 |
1996年 | 1篇 |
1995年 | 2篇 |
1994年 | 3篇 |
1993年 | 6篇 |
1992年 | 4篇 |
1991年 | 1篇 |
1990年 | 2篇 |
1988年 | 1篇 |
1987年 | 1篇 |
1986年 | 1篇 |
排序方式: 共有419条查询结果,搜索用时 187 毫秒
31.
中俄联合火星电离层星-星掩星探测 总被引:1,自引:0,他引:1
孙越强 杜起飞 朱光武 吴季 陶鹏 白伟华 赵华 胡雄 吴小成 郑建华 A S Kosov T K Breus V M Gotlib A M Krymskii A V Zakharov 《空间科学学报》2009,(5)
中俄联合火星星-星掩星探测是人类首次在火星空间环境进行此类的联合试验。用于探测火星电离层的星-星掩星技术较以前星地间的探测技术相比,有可接收高信噪比信号,反演精度高,可探测火星上太阳天顶角大于43°,或者小于138°的区域电离层等优点。本文介绍了中俄联合火星星-星掩星探测方案、基本原理,给出了主要技术指标、地面模拟测试结果。 相似文献
32.
33.
对校正天波超视距雷达电离层相位污染的五种典型方法进行了综合性能评估,主要从校正效果、对不同污染的普适性、污染参数变化对方法的影响、信噪比对方法性能的影响、运算量等几个方面进行了比较与分析,为实际工程实现和改进电离层相位污染校正方法提供参考。 相似文献
34.
35.
36.
日照边缘区域电离层对耀斑的响应特点研究 总被引:1,自引:1,他引:0
利用MSIS模型和背景太阳辐射谱模型,在一定大耀斑辐射谱假设的前提下,计算了耀斑期间日照边缘区域的电子产生率,分析了这一区域电离层电子密度的变化特点.结果表明,大耀斑期间在日照边缘区域,甚至大于太阳天顶角90°的区域都有明显的电子产生率的增加.从不同太阳天顶角处的电子产生率剖面的形态来看,随着天顶角的增加最大电离率减少,但高度增加.计算还显示了在太阳天顶角小于90°的区域内电子产生率的垂直分布有明显的双峰结构,这种结构对应着电离层的E区和F区,但在天顶角大于90°区域,F区的电子产生率要大得多.考虑到离子和电子的复合过程,这一区域的总电子含量的增加主要产生在高F区. 相似文献
37.
广播式自动相关监视(ADS-B)作为机载综合监视系统(ISS)的新增重要组成部分,在保证飞机飞行安全的前提下,在监视成本和效率方面展现出优势,引领了未来监视技术的发展。本文首先介绍了ADS-B系统功能与优劣势,梳理了国内外技术和产品现状;然后从保障飞行安全和高效的角度出发,分析和综述了机载ISS中ADS-B的关键技术,并详细阐述了技术内涵及难点;最后结合下一代空域运行理念,探讨和展望了技术发展趋势,提出了4个ADS-B技术的未来发展方向,为推动ADS-B技术在实际运行与理论研究方面的发展提供参考。 相似文献
38.
Fanfan Su Zhengyu ZhaoFeng Deng Shipeng Li 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The high frequency management system with backscatter radar supplies the real time ionosphere channel conditions to high frequency users, which leads to the demand for the ground range between the radar location and the scatters on the distant ground. The ionosphere electron density profile is usually inversed to obtain the ground range. An inversion algorithm, with which the ground range on the leading edge of the backscatter ionograms can be obtained without electron density, is presented in this paper. The ray path geometry of the backscatter sounding and the change in the group path on the leading edge with operating frequency are used to derive the ground range. Synthesized backscatter ionogram and experimental backscatter ionograms are processed to validate the algorithm. The results indicate that the algorithm is usable for high frequency management system. 相似文献
39.
Kh. Karami S. Ghader A. Raeen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
In the present work values of peak electron density (NmF2) and height of F2 ionospheric layer (hmF2) over Tehran region at a low solar activity period are compared with the predictions of the International Reference Ionosphere models (IRI-2001 and IRI-2007). Data measured by a digital ionosonde at the ionospheric station of the Institute of Geophysics, University of Tehran from July 2006 to June 2007 are used to perform the calculations. Formulations proposed by and are utilized to calculate the hmF2. The International Union of Radio Science (URSI) and International Radio Consultative Committee (CCIR) options are employed to run the IRI-2001 and IRI-2007 models. Results show that both IRI-2007 and IRI-2001 can successfully predict the NmF2 and hmF2 over Tehran region. In addition, the study shows that predictions of IRI-2007 model with CCIR coefficient has closer values to the observations. Furthermore, it is found that the monthly average of the percentage deviation between the IRI models predictions and the values of hmF2 and NmF2 parameters are less than 10% and 21%, respectively. 相似文献
40.
Janusz Mlynarczyk Piotr Koperski Andrzej Kulak 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012,49(1):83-88
The Digital Radio Mondiale (DRM), one of the new digital radio broadcasting standards, has been designed to overcome typical short wave radio channel difficulties, such as the multipath propagation and fast temporal changes of the received signal level, both related to the properties of the ionosphere along the path of propagation. In particular, some of the RF carriers used in the applied COFDM transmission technique serve to estimate the current state of the radio channel to enable the proper demodulation of the received signal.We have been detecting such RF carriers on select frequency channels (standard DRM broadcast) using a network of recording stations located in different parts of Poland in order to collect data on the HF radio channel. We have been also evaluating the usefulness of this procedure in providing information on the current state of the ionosphere in the refraction region between the transmitter and receivers. When the DRM system becomes more widespread, this method can supplement data that comes from the ionosondes, since it does not require much financial resources and the receivers can be easily scattered over a large area. This paper presents a set of experimental data and its analysis. 相似文献