全文获取类型
收费全文 | 845篇 |
免费 | 157篇 |
国内免费 | 249篇 |
专业分类
航空 | 771篇 |
航天技术 | 190篇 |
综合类 | 182篇 |
航天 | 108篇 |
出版年
2024年 | 3篇 |
2023年 | 17篇 |
2022年 | 34篇 |
2021年 | 45篇 |
2020年 | 48篇 |
2019年 | 37篇 |
2018年 | 48篇 |
2017年 | 33篇 |
2016年 | 59篇 |
2015年 | 63篇 |
2014年 | 65篇 |
2013年 | 45篇 |
2012年 | 53篇 |
2011年 | 61篇 |
2010年 | 50篇 |
2009年 | 63篇 |
2008年 | 47篇 |
2007年 | 55篇 |
2006年 | 44篇 |
2005年 | 32篇 |
2004年 | 39篇 |
2003年 | 32篇 |
2002年 | 28篇 |
2001年 | 21篇 |
2000年 | 20篇 |
1999年 | 21篇 |
1998年 | 20篇 |
1997年 | 22篇 |
1996年 | 23篇 |
1995年 | 20篇 |
1994年 | 12篇 |
1993年 | 18篇 |
1992年 | 10篇 |
1991年 | 12篇 |
1990年 | 18篇 |
1989年 | 14篇 |
1988年 | 16篇 |
1987年 | 2篇 |
1986年 | 1篇 |
排序方式: 共有1251条查询结果,搜索用时 15 毫秒
1.
《中国航空学报》2021,34(5):617-627
In this paper, a progressive approach to predict the multiple shot peening process parameters for complex integral panel is proposed. Firstly, the invariable parameters in the forming process including shot size, mass flow, peening distance and peening angle are determined according to the empirical and machine type. Then, the optimal value of air pressure for the whole shot peening is selected by the experimental data. Finally, the feeding speed for every shot peening path is predicted by regression equation. The integral panel part with thickness from 2 mm to 5 mm and curvature radius from 3200 mm to 16000 mm is taken as a research object, and four experiments are conducted. In order to design specimens for acquiring the forming data, one experiment is conducted to compare the curvature radius of the plate and stringer-structural specimens, which were peened along the middle of the two stringers. The most striking finding of this experiment is that the outer shape error range is below 3.9%, so the plate specimens can be used in predicting feeding speed of the integral panel. The second experiment is performed and results show that when the coverage reaches the limit of 80%, the minimum feeding speed is 50 mm/s. By this feeding speed, the forming curvature radius of the specimens with different thickness from the third experiment is measured and compared with the research object, and the optimal air pressure is 0.15 MPa. Then, the plate specimens with thickness from 2 mm to 5 mm are peened in the fourth experiment, and the measured curvature radius data are used to calculate the feeding speed of different shot peening path by regressive analysis method. The algorithm is validated by forming a test part and the average deviation is 0.496 mm. It is shown that the approach can realize the forming of the integral panel precisely. 相似文献
2.
3.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2007,39(5):661-667
Monthly median values of foF2, hmF2 and M(3000)F2 parameters, with hourly time interval resolution for the diurnal variation, obtained with DPS-4 digisonde observations at Hainan (19.4°N, 109.0°E) are used to study the low latitude ionospheric variation behavior. The observational results are compared with the International Reference Ionospheric Model (IRI) predictions. The time period coverage of the data used for the present study is from March 2002 to February 2005. Our present study showed that: (1) In general, IRI predictions using CCIR and URSI coefficients follow well the diurnal and seasonal variation patterns of the experimental values of foF2. However, CCIR foF2 and URSI foF2 IRI predictions systematically underestimate the observed results during most time period of the day, with the percentage difference ΔfoF2 (%) values changing between about −5% and −25%, whereas for a few hours around pre-sunrise, the IRI predictions generally overestimate the observational ones with ΔfoF2 (%) sometimes reaching as large as ∼30%. The agreement between the IRI results and the observational ones is better for the year 2002 than for the other years. The best agreement between the IRI results and the observational ones is obtained in summer when using URSI coefficients, with the seasonal average values of ΔfoF2 (%) being within the limits of ±10%. (2) In general, the IRI predicted hmF2 values using CCIR M(3000)F2 option shows a poor agreement with the observational results. However, when using the measured M(3000)F2 as input, the diurnal variation pattern of hmF2 given by IRI2001 has a much better agreement with the observational one with the detailed fine structures including the pre-sunrise and post-sunset peaks reproduced reasonably well. The agreement between the IRI predicted hmF2 values using CCIR M(30,000)F2 option and the observational ones is worst for the afternoon to post-midnight hours for the high solar activity year 2002. During daytime hours the agreement between the hmF2 values obtained with CCIR M(30,000)F2 option and the observational ones is best for summer season. The discrepancy between the observational hmF2 and that obtained with CCIR M(30,000)F2 option stem from the CCIR M(3000)F2 model, which does not produce the small scale structures observed in the measured M(3000)F2. 相似文献
4.
