全文获取类型
收费全文 | 5552篇 |
免费 | 1398篇 |
国内免费 | 891篇 |
专业分类
航空 | 4040篇 |
航天技术 | 1238篇 |
综合类 | 767篇 |
航天 | 1796篇 |
出版年
2024年 | 22篇 |
2023年 | 91篇 |
2022年 | 222篇 |
2021年 | 260篇 |
2020年 | 255篇 |
2019年 | 187篇 |
2018年 | 189篇 |
2017年 | 253篇 |
2016年 | 219篇 |
2015年 | 296篇 |
2014年 | 345篇 |
2013年 | 380篇 |
2012年 | 459篇 |
2011年 | 447篇 |
2010年 | 473篇 |
2009年 | 465篇 |
2008年 | 392篇 |
2007年 | 375篇 |
2006年 | 361篇 |
2005年 | 255篇 |
2004年 | 172篇 |
2003年 | 186篇 |
2002年 | 208篇 |
2001年 | 196篇 |
2000年 | 154篇 |
1999年 | 180篇 |
1998年 | 121篇 |
1997年 | 110篇 |
1996年 | 111篇 |
1995年 | 74篇 |
1994年 | 83篇 |
1993年 | 49篇 |
1992年 | 59篇 |
1991年 | 47篇 |
1990年 | 47篇 |
1989年 | 41篇 |
1988年 | 23篇 |
1987年 | 18篇 |
1986年 | 7篇 |
1985年 | 3篇 |
1983年 | 1篇 |
1982年 | 1篇 |
1981年 | 1篇 |
1979年 | 1篇 |
1965年 | 1篇 |
1900年 | 1篇 |
排序方式: 共有7841条查询结果,搜索用时 15 毫秒
1.
2.
Yi Wei Qingjun Li Fangnuan Xu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(1):393-400
A new orbit-attitude-vibration coupled dynamic model of the tethered solar power satellite (Tethered SPS) is established based on absolute nodal coordinate formulation. The Hamilton’s equation of the system is derived by introducing generalized momentum through Legendre transformation. The correctness of the proposed model is verified by an example. The dynamic characteristics of the Tethered SPS are studied using the symplectic Runge-Kutta method. Simulation results show that the orbital radius and the total energy of the system are well preserved. The attitude of the system is unstable when the mass of the bus system is small. However, the attitude stability is dependent on some other parameters of the system, which requires further studies. It is also found that the average tether force/deformation can be roughly estimated by simplifying the solar panel as a particle. The proposed model can be used to study the orbit-attitude-vibration coupled dynamics and control problems. 相似文献
3.
Yongjie Ding Jia Boyang Hezhi Sun Liqiu Wei Wuji Peng Peng Li Daren Yu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(3):837-843
Discharge characteristics of a non-wall-loss Hall thruster were studied under different channel lengths using a design based on pushing a magnetic field through a double permanent magnet ring. The effect of different magnetic field intensities and channel lengths on ionization, efficiency, and plume divergence angle were studied. The experimental results show that propellant utilization is improved for optimal matching between the magnetic field and channel length. While matching the magnetic field and channel length, the ionization position of the neutral gas changes. The ion flow is effectively controlled, allowing the thrust force, specific impulse, and efficiency to be improved. Our study shows that the channel length is an important design parameter to consider for improving the performance of non-wall-loss Hall thrusters. 相似文献
4.
X.B. Zhao W.Z. Shao L.B. Zhao Y. Gao Y.Y. Hu X.Z. Yuan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(10):3072-3086
The main objective of our work was to investigate the impact of rain on wave observations from C-band (~5.3 GHz) synthetic aperture radar (SAR) in tropical cyclones. In this study, 10 Sentinel-1 SAR images were available from the Satellite Hurricane Observation Campaign, which were taken under cyclonic conditions during the 2016 hurricane season. The third-generation wave model, known as Simulating WAves Nearshore (SWAN) (version 41.31), was used to simulate the wave fields corresponding to these Sentinel-1 SAR images. In addition, rainfall data from the Tropical Rainfall Measuring Mission satellite passing over the spatial coverage of the Sentinel-1 SAR images were collected. The simulated results were validated against significant wave heights (SWHs) from the Jason-2 altimeter and European Centre for Medium-Range Weather Forecasts data, revealing a root mean square error (RMSE) of ~0.5 m with a 0.25 scatter index. Winds retrieved from the VH-polarized Sentinel-1 SAR images using the Sentinel-1 Extra Wide-swath Mode Wind Speed Retrieval Model after Noise Removal were taken as prior information for wave retrieval. It was discovered that rain did indeed affect the SAR wave retrieval, as evidenced by the 3.21-m RMSE of SWHs between the SAR images and the SWAN model, which was obtained for the ~1000 match-ups with raindrops. The raindrops dampened the wave retrieval when the rain rate was < ~5 mm/hr; however, they enhanced wave retrieval for higher rain rates. It was also found that the portion of the rain-induced ring wave with a wave number > 0.05 rad/m (~125 m wavelength) was clearly observed in the SAR-derived wave spectra. 相似文献
5.
