全文获取类型
收费全文 | 270篇 |
免费 | 43篇 |
国内免费 | 9篇 |
专业分类
航空 | 127篇 |
航天技术 | 168篇 |
综合类 | 4篇 |
航天 | 23篇 |
出版年
2023年 | 10篇 |
2022年 | 6篇 |
2021年 | 10篇 |
2020年 | 8篇 |
2019年 | 12篇 |
2018年 | 9篇 |
2017年 | 11篇 |
2016年 | 7篇 |
2015年 | 6篇 |
2014年 | 20篇 |
2013年 | 24篇 |
2012年 | 20篇 |
2011年 | 21篇 |
2010年 | 13篇 |
2009年 | 29篇 |
2008年 | 12篇 |
2007年 | 10篇 |
2006年 | 6篇 |
2005年 | 20篇 |
2004年 | 6篇 |
2003年 | 11篇 |
2002年 | 2篇 |
2001年 | 3篇 |
2000年 | 4篇 |
1999年 | 4篇 |
1998年 | 5篇 |
1997年 | 6篇 |
1996年 | 2篇 |
1995年 | 2篇 |
1994年 | 8篇 |
1993年 | 4篇 |
1992年 | 3篇 |
1991年 | 4篇 |
1990年 | 1篇 |
1989年 | 1篇 |
1987年 | 2篇 |
排序方式: 共有322条查询结果,搜索用时 78 毫秒
41.
针对网络线缆分析仪插入损耗的校准,本文采用插入法和替代法分别进行了校准实验,并通过数据分析比较两种方法对测试结果的影响,得出了选用替代法校准更为适宜的结论。对替代法测试数据进行不确定度评定分析,证明了本文选用替代法能达到校准网络线缆分析仪插入损耗的要求。 相似文献
42.
研究防静电Kapton二次表面镜(ITO/Kapton/Al)、S781白漆两种典型热控涂层,在不同能量电子辐照后太阳吸收比退化情况,并利用X射线光电子能谱和扫描电子显微镜对样品表面的成分和形貌进行了分析。结果表明:相同电子注量下,不同能量电子对样品的太阳吸收比退化作用程度是有区别的。而样品光谱反射率、表面形貌、表面成分的损伤效应类似,说明不同能量电子辐照下,样品的退化机理是一致的。 相似文献
43.
硅化物涂层电子束重熔表面改性技术 总被引:1,自引:0,他引:1
在Nb521铌合金表面采用料浆烧结法制备硅化物涂层,利用高频扫描电子束对硅化物涂层进行重熔处理,通过扫描电子显微镜对处理样品表面形貌进行组织结构分析。研究表明,经过电子束重熔处理,硅化物涂层表面陶瓷晶粒粒度降低,表面粗糙度降低,陶瓷颗粒之间烧结作用增强,重熔区域与未处理区域具有明显的边界,电子束能量分布较均匀,电子束重熔提高了硅化物涂层的抗氧化性能和抗热震性能。 相似文献
44.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(6):2759-2769
In this study, predictions of the E-CHAIM ionospheric model are compared with measurements by the incoherent scatter radars RISR at Resolute Bay, Canada, in the northern polar cap. Reasonable coverage was available for all seasons except winter for which no conclusions were drawn. It is shown that ratios of the model-to measured electron densities are close to unity in the central part of the F layer, around its peak. This is particularly evident for summer daytime. Distributions of the ratios are wider for other seasons indicating larger number of cases when the model underestimates or overestimates. E-CHAIM underestimates the electron density at ionospheric topside and bottomside by ~ 10–20 %. At the bottomside, the underestimations are strongest in summer and equinoctial nighttime. At the topside, the underestimations are strongest in autumn nighttime. Model overestimations are noticeable in the middle part of the F layer during dawn hours in autumn. Overall, the model tends to not predict highest-observed peak electron densities and the largest-observed heights of the peak. 相似文献
45.