介绍了H 6部件与外扌圭物测力试验的难点 :一是天平的设计载荷极不匹配 ,如机翼天平的滚转力矩是常规天平的 1 0多倍 ;二是模型尾部是船形尾段。采用常规的支撑方式 ,支杆强度太弱 ,试验不安全 ,同时也不利于多台天平的敷线 ,总体方案采用模型尾部与支杆合为一体的结构形式 ,既保证了试验安全又便于多台天平的敷线。天平设计首先保证试验安全 ,用双电桥提高天平的输出。试验结果表明 :总体试验方案正确 ,天平设计合理 ,支撑刚度好 ,测量精度高。 相似文献
5.
6.
螺旋桨滑流对飞机绕流影响的试验研究 总被引:1,自引:0,他引:1
在国产双涡桨支线飞机发展过程中,曾专门研究过螺旋桨滑流对飞机表面压力分布的影响。本文以此为基础,从滑流对飞机绕流影响出发,研究了螺旋桨滑流引起飞机气动特性的变化,重点讨论了气动特性变化的机理。 相似文献
7.
尺寸参数对气动液阀启动特性的影响 总被引:1,自引:0,他引:1
为气动液阀的启动过程建立了数学模型,分析了尺寸参数对该阀启动特性的影响。计算结果表明:在保证必要的工作寿命的前提下,适当地增大控制腔气孔的直径或增大靠近控制腔的活塞端面直径有利于提高该阀的响应能力。本文所得的结论有利于此类阀门的设计。 相似文献
8.
9.
We describe work that has recently been completed on deriving the fundamental parameters of eight WR stars through the photoionization modelling of their surrounding nebulae using non-LTE WR flux distributions. The resulting effective temperatures range from 57 000–71 000 K for the WN4-5 stars and <30 000–42 000 K for the WN6-8 stars. The derived stellar parameters are compared with those obtained from stellar emission line modelling. We find good agreement for the hot early WN stars, indicating that the non-LTE WR flux distributions have essentially the correct shape in the crucial far-UV region. We find lower temperatures for the four cooler late WN stars, particularly for the two WN6 stars. For the nebulae surrounding these stars, we find that the model flux distributions produce too much nebular ionization. We suggest that these discrepancies arise because of the lack of line-blanketing in the WR atmospheres. For the WO1 central star of G2.4+1.4, with strong nebular He II 4686 A emission, we derive a temperature of 105 000 K, somewhat less than previous estimates. The positions of our eight WR stars on the H-R diagram are compared with the evolutionary tracks of Maeder (1990) for solar metallicity. In common with previous workers, we find that our derived luminosities are too low, giving an initial mass range of 25–40 M, below that expected for the majority of WR stars. 相似文献
10.
基于模糊聚类的模糊神经网络在非定常气动力建模中的应用 总被引:2,自引:0,他引:2
建立了一种基于模糊聚类的模糊神经网络模型.该模型利用模糊聚类技术确定系统的模糊空间和模糊规则数,利用BP算法调整模糊神经网络的权系数.应用该模型对某飞机模型做俯仰-滚转耦合运动的非定常气动力进行了辨识.结果表明,基于模糊聚类的模糊神经网络计算速度快,辨识结果与实验结果符合较好.用模糊聚类技术可以解决模糊神经网络的结构辨识问题,基于模糊聚类的模糊神经网络可以很好地用于复杂机动飞行的非定常气动力建模. 相似文献