全文获取类型
收费全文 | 1030篇 |
免费 | 244篇 |
国内免费 | 287篇 |
专业分类
航空 | 790篇 |
航天技术 | 349篇 |
综合类 | 171篇 |
航天 | 251篇 |
出版年
2024年 | 3篇 |
2023年 | 13篇 |
2022年 | 33篇 |
2021年 | 39篇 |
2020年 | 41篇 |
2019年 | 50篇 |
2018年 | 66篇 |
2017年 | 56篇 |
2016年 | 51篇 |
2015年 | 38篇 |
2014年 | 64篇 |
2013年 | 54篇 |
2012年 | 65篇 |
2011年 | 77篇 |
2010年 | 77篇 |
2009年 | 65篇 |
2008年 | 67篇 |
2007年 | 66篇 |
2006年 | 89篇 |
2005年 | 66篇 |
2004年 | 60篇 |
2003年 | 49篇 |
2002年 | 31篇 |
2001年 | 32篇 |
2000年 | 44篇 |
1999年 | 39篇 |
1998年 | 31篇 |
1997年 | 23篇 |
1996年 | 45篇 |
1995年 | 24篇 |
1994年 | 37篇 |
1993年 | 16篇 |
1992年 | 10篇 |
1991年 | 6篇 |
1990年 | 12篇 |
1989年 | 5篇 |
1988年 | 11篇 |
1987年 | 2篇 |
1986年 | 2篇 |
1984年 | 2篇 |
排序方式: 共有1561条查询结果,搜索用时 93 毫秒
631.
对多层阻抗渐变的吸波结构设计思想进行了分析,介绍了多层阻抗渐变思想在吸波层板和泡沫两类结构吸波材料设计上的应用。理论计算与试验验证结果均表明,采用多层阻抗渐变设计能够使吸波层板和泡沫的吸波带宽向低频拓展,同时显著提高吸波泡沫的吸收强度。具有三个阻抗渐变吸收层的4 mm厚吸波层板在5~18 GHz频段反射率小于-10 d B;具有六个阻抗渐变吸收层的22 mm厚吸波泡沫在2~18 GHz频段反射率小于-10 d B,其中在6~18 GHz频段反射率小于-20 d B,8~12 GHz频段反射率小于-30 d B。多层阻抗渐变设计是提高结构吸波材料吸波性能的有效手段。 相似文献
632.
A.R. Qian P.F. Yang L.F. Hu W. Zhang S.M. Di Z. Wang J. Han X. Gao P. Shang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
The effects of a high magnetic gradient environment (HMGE) on the cytoskeletal architecture and genes associated with the cytoskeleton in osteoblasts (MC3T3-E1 and MG-63 cells) were investigated using confocal microscopy, real-time polymerase chain reaction (PCR) and atomic force microscopy (AFM). The findings showed that, under diamagnetic levitation conditions, the architecture and average height of the cytoskeleton and surface roughness in osteoblasts were dramatically altered. HMGE affects cytoskeleton arrangement and cytoskeleton-associated gene expression. 相似文献
633.
C. Taricco N. Bhandari P. Colombetti N. Verma 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(2):275-279
Measurements of 44Ti activity in meteorites show that the galactic cosmic ray (GCR) intensity has been declining in the interplanetary space during the past three centuries and has a component of cyclic variation, with periodicity of about 87 years [Taricco, C., Bhandari, N., Cane, D., et al. Galactic cosmic ray flux decline and periodicities in the interplanetary space during the last 3 centuries revealed by 44Ti in meteorites. J. Geophys. Res. 111, A08102, 2006.]. In order to verify these results, we have measured 44Ti activity in Allegan meteorite which fell in 1899 and in some other meteorites with better precision. The measurements confirm low cosmic ray flux and consequently high solar activity near the middle of 19th century. 相似文献
634.
S. Benck M. Cyamukungu J. Cabrera 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,42(9):1538-1549
The topic of relativistic electron dynamics in the outer radiation belt has received considerable attention for many years. Nevertheless, the problem of understanding the physical phenomenon involved is far from being resolved. In this paper, we use DEMETER observations to examine the variations of the energetic electron fluxes and ELF/VLF wave intensities in the inner magnetosphere during the intense 8 November 2004 magnetic storm. Electron flux spectra and associated wave intensity spectra are analysed throughout the magnetic storm and common characteristics or differences to other storm events are retained. The overall objective of this study is to identify and derive parameters that are relevant for particle flux modelling; the time constant characterizing the persistent decay after particle enhancement was found to be one of these important model parameters.The analysis of the 8 November 2004 event reveals that for L-shell parameter higher than 4, an electron flux dropout is observed during the storm’s main phase for electrons in the energy range 0.1–1 MeV, as has been reported from other measurements. Characteristic wave spectra accompanying this phase are analysed. They show a typical enhancement in the frequency range 0.3–10 kHz at onset for all L-shell values under consideration (2 < L < 5). During the first stage of the recovery phase, the electron fluxes are increased to a level higher than the pre-storm level, whereas the level of wave intensity in the frequency range observed below 300 Hz is at its highest. In the second stage, the particle flux decrease goes hand in hand with a global wave activity decline, the relaxation time of the latter being smaller than the former’s one. In some other cases, long-lasting electron enhancement associated with constant wave activity has been observed during this latter stage. For the above mentioned storm, while at low L values the decay time constants are higher for low energy electrons than for high energy electrons, this order is reversed at high L values. At about L = 3.6 the time constant is independent of electron energy. 相似文献
635.
636.
637.
含不确定参数的复合材料板振动的 区间分析法 总被引:7,自引:2,他引:5
提出了求解具有不确定参数的复合材料板的振动固有频率区间分析法.区间分析法利用区间数学和泰勒定理,把不确定变量简化为区间向量.这样可以在较少的结构信息的情况下确定结构响应的变化区间.在样本比较小,概率统计特性缺乏,从而通常的概率统计方法不能有效应用时,区间分析仍然有效. 对复合材料板的振动固有频率的区间法公式进行了推导,并用2个数值例子与凸模型方法的解进行比较.结果表明区间分析法比凸模型方法的解区间小. 相似文献
638.
一种磁悬浮飞轮用新型永磁偏置径向磁轴承 总被引:10,自引:1,他引:9
为了克服现有永磁偏置径向混合磁轴承的缺陷,提出了一种磁悬浮飞轮用新型永磁偏置径向混合磁轴承,分析了其工作原理,并分别利用等效磁路法及有限元方法对该永磁偏置径向混合磁轴承进行了电磁分析.分析结果表明:所提出的新型永磁偏置径向混合磁轴承采用永磁磁场作为偏置磁场,并且其永磁磁路与电励磁磁路在任一径向截面中共面,可使磁轴承轴向长度大为减小,与现有永磁偏置径向混合磁轴承相比具有体积更小的优点,同时该种永磁偏置径向混合磁轴承产生的偏置磁场在X,Y方向上不会产生耦合,可使控制更加容易,特别适用于高速、低功耗等场合. 相似文献
639.
现阶段粘土制品在大部分城市被禁用,作者结合实际工程经验对可供选择的砌体材料做出介绍,并对高烈度区砌体结构的抗震措施及发展方向进行讨论. 相似文献
640.