全文获取类型
收费全文 | 1286篇 |
免费 | 229篇 |
国内免费 | 261篇 |
专业分类
航空 | 975篇 |
航天技术 | 434篇 |
综合类 | 184篇 |
航天 | 183篇 |
出版年
2024年 | 6篇 |
2023年 | 26篇 |
2022年 | 51篇 |
2021年 | 54篇 |
2020年 | 64篇 |
2019年 | 59篇 |
2018年 | 70篇 |
2017年 | 71篇 |
2016年 | 66篇 |
2015年 | 73篇 |
2014年 | 111篇 |
2013年 | 95篇 |
2012年 | 97篇 |
2011年 | 112篇 |
2010年 | 79篇 |
2009年 | 120篇 |
2008年 | 96篇 |
2007年 | 61篇 |
2006年 | 68篇 |
2005年 | 68篇 |
2004年 | 40篇 |
2003年 | 36篇 |
2002年 | 32篇 |
2001年 | 31篇 |
2000年 | 23篇 |
1999年 | 20篇 |
1998年 | 18篇 |
1997年 | 16篇 |
1996年 | 16篇 |
1995年 | 14篇 |
1994年 | 17篇 |
1993年 | 12篇 |
1992年 | 15篇 |
1991年 | 15篇 |
1990年 | 9篇 |
1989年 | 11篇 |
1988年 | 1篇 |
1987年 | 1篇 |
1984年 | 2篇 |
排序方式: 共有1776条查询结果,搜索用时 281 毫秒
91.
92.
本文采用直接过滤的Navier-Stokes方程组作为可压缩湍流大涡模拟控制方程组。方程组中因过滤产生的高阶相关项用Taylor级数展开近似,但仅保留级数的一阶导数项。这样产生的误差相当于丢失了模型的部分耗散作用,本文用一种动力学非线性亚格子模型来补偿丢失的耗散影响。本文根据Caylay-Hamilton定理导出了一个非线性亚格子模型,模型中包含的系数由动力学模式确定。与传统的动力学Smagorinsky模式相比,这种动力学非线性模型(DNM)稳定性更好,且不需要在统计均匀方向进行统计平均来计算模型系数,因此减少了计算开销。本文用这种非线性亚格子模型对绕双椭球高超声速湍流进行了模拟,并将所得结果与实验值、计算值及理论值进行了对比。结果表明,本文模型可以有效地模拟可压缩湍流流场。 相似文献
93.
94.
M. Ayub S. Iqbal M.A. Ameen B.W. Reinisch 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The monthly hourly medians of maximum electron density, NmF2, at two Pakistani ionospheric stations, Karachi and Islamabad, have been determined for solar minimum (1996) and solar maximum (2000) and compared with IRI predictions using the URSI coefficients. At night and pre-noon period the NmF2 values at both stations are almost equal during the 2 years. However, at post-noon the values at Karachi are considerably larger than those at Islamabad due to the equatorial or geomagnetic anomaly. Karachi (geomag. coord. 16.44°N, 139.08°E) lies near the region of the equatorial anomaly (+20 and −20 geomagnetic latitude), so most of the NmF2 values at Karachi are larger than those at Islamabad (geomag. coord. 24.46°N, 145.67°E). The maximum monthly values of NmF2 show a semi-annual variation at Karachi and Islamabad both during 1996 and 2000 as predicted by IRI. 相似文献
95.
96.
Yen-Hsyang Chu Chin-Lung SuHsiao-Tsung Ko 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
With a network of ground-based ionosondes distributed around the world, the ionospheric peak electron density and its height measured by FORMOSAT-3/COSMIC satellites in terms of GPS radio occultation technique are extensively examined in this article. It is found that, in spite of the latitude, the mean values of the peak electron density measured by COSMIC satellites are systematically smaller than those observed by ground-based ionosondes. The discrepancy between them is dependent on the latitude, namely, it is small in low and mid-latitudes and large in high-latitude region. Moreover, statistical analysis shows that the slopes of the regression line that is best fitted to the scatter diagram of occultation-retrieved peak electron density (ordinate axis) versus ionosonde-observed peak density (abscissa axis) are universally less than one. This feature is believed to be the result of path average effect of non-uniform distribution of the electron density along the GSP ray during the occultation. A comparison between COSMIC-measured peak height and ionosonde-derived peak height hmF2 indicates that the former is systematically higher than the latter. The difference in the two can be as large as 20% or more in equatorial and low-latitude regions. This result implies that the peak height hmF2 derived from the virtual height through true height analysis based on Titheridge method seems to underestimate the true peak height. The correlation between COSMIC and ionosonde peak electron densities is analyzed and the result reveals that correlation coefficient seems to be dependent on the fluctuation of the occultation-retrieved electron density profile. The correlation will be higher (lower) for the electron density profiles with smaller (larger) fluctuations. This feature suggests that the inhomogeneous distribution of the electron density along the GPS ray path during the occultation plays an important role affecting the correlation between COSMIC and ionosonde measurements. 相似文献
97.
M.A. Van Zele A. Meza 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
This paper studies the efficiency of geomagnetic solar flare effects (gsfe) in X solar flare detection; so during the period 1999–2007 a comparison between solar flare (sf) observed by satellites of the Geostationary Operational Environmental Satellite (GOES) programme and gsfe published by the Service International des Indices Geomagnetiques (SIIG) is made. 相似文献
98.
幂等自映射的Nielsen数(4) 总被引:1,自引:0,他引:1
本文利用粘接等方法证明了一类拓朴空间上的幂等自映射的Nielsen数不超过1。 相似文献
99.
100.
相关系数平稳过程时频分析方法 总被引:9,自引:6,他引:9
相关系数平稳过程是从非平稳过程中分离出的一类工程上常见且便于研究的随机过程,其均值和方差都可随时间变化,传统的平稳随机过程是它的一个特例。本文提出了相关系数AR(p),MA(q)和ARMA(p,q)序列的概念,建立了相关系数平稳过程的时频分析方法。该方法首先在时域进行全程分析,得到相关系数平稳过程的均值函数、方差函数和相关系数函数,然后可以对其进行傅里叶变换、短时傅里叶变换或小波变换,给出相关系数平稳过程的谱密度,同时提出了随机项谱密度和趋势项谱密度的概念。文中还讨论了线性系统对相关系数平稳过程输入的响应。 相似文献