全文获取类型
收费全文 | 731篇 |
免费 | 77篇 |
国内免费 | 31篇 |
专业分类
航空 | 334篇 |
航天技术 | 217篇 |
综合类 | 34篇 |
航天 | 254篇 |
出版年
2024年 | 5篇 |
2023年 | 23篇 |
2022年 | 22篇 |
2021年 | 19篇 |
2020年 | 17篇 |
2019年 | 13篇 |
2018年 | 12篇 |
2017年 | 15篇 |
2016年 | 15篇 |
2015年 | 21篇 |
2014年 | 22篇 |
2013年 | 25篇 |
2012年 | 41篇 |
2011年 | 66篇 |
2010年 | 22篇 |
2009年 | 24篇 |
2008年 | 35篇 |
2007年 | 36篇 |
2006年 | 37篇 |
2005年 | 49篇 |
2004年 | 27篇 |
2003年 | 43篇 |
2002年 | 23篇 |
2001年 | 33篇 |
2000年 | 26篇 |
1999年 | 32篇 |
1998年 | 21篇 |
1997年 | 20篇 |
1996年 | 15篇 |
1995年 | 14篇 |
1994年 | 12篇 |
1993年 | 8篇 |
1992年 | 8篇 |
1991年 | 13篇 |
1990年 | 7篇 |
1989年 | 7篇 |
1988年 | 6篇 |
1987年 | 5篇 |
排序方式: 共有839条查询结果,搜索用时 421 毫秒
321.
《中国航空学报》2021,34(2):124-135
The target of this paper is the performance-based diagnostics of a gas turbine for the automated early detection of components malfunctions. The paper proposes a new combination of multiple methodologies for the performance-based diagnostics of single and multiple failures on a two-spool engine. The aim of this technique is to combine the strength of each methodology and provide a high success rate for single and multiple failures with the presence of measurement malfunctions. A combination of KF (Kalman Filter), ANN (Artificial Neural Network) and FL (Fuzzy Logic) is used in this research in order to improve the success rate, to increase the flexibility and the number of failures detected and to combine the strength of multiple methods to have a more robust solution. The Kalman filter has in his strength the measurement noise treatment, the artificial neural network the simulation and prediction of reference and deteriorated performance profile and the fuzzy logic the categorization flexibility, which is used to quantify and classify the failures. In the area of GT (Gas Turbine) diagnostics, the multiple failures in combination with measurement issues and the utilization of multiple methods for a 2-spool industrial gas turbine engine has not been investigated extensively.This paper reports the key contribution of each component of the methodology and brief the results in the quantification and classification success rate. The methodology is tested for constant deterioration and increasing noise and for random deterioration. For the random deterioration and nominal noise of 0.4%, in particular, the quantification success rate is above 92.0%, while the classification success rate is above 95.1%. Moreover, the speed of the data processing (1.7 s/sample) proves the suitability of this methodology for online diagnostics. 相似文献
322.
针对微波无线功率传输对于高功率处理能力的高效整流器需求,提出一种基于高效率功率放大器的功放-整流一体化设计思路。文章首先使用型号为CG2H40010F的氮化镓高电子迁移率晶体管(GaN HEMT),通过谐波控制、负载牵引等方法,设计出一款工作在2.45GHz逆F类高效率功率放大器。在高效率功率放大器的基础上基于时间反转对偶理论,通过改变逆F类功率放大器电流方向,同时结合耦合器和移相器实现了高功率容量整流电路的设计。仿真结果表明,在245GHz工作频率下,功率放大器的输入功率为28dBm时,功率附加效率达到76%,输出功率40dBm;整流电路的输入功率为41dBm时,RF-DC转换效率可达到79%,整流最佳效率大于80%,显示了整流器的高功率处理能力。引入了两个单刀双掷开关实现功率放大器和整流器的功能切换,文章对核心电路功率放大器进行了实物测试,测试结果与仿真重合较好,验证了功放-整流一体化设计的可行性。 相似文献
323.
S.V. Vadawale M. Shanmugam Y.B. Acharya A.R. Patel S.K. Goyal B. Shah A.K. Hait A. Patinge D. Subrahmanyam 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The remote X-ray fluorescence spectroscopy is a powerful technique to investigate the elemental abundances in the atmosphere-less planetary bodies. The experiment involves measuring spectra of fluorescent X-rays from lunar surface using a low energy X-ray detector onboard an orbiting satellite. Since the flux of fluorescent X-ray lines critically depend on the flux and spectrum of the incident solar X-rays, it is essential to have simultaneous and accurate measurement of X-ray from both Moon and Sun. In the context of Moon, this technique has been employed since early days of space exploration to determine elemental composition of lunar surface. However, so far it has not been possible to exploit it to its full potential due to various reasons. Therefore it is planned to continue the remote X-ray fluorescence spectroscopy experiment on-board Chandrayaan-2 which includes both lunar X-ray observations and solar X-ray observations as two separate payloads. The lunar X-ray observations will be carried out by Chandra Large Area Soft x-ray Spectrometer (CLASS) experiment; whereas the solar X-ray observations will be carried out by a separate payload, Solar X-ray Monitor (XSM). Here we present the overall design of the XSM instrument, the present development status as well as preliminary results of the laboratory model testing. XSM instrument will have two packages namely – XSM sensor package and XSM electronics package. XSM will accurately measure spectrum of Solar X-rays in the energy range of 1–15 keV with energy resolution ∼200 eV @ 5.9 keV. This will be achieved by using state-of-the-art Silicon Drift Detector (SDD), which has a unique capability of maintaining high energy resolution at very high incident count rate expected from Solar X-rays. XSM onboard Chandrayaan-2 will be the first experiment to use such detector for Solar X-ray monitoring. 相似文献
324.
325.
326.
327.
328.
329.
330.