全文获取类型
收费全文 | 249篇 |
免费 | 45篇 |
国内免费 | 14篇 |
专业分类
航空 | 110篇 |
航天技术 | 167篇 |
综合类 | 5篇 |
航天 | 26篇 |
出版年
2024年 | 2篇 |
2023年 | 11篇 |
2022年 | 6篇 |
2021年 | 11篇 |
2020年 | 12篇 |
2019年 | 8篇 |
2018年 | 7篇 |
2017年 | 13篇 |
2016年 | 8篇 |
2015年 | 5篇 |
2014年 | 18篇 |
2013年 | 24篇 |
2012年 | 18篇 |
2011年 | 24篇 |
2010年 | 11篇 |
2009年 | 28篇 |
2008年 | 15篇 |
2007年 | 12篇 |
2006年 | 9篇 |
2005年 | 10篇 |
2004年 | 4篇 |
2003年 | 9篇 |
2002年 | 1篇 |
2001年 | 3篇 |
2000年 | 3篇 |
1999年 | 6篇 |
1998年 | 3篇 |
1997年 | 5篇 |
1996年 | 1篇 |
1995年 | 2篇 |
1994年 | 6篇 |
1993年 | 3篇 |
1992年 | 1篇 |
1991年 | 2篇 |
1990年 | 4篇 |
1987年 | 3篇 |
排序方式: 共有308条查询结果,搜索用时 15 毫秒
1.
2.
吴军%张立武%王常建 《宇航材料工艺》2003,33(4):57-61
采用金相显微镜、透射电镜观察了焊后不同时效状态下T— 2 5 0马氏体时效钢电子束焊缝的微观组织 ,测试了不同时效状态下焊接接头的室温强度、夏比缺口冲击韧性、显微硬度 ,并用扫描电镜分析了拉伸断口形貌。结果表明 :随时效温度的升高 ,焊缝区枝晶间逆转奥氏体析出量增加 ,焊缝缺口冲击韧性增大 ,断口韧窝增大 ;但由于 5 0 0℃× 4h时效处理后焊缝马氏体孪晶较多而使其拉伸强度和缺口冲击韧性降低。经 4 80℃× 4h时效处理后 ,焊接接头强度具有最佳强韧性配合 相似文献
3.
4.
介绍了一种新颖的原子氧模拟试验装置。该装置采用了微波电子回旋共振(electroncyclotronresonance简称“ECR”)的先进技术。最佳调试状态下,可获得10(15)/(cm2·s)的束流。在该试验装置上,对航天器上常用的Kapton和石墨环氧材料进行了原子氧效应试验,首次在国内成功的获得了原子氧束流模拟试验的样品结果。对样品的表面形貌分析证明:试验结果完全与国外同类设备的试验结论一致,这标志着中国在原子氧地面模拟技术领域的研究已取得重要进展。 相似文献
5.
利用MF雷达对耀斑期间电离层D区电子密度的观测研究 总被引:1,自引:0,他引:1
利用MF雷达观测资料对X级别耀斑爆发期间在66-80km高度之间的电子密度进行了研究,观测到了耀斑爆发期间电子密度的突然增加,在较低高度上的电子密度的时间变化趋势与耀斑的软X射线辐射通量相关.电子密度的变化强度依赖于具体的耀斑参数,有些耀斑引起的电子密度增加高达400cm^-3,有些仅为100cm^-3左右.但耀斑期间在这一高度区间增加的总电子含量增量仅占耀斑辐射引起的整个电离层总电子含量增量的千分之一左右.最后,利用恢复阶段电子密度的时间变化过程估算了1997年11月4日耀斑期间部分高度上的有效复合系数. 相似文献
6.
7.