M. Pezzopane M. Pietrella A. Pignatelli B. Zolesi Lj.R. Cander 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
This paper describes the three-dimensional (3-D) electron density mapping of the ionosphere given as output by the assimilative IRI-SIRMUP-P (ISP) model for three different geomagnetic storms. Results of the 3-D model are shown by comparing the electron density profiles given by the model with the ones measured at two testing ionospheric stations: Roquetes (40.8°N, 0.5°E), Spain, and San Vito (40.6°N, 17.8°E), Italy. The reference ionospheric stations from which the autoscaled foF2 and M(3000)F2 data as well as the real-time vertical electron density profiles are assimilated by the ISP model are those of El Arenosillo (37.1°N, 353.3°E), Spain, Rome (41.8°N, 12.5°E), and Gibilmanna (37.9°N, 14.0°E), Italy. Overall, the representation of the ionosphere made by the ISP model is better than the climatological representation made by only the IRI-URSI and the IRI-CCIR models. However, there are few cases for which the assimilation of the autoscaled data from the reference stations causes either a strong underestimation or a strong overestimation of the real conditions of the ionosphere, which is in these cases better represented by only the IRI-URSI model. This ISP misrepresentation is mainly due to the fact that the reference ionospheric stations covering the region mapped by the model turn out to be few, especially for disturbed periods when the ionosphere is very variable both in time and in space and hence a larger number of stations would be required. The inclusion of new additional reference ionospheric stations could surely smooth out this concern. 相似文献
46.
47.
48.
P.L. Saranya K. VenkateshD.S.V.V.D. Prasad P.V.S. Rama RaoK. Niranjan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The pre-storm behavior of NmF2 and TEC over an equatorial station, Trivandrum (8.47°N, 76.91°E, dip 0.6°S) and a low latitude station, Waltair (17.7°N,83.3°E, dip 20°N) has been studied for a total of 18 strong geomagnetic storms with DST ? −100 nT. The simultaneous measurements of GPS-TEC and NmF2 over Trivandrum and Waltair during the period 2000–2005 have been considered for the present study. It is found that there is a substantial increase in NmF2 and TEC before the onset of the storm over Waltair, while the increase is not present at Trivandrum. The origin of pre-storm enhancements in electron density still remains unresolved owing to several conditions in their potential sources and occurrence mechanisms. In the present study an attempt is made to identify the possible mechanisms responsible for such enhancements in electron density of the F-region. 相似文献
49.
电子回旋共振推力器放电室内磁场与微波电磁场分析 总被引:2,自引:0,他引:2
电子回旋共振推力器具有寿命长、比冲高、结构简单等特点,适宜用作深空探测器主推进装置。放电室是电子回旋共振推力器的关键部件,其作用是产生电子回旋共振等离子体。放电室内的磁场和微波电磁场分布对于推力器的可靠启动、稳定工作有着重要的影响。为此针对10cm推力器,采用大型有限元分析软件ANSYS建立了三种磁路模型,计算了放电室内的磁场分布,得出三种方案中电子回旋共振面的位置,分析放电室材料不同时磁场分布的变化;最后采用ANSYS有限元分析软件计算了放电室内的电磁场分布。结果表明,在电子回旋共振面上微波能量满足放电所需能量。计算结果可以为电子回旋共振推力器放电室的设计提供帮助。 相似文献
50.
数字调制信号误差矢量幅度校准研究 总被引:1,自引:0,他引:1
从计量领域的现状看,对于矢量信号分析仪的误差矢量幅度,分析其准确度尚没有业内统一的方法。通过对数字调制信号的调制过程和解调过程的分析,罗列出影响误差矢量幅度的各种因素。在此基础上,总结出一套对误差矢量幅度的测量结果的理论计算方法,从而提出一种EVM测量结果的不确定度评定方法。此方法能够有效地分析误差矢量幅度的数字特性。 相似文献