全文获取类型
收费全文 | 41篇 |
免费 | 11篇 |
国内免费 | 7篇 |
专业分类
航空 | 28篇 |
航天技术 | 16篇 |
综合类 | 7篇 |
航天 | 8篇 |
出版年
2024年 | 2篇 |
2023年 | 1篇 |
2022年 | 5篇 |
2021年 | 3篇 |
2020年 | 2篇 |
2019年 | 2篇 |
2018年 | 3篇 |
2017年 | 2篇 |
2016年 | 2篇 |
2015年 | 2篇 |
2014年 | 6篇 |
2013年 | 3篇 |
2012年 | 4篇 |
2011年 | 2篇 |
2009年 | 2篇 |
2007年 | 3篇 |
2006年 | 1篇 |
2005年 | 1篇 |
2004年 | 1篇 |
2003年 | 3篇 |
2001年 | 1篇 |
2000年 | 2篇 |
1999年 | 2篇 |
1997年 | 2篇 |
1995年 | 1篇 |
1992年 | 1篇 |
排序方式: 共有59条查询结果,搜索用时 15 毫秒
1.
为推动微通道冷却技术在航空发动机中的应用,进一步提高航空发动机性能,本文通过扫描电子显微镜、粗糙度扫描仪等多方式扫描得到实际加工物体表面形貌,结合分形理论进行处理,得到真实、光滑、分形插值、康托尔集四类圆形截面管模型,管径100μm~400μm;采用格子Boltzmann方法进行数值模拟,首先通过与文献中实验结果的对比,验证了此方法的正确性,然后对空气在这四类圆形截面微通道中的对流换热特性进行了数值模拟,计算雷诺数Re范围80~640;结果发现:表面形貌是微通道中对流换热不可忽略的因素,相对粗糙度越大越有利于换热,真实扫描管的换热性能要比相同条件下光滑管高2.22%;分形理论可用于微通道表面形貌的构建,在相同迭代次数下,分形插值模型与真实扫描形貌换热性能相差0.03%,而康托尔集模型与真实扫描形貌换热性能相差1.88%,分形插值模型较康托尔集模型更能真实地反映实际形貌;微通道中,随着雷诺数的增加Nu将不再是常数,而是有增加的趋势。 相似文献
2.
3.
单向层合结构的高强度碳纤维增强树脂基复合材料已逐渐发展成为航空承力结构件的主要材料,相关的切削加工需求也越来越多。由于显著的各向异性,单向层合结构的碳纤维复合材料易在切削加工中形成缺陷,难切削加工性明显。采用直角自由切削试验的方法,得到了T700航空高强度碳纤维单向层合结构复合材料在不同纤维方向角下的切削力、切削比能、切削温度、切削加工表面。基于试验结果讨论了碳纤维单向层合材料在切削过程中力热行为的各向异性,得到了不同切削参数条件下的切削比能图谱以及碳纤维复合材料的切削热源和传导模型。通过扫描电子显微镜(Scanning electron microscope,SEM)分析了典型切削加工表面的特征,得到了不同纤维方向下的表面形成规律。 相似文献
4.
Jerome Bouffard Francesco Nencioli Romain Escudier Andrea Michelangelo Doglioli Anne A. Petrenko Ananda Pascual Pierre-Marie Poulain Dalila Elhmaidi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Optimal interpolation methods for improving the reconstruction of coastal dynamics from along-track satellite altimetry measurements have been recently developed over the North Western Mediterranean Sea. Maps of satellite-derived geostrophic current anomalies are generated using these methods, and added to different mean circulation fields in order to obtained absolute geostrophic currents. The resulting fields are then compared to standard AVISO products, and their accuracies are assessed with Lagrangian diagnostics. The trajectories of virtual particle clusters are simulated with a Lagrangian code either with new current fields or with the AVISO ones. The simulated trajectories are then compared to 16 in situ drifter trajectories to evaluate the performance of the different velocity fields. The comparisons show that the new current fields lead to better results than the AVISO one, especially over the shallow continental shelf of the Gulf of Lion. However, despite the use of innovative strategies, some altimetry limitations still persist in the coastal domain, where small scale processes remain sub-sampled by conventional altimetry coverage but will benefit from technological development in the near future. Some of the limitations of the Lagrangian diagnostics presently used are also analyzed, but dedicated studies will be required for future further investigations. 相似文献
5.
Influence of lunar topography on simulated surface temperature 总被引:2,自引:0,他引:2
Meng Zhiguo Xu Yi Cai Zhanchuan Chen Shengbo Lian Yi Huang Hang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The surface temperature of the Moon is one of the essential parameters for the lunar exploration, especially to evaluate the Moon thermophysical features. The distribution of the temperature is heavily influenced by the Moon topography, which, however, is rarely studied in the state-of-art surface temperature models. Therefore, this paper takes the Moon topography into account to improve the surface temperature model, Racca model. The main parameters, such as slopes along the longitude and latitude directions, are estimated with the topography data from Chang’E-1 satellite and the Horn algorithm. Then the effective solar illumination model is then constructed with the slopes and the relative position to the subsolar point. Finally, the temperature distribution over the Moon surface is obtained with the effective illumination model and the improved Racca model. The results indicate that the distribution of the temperature is very sensitive to the fluctuation of the Moon surface. The change of the surface temperature is up to 150 K in some places compared to the result without considering the topography. In addition, the variation of the surface temperature increases with the distance from the subsolar point and the elevation, along both latitude and longitude directions. Furthermore, the simulated surface temperature coincides well with the brightness temperature in 37 GHz observed by the microwave sounder onboard Chang’E-2 satellite. The corresponded emissivity map not only eliminates the influence of the topography, but also hints the inherent properties of the lunar regolith just below the surface. Last but not the least, the distribution of the permanently shadowed regions (PSRs) in the lunar pole area is also evaluated with the simulated surface temperature result. 相似文献
6.
7.
8.
多重分形谱在材料分析中的应用研究 总被引:13,自引:0,他引:13
基于多重分形谱的物理意义,通过图像分析与处理技术,利用Delphi语言设计了图像结构的多重分形谱的计算程序。通过程序中图像黑白二值化转化阈值的设定,实现了从材料组织结构形貌图像上提取其相应的概率测度和标度指数的功能,并计算了它们的多重分形谱。分析表明:在对材料的组织结构进行研究的问题中,多重分形谱是一种有意义的表征参数,能够从多分形角度对材料的组织结构开展定量化的分析与解释。 相似文献
9.
10.
Zhen Zhong Fei Li Jianguo Yan Peng Yan James M. Dohm 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
This paper presents a FORTRAN computer program. The program as code will be used for lunar parameter inversions based on gravity/topography admittance. This will be done by assuming that the lunar lithosphere is modeled as a thin elastic spherical shell. The parameters discussed here include; load ratio, crustal thickness, subsurface load depth, crustal density and elastic lithosphere thickness. The admittance of the best-fitting model can be found through automatically adjusting misfits between one theoretical admittance and an observed one. The results in this paper indicate that this research’s theoretical model is reasonable for exploring the best-fitting parameters. In addition, this code is not only able to automatically and simultaneously calculate the global optimum solution of the parameters studied, but also performs well in computational speed. The code can be easily modified to include more parameter inversions; such as the inversion for subsurface density anomaly and the case of considering infilling material in some lunar mare basins. 相似文献