全文获取类型
收费全文 | 931篇 |
免费 | 193篇 |
国内免费 | 149篇 |
专业分类
航空 | 616篇 |
航天技术 | 218篇 |
综合类 | 174篇 |
航天 | 265篇 |
出版年
2024年 | 5篇 |
2023年 | 20篇 |
2022年 | 34篇 |
2021年 | 38篇 |
2020年 | 47篇 |
2019年 | 37篇 |
2018年 | 33篇 |
2017年 | 34篇 |
2016年 | 22篇 |
2015年 | 48篇 |
2014年 | 57篇 |
2013年 | 58篇 |
2012年 | 62篇 |
2011年 | 66篇 |
2010年 | 75篇 |
2009年 | 68篇 |
2008年 | 48篇 |
2007年 | 68篇 |
2006年 | 56篇 |
2005年 | 59篇 |
2004年 | 29篇 |
2003年 | 21篇 |
2002年 | 20篇 |
2001年 | 34篇 |
2000年 | 26篇 |
1999年 | 32篇 |
1998年 | 21篇 |
1997年 | 20篇 |
1996年 | 32篇 |
1995年 | 17篇 |
1994年 | 12篇 |
1993年 | 12篇 |
1992年 | 11篇 |
1991年 | 10篇 |
1990年 | 15篇 |
1989年 | 12篇 |
1988年 | 5篇 |
1987年 | 6篇 |
1986年 | 1篇 |
1984年 | 2篇 |
排序方式: 共有1273条查询结果,搜索用时 15 毫秒
981.
纳米光催化技术在客机座舱空气质量控制中的应用 总被引:1,自引:0,他引:1
纳米光催化技术是一种新型的空气净化技术,近年来已成为空气净化领域的研究热点之一。本文简要介绍了纳米光催化技术的发展历史、净化机理以及国内外的研究进展;分析了实际应用中存在的问题;并指出了纳米光催化技术在客机座舱空气质量控制中的应用前景。 相似文献
982.
983.
针对常规时频分析方法对多分量雷达信号分析的不足,提出一种基于神经网络的时频域多分量雷达信号调制参数估计新方法.把多分量雷达信号的时频分布作为灰度图像,通过神经网络训练得到高分辨率时频平面图,然后在时频域实现雷达信号各分量的调制参数估计,相对于时频重排等方法,其对时频分布的处理不需要关于各分量信号的先验知识.仿真实验表明,该方法在得到比时频重排方法更高分辨率时频图的基础上,能够较准确地估计各分量雷达信号调制参数. 相似文献
984.
985.
Qiang Xu Xiaohu Fan Ai Gang Zhao Hongliang Cui Liguo Xu Ning Liu Bangping Ding 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(1):583-596
In order to shorten the data update period and further improve the accuracy, a pre-correction X-ray pulsar navigation algorithm based on asynchronous overlapping observation method is proposed. The asynchronous overlapping observation method partially overlaps the two adjacent observation periods, so that the data update period depends on the minimum pulsar observation period rather than the maximum like the other algorithms. The number of sampling points is also reduced to 2, which will effectively reduce the calculation burden. The proposed pre-correction extended Kalman filter uses observation data of adjacent sampling points to achieve a two-fold correction and makes up for the problem of insufficient observations on some sampling points caused by the observation method. Finally, simulations show that the proposed algorithm reduces the position and velocity errors by 21.55% and 19.13% compared to the EKF based on asynchronous observation method when using three detectors to observe the corresponding pulsars simultaneously. At the same time, the running time of one data update calculation is only 6.6% more than that of the EKF algorithm based on synchronous observation method. 相似文献
986.
987.
988.
A MARS-based method for estimating regional 2-D ionospheric VTEC and receiver differential code bias
Szu-Pyng Kao Yao-Chung Chen Fang-Shii Ning 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The geometry-free linear combination of dual-frequency GNSS reference station ground observations are currently used to build the Vertical Total Electron Content (VTEC) model of the ionosphere. As it is known, besides ionospheric delays, there are differential code bias (DCB) of satellite (SDCB) and receiver (RDCB) in the geometry-free observation equation. The SDCB can be obtained using the International GNSS Service (IGS) analysis centers, but the RDCB for regional and local network receivers are not provided. Therefore, estimating the RDCB and VTEC model accurately and simultaneously is a critical factor investigated by researchers. This study uses Multivariate Adaptive Regression Splines (MARS) to estimate the VTEC approximate model and then substitutes this model in the observation equation to form the normal equation. The least squares method is used to solve the RDCB and VTEC model together. The research findings show that this method has good modeling effectiveness and the estimated RDCB has good reliability. The estimated VTEC model applied to GPS single-frequency precise point positioning has better positioning accuracy in comparison to the IGS global ionosphere map (GIM). 相似文献
989.
Reconstruction of 3D surface irradiance distribution using multiple views captured by charged coupled device(CCD)camera is the basis of solving the light source in bioluminescence tomography(BLT).A simple and convenient mapping technique based on the pin-hole imaging model and Lambert′s cosine law was presented to establish the relationship between gray levels and irradiance intensities.Compared with previous integrating sphere camera calibration used in BLT,the proposed method can effectively avoid heavy burden of simulation experiment to obtain the corresponding relationship of gray levels and irradiance intensities.The accuracy and feasibility of the proposed method are validated with no more than 1mm location error by different types of phantom experiments.The mapping approach is also applicable to other noncontact optical imaging system. 相似文献
990.
Xiukuan Zhao Baiqi Ning Libo Liu Gangbing Song 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
In this paper, the AdaBoost-BP algorithm is used to construct a new model to predict the critical frequency of the ionospheric F2-layer (foF2) one hour ahead. Different indices were used to characterize ionospheric diurnal and seasonal variations and their dependence on solar and geomagnetic activity. These indices, together with the current observed foF2 value, were input into the prediction model and the foF2 value at one hour ahead was output. We analyzed twenty-two years’ foF2 data from nine ionosonde stations in the East-Asian sector in this work. The first eleven years’ data were used as a training dataset and the second eleven years’ data were used as a testing dataset. The results show that the performance of AdaBoost-BP is better than those of BP Neural Network (BPNN), Support Vector Regression (SVR) and the IRI model. For example, the AdaBoost-BP prediction absolute error of foF2 at Irkutsk station (a middle latitude station) is 0.32 MHz, which is better than 0.34 MHz from BPNN, 0.35 MHz from SVR and also significantly outperforms the IRI model whose absolute error is 0.64 MHz. Meanwhile, AdaBoost-BP prediction absolute error at Taipei station from the low latitude is 0.78 MHz, which is better than 0.81 MHz from BPNN, 0.81 MHz from SVR and 1.37 MHz from the IRI model. Finally, the variety characteristics of the AdaBoost-BP prediction error along with seasonal variation, solar activity and latitude variation were also discussed in the paper. 相似文献