全文获取类型
收费全文 | 1048篇 |
免费 | 187篇 |
国内免费 | 215篇 |
专业分类
航空 | 492篇 |
航天技术 | 488篇 |
综合类 | 53篇 |
航天 | 417篇 |
出版年
2024年 | 12篇 |
2023年 | 26篇 |
2022年 | 38篇 |
2021年 | 59篇 |
2020年 | 63篇 |
2019年 | 58篇 |
2018年 | 57篇 |
2017年 | 50篇 |
2016年 | 60篇 |
2015年 | 67篇 |
2014年 | 85篇 |
2013年 | 64篇 |
2012年 | 72篇 |
2011年 | 114篇 |
2010年 | 82篇 |
2009年 | 62篇 |
2008年 | 70篇 |
2007年 | 63篇 |
2006年 | 58篇 |
2005年 | 58篇 |
2004年 | 45篇 |
2003年 | 33篇 |
2002年 | 23篇 |
2001年 | 26篇 |
2000年 | 26篇 |
1999年 | 16篇 |
1998年 | 12篇 |
1997年 | 10篇 |
1996年 | 2篇 |
1995年 | 6篇 |
1994年 | 5篇 |
1993年 | 5篇 |
1992年 | 1篇 |
1991年 | 7篇 |
1990年 | 6篇 |
1989年 | 4篇 |
1988年 | 3篇 |
1987年 | 2篇 |
排序方式: 共有1450条查询结果,搜索用时 31 毫秒
821.
822.
基于特征模型的某型无人机智能PID控制器 总被引:2,自引:1,他引:1
无人机的飞行特性在很大程度上取决于其飞行控制律。本文以无人机的姿态控制回路为研究对象,分析了表征该无人机姿态控制特性的特征状态信息。利用特征建模的方法,设计一种基于控制对象特征模型的无人机姿态回路仿人智能P ID控制器,并进行了仿真试验。结果表明,该控制器具有较好的抗干扰和自适应能力,结构简单,针对性强,易于实现。 相似文献
823.
推导出制导火箭弹为获得期望着角所需的脉冲发动机数量解析公式,并根据此公式对比研究了火箭弹分别采用同时点火和依次点火时俯仰角初始值、期望着角和脉冲发动机推力对脉冲发动机数量的影响。研究表明,同时点火方式优于依次点火方式;飞行末段姿态调整时间较长时,期望着角和初始俯仰角对发动机数量的影响很小;随着脉冲推力的增加,所需的脉冲发动机数量递减。 相似文献
824.
传递对准姿态匹配的优化算法 总被引:1,自引:0,他引:1
推导了4种传递对准姿态匹配算法,分析了这4种姿态匹配算法的优缺点,证明并验证了其中的“最优姿态匹配法”在姿态匹配算法中的最优性。首先介绍了传统的“姿态角匹配法”及其改进算法,即“姿态矩阵匹配法”,接着引入了量测失准角的概念,经过理论推导,提出了利用量测失准角进行传递对准姿态匹配的“量测失准角匹配法”。上述3种姿态匹配算法都是在子惯导安装角是小量的条件下推导而获得的,只能适用于安装角是小量的条件,具有一定的局限性。基于此,对“量测失准角匹配法”进行了完善,推导出了一种可在多挂点下使用的现代姿态匹配算法——最优姿态匹配法。从理论上证明了4种姿态匹配算法的相互关系。最后,采用“速度+姿态”匹配方案进行的传递对准仿真结果表明:4种姿态匹配算法具有相同的估计精度;推导的“最优姿态匹配法”在保证精度的同时,可应用于子惯导安装角是任意角度的情况,具有更广的应用范围。 相似文献
825.
