全文获取类型
收费全文 | 454篇 |
免费 | 48篇 |
国内免费 | 23篇 |
专业分类
航空 | 156篇 |
航天技术 | 175篇 |
综合类 | 40篇 |
航天 | 154篇 |
出版年
2024年 | 4篇 |
2023年 | 8篇 |
2022年 | 11篇 |
2021年 | 20篇 |
2020年 | 17篇 |
2019年 | 15篇 |
2018年 | 12篇 |
2017年 | 12篇 |
2016年 | 22篇 |
2015年 | 14篇 |
2014年 | 31篇 |
2013年 | 25篇 |
2012年 | 30篇 |
2011年 | 32篇 |
2010年 | 26篇 |
2009年 | 25篇 |
2008年 | 20篇 |
2007年 | 23篇 |
2006年 | 25篇 |
2005年 | 28篇 |
2004年 | 19篇 |
2003年 | 14篇 |
2002年 | 15篇 |
2001年 | 10篇 |
2000年 | 13篇 |
1999年 | 3篇 |
1998年 | 8篇 |
1997年 | 3篇 |
1996年 | 1篇 |
1995年 | 3篇 |
1994年 | 7篇 |
1993年 | 6篇 |
1992年 | 8篇 |
1991年 | 4篇 |
1990年 | 5篇 |
1989年 | 1篇 |
1988年 | 4篇 |
1987年 | 1篇 |
排序方式: 共有525条查询结果,搜索用时 62 毫秒
391.
392.
实施卫星激光定轨的建议 总被引:5,自引:0,他引:5
随着卫星对地观测分辨率的不断提高 ,对卫星在轨位置精度的要求也越来越高。采用星载激光后向反射镜阵列与卫星激光测距定轨方法 ,可以获得厘米级的定轨精度。文中针对我国国情 ,建议我国的导航卫星和对地观测卫星采用激光定轨技术 ,并提出了创立卫星激光定轨条件的实施建议。 相似文献
393.
394.
GOLD码发生器广泛应用于CDMA码分多址系统.其主要用途是产生具有良好相关特性的码序列.调制技术可以应用在一个多用户CDMA系统中的各种形式的扩频技术中.最流行的是直接序列扩频技术.本文对广泛用于扩频通信的m序列及其复合序列平衡GOLD码进行了深入研究,并实现了一种基于DSP的平衡GOLD码发生器. 相似文献
395.
雷达信号脉内调制方式识别是电子对抗的重要内容。从工程应用的角度,对滤波后的复信号利用改进的相位展开算法,计算瞬时相位、瞬时频率。判断频率跳变点的个数,对时-频曲线进行拟合,根据拟合的参数和信号的时宽带宽积确定信号是否为线性调频-二相编码复合调制信号。再对正确识别的信号进行参数估计,接着重构原线性调频信号,共轭相乘得到基带相位编码信号。最后采用小波变换法提取码速率。仿真结果表明,该算法有很好的识别率和参数估计精度。 相似文献
396.
397.
提出了一种限定虚警概率的PN码捕获的自适应门限估计算法,首先在对判决变量的统计特性分析的基础上,计算出了判决门限的有偏估计量;然后分析了估计偏差对捕获系统检测概率和虚警概率的影响;最后,计算机仿真表明,在限定虚警概率的前提下,捕获系统在高斯白噪声信道和瑞利衰落信道下具有较高的检测概率,自适应门限的估计方法易于实现,且适合工程应用。 相似文献
398.
Qisheng Wang Shuanggen Jin Youjian Hu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(3):1049-1057
As an important error source in Global Navigation Satellite System (GNSS) positioning and ionospheric modeling, the differential code biases (DCB) need to be estimated accurately, e.g., the regional Quasi-Zenith satellite system (QZSS). In this paper, the DCB of QZSS is estimated by adopting the global ionospheric modeling method based on QZSS/GPS combined observations from Multi-GNSS experiment (MGEX). The performance of QZSS satellite and receiver DCB is analyzed with observations from day of year (DOY) 275–364, 2018. Good agreement between our estimated QZSS satellite DCB and the products from DLR and CAS is obtained. The bias and root mean square (RMS) of DCB are mostly within ±0.3 ns. The day-to-day fluctuation of the DCB time series is less than 0.5 ns with about 96% of the cases for all satellites. However, the receiver DCB is a little less stable than satellite DCB, and their standard deviations (STDs) are within 1.9 ns. The result shows that the stability of the receiver DCBs is not significantly related to the types of receiver or antenna. 相似文献
399.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(1):650-662
Multipath effects on code observables account for one of the major error sources in high-accuracy Global Positioning System (GPS)-based positioning, atmosphere sounding and timing applications. The multipath hemispherical model (MHM) represents one of the most widely used methods of mitigating code multipath effects by taking advantage of their spatial repeatability. The use of MHM usually assumes that the receiver code biases (RCBs) are time-invariant; however, this assumption is not always valid, as RCBs and linear combinations thereof (differential code biases, for instance) have long been found to be time-varying over a period of one day. In this contribution, we propose an extended multipath hemispherical model (EMHM) that is capable of mitigating the code multipath effects in the presence of time-varying RCBs. Consequently, the proposed EMHM has two advantages. First, the EMHM gives rise to code multipath corrections with improved reliability because it addresses the intraday variability of RCBs. Second, more interestingly, the EMHM allows easy and effective calibration of short-term temporal variations, if any, in the RCB on each frequency. These advantages are hopeful to benefit GPS code-related applications. 相似文献
400.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(5):1518-1527
Attitude is the important parameter for active debris removal and collision avoidance. This paper deduced the spin axis orientation and spin period of the rocket body, CZ-3B R/B (NORAD ID 38253), using the satellite laser ranging and light curve data measured with single-photon detector at Graz station. The epoch method and LC & SLR residuals fitting were combined to determine these values. The derived right ascension angle was around 220°, the declination angle was near 64° and the sidereal period was calculated to be 117.724 s, for 2017-07-03. The results derived from the two distinct methods were mutually validated. Rocket bodies are a major contributor to space debris and this work provides a reference for attitude determination and attitude modelling. 相似文献