M. Pezzopane M. Pietrella A. Pignatelli B. Zolesi Lj.R. Cander 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
This paper describes the three-dimensional (3-D) electron density mapping of the ionosphere given as output by the assimilative IRI-SIRMUP-P (ISP) model for three different geomagnetic storms. Results of the 3-D model are shown by comparing the electron density profiles given by the model with the ones measured at two testing ionospheric stations: Roquetes (40.8°N, 0.5°E), Spain, and San Vito (40.6°N, 17.8°E), Italy. The reference ionospheric stations from which the autoscaled foF2 and M(3000)F2 data as well as the real-time vertical electron density profiles are assimilated by the ISP model are those of El Arenosillo (37.1°N, 353.3°E), Spain, Rome (41.8°N, 12.5°E), and Gibilmanna (37.9°N, 14.0°E), Italy. Overall, the representation of the ionosphere made by the ISP model is better than the climatological representation made by only the IRI-URSI and the IRI-CCIR models. However, there are few cases for which the assimilation of the autoscaled data from the reference stations causes either a strong underestimation or a strong overestimation of the real conditions of the ionosphere, which is in these cases better represented by only the IRI-URSI model. This ISP misrepresentation is mainly due to the fact that the reference ionospheric stations covering the region mapped by the model turn out to be few, especially for disturbed periods when the ionosphere is very variable both in time and in space and hence a larger number of stations would be required. The inclusion of new additional reference ionospheric stations could surely smooth out this concern. 相似文献
8.
Analysis of the ionosphere/plasmasphere electron content variability during strong geomagnetic storm
Iu.V. Cherniak I.E. Zakharenkova D. Dzubanov A. Krankowski 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The ionosphere/plasmasphere electron content (PEC) variations during strong geomagnetic storms in November 2004 were estimated by combining of mid-latitude Kharkov incoherent scatter radar observations and GPS TEC data derived from global TEC maps. The comparison between two independent measurements was performed by analysis of the height-temporal distribution for specific location corresponding to the mid-latitudes of Europe. The percentage contribution of PEC to GPS TEC indicated the clear dependence from the time with maximal values (more than 70%) during night-time. During day-time the lesser values (30–45%) were observed for quiet geomagnetic conditions and rather high values of the PEC contribution to GPS TEC (up to 90%) were observed during strong negative storm. These changes can be explained by the competing effects of electric fields and winds, which tend to raise the layer to the region with lower loss rate and movement of the ionospheric plasma to the plasmasphere. 相似文献
9.
V. Truhlik D. Bilitza L. Triskova 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
A database of electron temperature (Te) measurements comprising of most of the available satellite measurements in the topside ionosphere is used for studying the solar activity variations of the electron temperature Te at different latitudes, altitudes, local times and seasons. The Te data are grouped into three levels of solar activity (low, medium, high) at four altitude ranges, for day and night, and for equinox and solstices. We find that in general Te changes with solar activity are small and comparable in magnitude with seasonal changes but much smaller than the changes with altitude, latitude, and from day to night. In all cases, except at low altitude during daytime, Te increases with increasing solar activity. But this increase is not linear as assumed in most empirical Te models but requires at least a parabolic approximation. At 550 km during daytime negative as well as positive correlation is found with solar activity. Our global data base allows to quantify the latitude range and seasonal conditions for which these correlations occur. A negative correlation with solar activity is found in the invdip latitude range from 20 to 55 degrees during equinox and from 20 degrees onward during winter. In the low latitude (20 to −20 degrees invdip) F-region there is almost no change with solar activity during solstice and a positive correlation during equinox. A positive correlation is also observed during summer from 30 degrees onward. 相似文献
10.
J. Watermann P. Stauning H. Lühr P.T. Newell F. Christiansen K. Schlegel 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
We examined some 75 observations from the low-altitude Earth orbiting DMSP, Ørsted and CHAMP satellites which were taken in the region of the nominal cusp. Our objective was to determine whether the actually observed cusp locations as inferred from magnetosheath-like particle precipitation (“particle cusp”) and intense small-scale magnetic field variations (“current cusp”), respectively, were identical and were consistent with the statistically expected latitude of the cusp derived from a huge number of charged particle spectrograms (“statistical cusp”). 相似文献