全文获取类型
收费全文 | 210篇 |
免费 | 46篇 |
国内免费 | 17篇 |
专业分类
航空 | 127篇 |
航天技术 | 104篇 |
综合类 | 10篇 |
航天 | 32篇 |
出版年
2024年 | 1篇 |
2023年 | 5篇 |
2022年 | 2篇 |
2021年 | 10篇 |
2020年 | 13篇 |
2019年 | 10篇 |
2018年 | 12篇 |
2017年 | 14篇 |
2016年 | 8篇 |
2015年 | 10篇 |
2014年 | 16篇 |
2013年 | 13篇 |
2012年 | 23篇 |
2011年 | 23篇 |
2010年 | 8篇 |
2009年 | 11篇 |
2008年 | 14篇 |
2007年 | 11篇 |
2006年 | 10篇 |
2005年 | 11篇 |
2004年 | 3篇 |
2003年 | 10篇 |
2002年 | 6篇 |
2001年 | 2篇 |
2000年 | 7篇 |
1999年 | 2篇 |
1998年 | 2篇 |
1997年 | 2篇 |
1996年 | 4篇 |
1995年 | 3篇 |
1993年 | 3篇 |
1992年 | 2篇 |
1990年 | 1篇 |
1988年 | 1篇 |
排序方式: 共有273条查询结果,搜索用时 15 毫秒
31.
主成分分析用于近红外光谱定量测定高硅氧/酚醛预浸料树脂含量及挥发份含量研究 总被引:1,自引:0,他引:1
采用傅里叶变换近红外漫反射光谱技术分析了酚醛树脂固化过程的光谱变化,发现高硅氧/酚醛预浸料的近红外光谱经一阶导数处理后,被树脂信息掩盖的挥发份(乙醇)的光谱信息显露出来,由此采用处理后的光谱定量分析挥发份能取得更精确的结果。结合主成分分析法研究了高硅氧/酚醛预浸料树脂含量、挥发份含量的定量分析。结果表明,预浸料的第一主成分在树脂含量上有极高的正载荷。用主成分回归所建立的模型对未知样品预测,树脂含量和挥发份含量平均标准偏差分别为0.6114和0.1885。 相似文献
32.
电子束固化高模量纤维增强复合材料力学性能研究 总被引:1,自引:0,他引:1
包建文%徐松华%李晔%陈祥宝 《宇航材料工艺》2003,33(4):53-56
用湿法缠绕工艺制备了M40/EB99—1预浸料,研究了电子束固化高模量石墨化碳纤维M40增强EB99-1环氧树脂复合材料的常规力学性能、耐热疲劳性能和热物理性能,并与M40/5228、M40/4211等热固化复合材料的性能进行了比较。实验研究表明,除了剪切强度稍逊于热固化M40/5228复合材料外,其它常规力学性能都优于热固化M40/5228、M40/211复合材料,表现了较好的综合力学性能。电子束固化M40/EB99—1复合材料经冷热交变循环后的性能明显优于热固化M40/5228、M40/4211复合材料,表现了较好的耐热疲劳性能。 相似文献
33.
34.
35.
Liming He Lixin Wu Sergey Pulinets Shanjun Liu Fan Yang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
A precise determination of ionospheric total electron content (TEC) anomaly variations that are likely associated with large earthquakes as observed by global positioning system (GPS) requires the elimination of the ionospheric effect from irregular solar electromagnetic radiation. In particular, revealing the seismo-ionospheric anomalies when earthquakes occurred during periods of high solar activity is of utmost importance. To overcome this constraint, a multiresolution time series processing technique based on wavelet transform applicable to global ionosphere map (GIM) TEC data was used to remove the nonlinear effect from solar radiation for the earthquake that struck Tohoku, Japan, on 11 March, 2011. As a result, it was found that the extracted TEC have a good correlation with the measured solar extreme ultraviolet flux in 26–34 nm (EUV26–34) and the 10.7 cm solar radio flux (F10.7). After removing the influence of solar radiation origin in GIM TEC, the analysis results show that the TEC around the forthcoming epicenter and its conjugate were significantly enhanced in the afternoon period of 8 March 2011, 3 days before the earthquake. The spatial distributions of the TEC anomalous and extreme enhancements indicate that the earthquake preparation process had brought with a TEC anomaly area of size approximately 1650 and 5700 km in the latitudinal and longitudinal directions, respectively. 相似文献
36.