量子科学实验卫星在轨运行期间完成4种光学实验,地面监测人员通过遥测参数阈值判断卫星是否进行光学实验、实验类型及实验结果.这种方法需要预先设定大量阈值,并且这些阈值需要根据在轨卫星重新设定,可扩展性较差.针对以上问题,提出一种基于机器学习的光学实验判别方法,将量子科学实验卫星的光学实验监测任务抽象为机器学习中的多元分类问题,构建分类模型,利用量子科学实验卫星的真实历史遥测数据对模型进行训练,并通过真实实验计划对训练得到的模型进行验证.实验结果表明,本文提出的方法在没有专家先验知识的前提下,判别准确率达到99%,可用于量子科学实验卫星光学实验的实时监测任务.提出的基于机器学习的判别方法具有较强的可扩展性,可应用于卫星在轨运行的其他监测任务. 相似文献
6.
针对拦截高速目标的作战特点,分析了比例导引(PN)与反比例导引(RPN)的捕获区。首先,通过分析拦截弹与目标的相对运动关系,推导得到了顺轨和逆轨的零控拦截条件,此条件由目标和拦截弹的速度前置角以及二者速度比确定;其次,以拦截弹和目标速度前置角为坐标系,推导得到了PN以及RPN捕获区以及各自导航比设置范围。PN的捕获区由逆轨零控拦截条件以及与其相切且斜率为1/(N-1)的两条直线构成,RPN的捕获区由顺轨零控拦截条件以及与其相切且斜率为1/(-N-1)的两条直线构成;然后,利用函数对称性将PN与RPN捕获区转换到同一坐标区间,得到了相同条件下RPN捕获区要大于PN捕获区的结论;最后,开展了四种情形下的仿真,验证了本文捕获区分析的合理性及有效性。 相似文献
7.
An improved numerical method that can construct Halo/Lissajous orbits in the vicinity of collinear libration points in a full solar system model is investigated. A full solar system gravitational model in the geocentric rotating coordinate system with a clear presentation of the angular velocity relative to the inertial coordinate system is proposed. An alternative way to determine patch points in the multiple shooting method is provided based on a dynamical analysis with Poincare′sections. By employing the new patch points and sequential quadratic programming, Halo orbits for L_1, L_2, and L_3 points as well as Lissajous orbits for L_1 and L_2 points in the EarthMoon system are generated with the proposed full solar system gravitational model to verify the effectiveness of the proposed method. 相似文献
8.
Pengbin Guo Jian Sun Shuling Hu Ju Xue 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(3):787-798
Pulsar navigation is a promising navigation method for high-altitude orbit space tasks or deep space exploration. At present, an important reason for restricting the development of pulsar navigation is that navigation accuracy is not high due to the slow update of the measurements. In order to improve the accuracy of pulsar navigation, an asynchronous observation model which can improve the update rate of the measurements is proposed on the basis of satellite constellation which has a broad space for development because of its visibility and reliability. The simulation results show that the asynchronous observation model improves the positioning accuracy by 31.48% and velocity accuracy by 24.75% than that of the synchronous observation model. With the new Doppler effects compensation method in the asynchronous observation model proposed in this paper, the positioning accuracy is improved by 32.27%, and the velocity accuracy is improved by 34.07% than that of the traditional method. The simulation results show that without considering the clock error will result in a filtering divergence. 相似文献
9.
在机器人自动制孔过程中,制孔点位信息通常从待制孔工件工艺数模上获取,而待制孔工件安装过程中会出现位置偏移和变形,由工艺数模得到的点位信息无法直接满足孔位精度要求。为了保证自动制孔的孔位精度,提出了一种基于遗传算法的插值Coons曲面孔位修正方法。利用制孔区域边角基准孔建立双线性Coons误差曲面模型,通过模型计算出待制孔的误差补偿向量,并补偿至理论制孔位置。针对误差曲面切矢模长无法确定的情况,利用制孔区域内的基准孔构建遗传算法模型,计算出切矢模长最优值,使拟合的误差曲面更符合实际制孔区域曲面。通过试验对算法的有效性和精度进行验证,结果表明:采用基于遗传算法的插值Coons曲面孔位修正方法,可以使孔位误差得到有效的补偿。补偿后的平均孔位误差仅为0.195 6 mm,与传统的插值曲面方法相比,孔位误差降低了5%~10%。 相似文献
10.