作为实现导弹快速机动响应的关键部件,固体姿轨控发动机的性能需要通过动态多分力测试评价,但由于推力测试台结构复杂,对测试数据补偿提出了更高的要求。本文采用双模态阻尼补偿法开展固体姿轨控发动机推力补偿研究,通过脉冲激励试验获得了主要模态参数,并对脉冲激励和发动机冷流试验数据进行补偿,验证了双模态阻尼补偿方法的可行性和应用效果。结果表明:双模态阻尼补偿效果优于单模态补偿,可以有效恢复动态推力信号。所建立的双模态阻尼补偿,在姿轨控发动机研制中得到了应用。 相似文献
826.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(3):978-996
Continuous and timely real-time satellite orbit and clock products are mandatory for real-time precise point positioning (RT-PPP). Real-time high-precision satellite orbit and clock products should be predicted within a short time in case of communication delay or connection breakdown in practical applications. For prediction, historical data describing the characteristics of the real-time orbit and clock can be used as the basis for performing the prediction. When historical data are scarce, it is difficult for many existing models to perform precise predictions. In this paper, a linear regression model is used to predict clock products. Seven-day GeoForschungsZentrum (GFZ) final clock products sampled at 30 s are used to analyze the characteristics of GNSS clocks. It is shown that the linear regression model can be used as the prediction model for the satellite clock products. In addition, the accuracy of the clock prediction for different satellites are analyzed using historical data with different periods (such as 2 and 10 epochs). Experimental results show that the accuracy of the clock with the linear regression prediction model using historical data with 10 epochs is 1.0 ns within 900 s. This is higher accuracy than that achieved using historical data of 2 epochs. Finally, the performance analysis for real-time kinematic precise point positioning (PPP) is provided using GFZ final clock prediction results and state space representation (SSR) clock prediction results when communication delay or connection breakdown occur. Experimental results show that the positioning accuracy without prediction is better than that with prediction in general, whether using the final clock product or the SSR clock product. For the final clock product, the positioning accuracy in the north (N), east (E), and up (U) directions is better than 10.0 cm with all visible GNSS satellites with prediction. In comparison, the 3D positioning accuracy of N, E, and U directions with visible GNSS satellites whose prediction accuracy is better than 0.1 ns using historical data of 10 epochs is improved from 15.0 cm to 7.0 cm. For the SSR clock product, the positioning accuracy of N, E, and U directions is better than 12.0 cm with visible GNSS satellites with prediction. In comparison, the 3D positioning accuracy of N, E, and U directions with visible GNSS satellites whose prediction accuracy is better than 0.1 ns using historical data of 10 epochs is improved from 12.0 cm to 9.0 cm. 相似文献
827.
828.
829.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(1):271-284
Space telescope ultrahigh precision pointing control requires the spacecraft platform to provide an ultra-quiet working environment. Vibration isolator rejection control and the multi-stage integrated control method is believed to be one of the best methods to improve the space telescope attitude control performance. In this paper, the fine dynamics model of multi-stage spacecraft systems is presented and the multi-stage integrated controller design techniques are provided. Effectiveness of the multi-stage integrated control approach is demonstrated by both the numerical simulation and experiment results. An integrated design and demonstrated experimental environment is developed for high-fidelity control performance assessment. The verification experiments for the space telescope attitude control and vibration control are carried out. The results show that the pointing accuracy and stability of the line-of-sight (LOS) for space telescope are improved at least one order by the multi-stage integrated control method. 相似文献
830.
Ernst Schrama 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(1):235-247
In this paper we discuss our efforts to perform precision orbit determination (POD) of CryoSat-2 which depends on Doppler and satellite laser ranging tracking data. A dynamic orbit model is set-up and the residuals between the model and the tracking data is evaluated. The average r.m.s. of the 10?s averaged Doppler tracking pass residuals is approximately 0.39?mm/s; and the average of the laser tracking pass residuals becomes 1.42?cm. There are a number of other tests to verify the quality of the orbit solution, we compare our computed orbits against three independent external trajectories provided by the CNES. The CNES products are part of the CryoSat-2 products distributed by ESA. The radial differences of our solution relative to the CNES precision orbits shows an average r.m.s. of 1.25?cm between Jun-2010 and Apr-2017. The SIRAL altimeter crossover difference statistics demonstrate that the quality of our orbit solution is comparable to that of the POE solution computed by the CNES. In this paper we will discuss three important changes in our POD activities that have brought the orbit performance to this level. The improvements concern the way we implement temporal gravity accelerations observed by GRACE; the implementation of ITRF2014 coordinates and velocities for the DORIS beacons and the SLR tracking sites. We also discuss an adjustment of the SLR retroreflector position within the satellite reference frame. An unexpected result is that we find a systematic difference between the median of the 10 s Doppler tracking residuals which displays a statistically significant pattern in the South Atlantic Anomaly (SSA) area where the median of the velocity residuals varies in the range of ?0.15 to +0.15?mm/s. 相似文献