A.O. Adewale E.O. Oyeyemi J. Olwendo 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
Vertical total electron content (VTEC) observed at Mbarara (geographic co-ordinates: 0.60°S, 30.74°E; geomagnetic coordinates: 10.22°S, 102.36°E), Uganda, for the period 2001–2009 have been used to study the diurnal, seasonal and solar activity variations. The daily values of the 10.7 cm radio flux (F10.7) and sunspot number (R) were used to represent Solar Extreme Ultraviolet Variability (EUV). VTEC is generally higher during high solar activity period for all the seasons and increases from 0600 h LT and reaches its maximum value within 1400 h–1500 h LT. All analysed linear and quadratic fits demonstrate positive VTEC-F10.7 and positive VTEC-R correlation, with all fits at 0000 h and 1400 h LT being significant with a confidence level of 95% when both linear and quadratic models are used. All the fits at 0600 h LT are insignificant with a confidence level of 95%. Generally, over Mbarara, quadratic fit shows that VTEC saturates during all seasons for F10.7 more than 200 units and R more than 150 units. The result of this study can be used to improve the International Reference Ionosphere (IRI) prediction of TEC around the equatorial region of the African sector. 相似文献
37.
Malini Aggarwal H.P. Joshi K.N. Iyer Y.S. Kwak 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
In this paper, response of low latitude ionosphere to a moderate geomagnetic storm of 7–8 May 2005 (SSC: 1920 UT on 7 May with Sym-H minimum, ∼−112 nT around 1600 UT on 8 May) has been investigated using the GPS measurements from a near EIA crest region, Rajkot (Geog. 22.29°N, 70.74°E, Geomag.14°), India. We found a decrease in total electron content (TEC) in 12 h after the onset of the storm, an increase during and after 6 h of Sym-H deep minimum with a decrease below its usual-day level on the second day during the recovery phase of the storm. On 8 May, an increase of TEC is observed after sunset and during post-midnight hours (maximum up to 170%) with the formation of ionospheric plasma bubbles followed by a nearly simultaneous onset of scintillations at L-band frequencies following the time of rapid decrease in Sym-H index (−30 nT/h around 1300 UT). 相似文献
38.
S.S. Kouris K.V. Polimeris L. Ciraolo D.N. Fotiadis 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Several years of hourly daily GPS measurements of the vertical total electron content (TEC) and of the equivalent slab thickness made at different European locations are analysed by using the linear regression technique to demonstrate the response of these two ionospheric parameters to seasonal variations. It is found that both TEC and slab thickness are highly correlated with season. Analytical relationships are determined expressing the seasonal dependence of the vertical TEC and of the equivalent slab thickness as a function of the seasonal parameter cos χ at noon in each location. 相似文献
39.
研究了氢醌库仑法测定金含量的方法、条件、考察共存离子的影响,并应用于岩矿石中金的分析。研究表明该法选择及结果都很好。 相似文献
40.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(11):2529-2539
From September 7 to 8, 2017, a G4-level strong geomagnetic storm occurred, which seriously impacted on the Earth’s ionosphere. In this work, the global ionospheric maps released by Chinese Academy of Sciences are used to investigate the ionospheric responses over China and its adjacent regions during the strong storm. The prominent TEC enhancements, which mainly associated with the neutral wind and eastward prompt penetration electric field, are observed at equatorial ionization anomaly crests during the main phase of the storm on 8 September 2017. Compared with those on 8 September, the TEC enhancements move to lower-latitude regions during the recovery phase on 9 September. A moderate storm occurred well before the start of the strong storm causes similar middle-latitude TEC enhancements on 7 September. However, the weak TEC depletion is observed at middle and low latitude on 9–10 September, which could be associated with the prevailing westward disturbance electric field or storm-time neural composition changes. In addition, the storm-time RMS and STD values of the ionospheric TEC grids over China increase significantly due to the major geomagnetic storm. The maximum of the RMS reaches 12.0 TECU, while the maximum of the STD reaches 8.3 TECU at ~04UT on 8 September. 相似文献