全文获取类型
收费全文 | 323篇 |
免费 | 81篇 |
国内免费 | 109篇 |
专业分类
航空 | 279篇 |
航天技术 | 108篇 |
综合类 | 52篇 |
航天 | 74篇 |
出版年
2024年 | 1篇 |
2023年 | 3篇 |
2022年 | 12篇 |
2021年 | 24篇 |
2020年 | 26篇 |
2019年 | 23篇 |
2018年 | 26篇 |
2017年 | 19篇 |
2016年 | 21篇 |
2015年 | 24篇 |
2014年 | 18篇 |
2013年 | 16篇 |
2012年 | 15篇 |
2011年 | 22篇 |
2010年 | 22篇 |
2009年 | 21篇 |
2008年 | 13篇 |
2007年 | 17篇 |
2006年 | 28篇 |
2005年 | 22篇 |
2004年 | 10篇 |
2003年 | 19篇 |
2002年 | 8篇 |
2001年 | 21篇 |
2000年 | 16篇 |
1999年 | 17篇 |
1998年 | 14篇 |
1997年 | 4篇 |
1996年 | 6篇 |
1995年 | 7篇 |
1994年 | 8篇 |
1992年 | 4篇 |
1991年 | 4篇 |
1990年 | 1篇 |
1989年 | 1篇 |
排序方式: 共有513条查询结果,搜索用时 31 毫秒
31.
Yingtai Chen Yumin Li Hong Zhang Yi Xie Xuezhong Chen Jinyu Ren Xiaowei Zhang Zijiang Zhu Hongliang Liu Yawei Zhang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
The aim of this study was to estimate the acute effects of low dose 12C6+ ions or X-ray radiation on human immune function. The human peripheral blood lymphocytes (HPBL) of seven healthy donors were exposed to 0.05 Gy 12C6+ ions or X-ray radiation and cell responses were measured at 24 h after exposure. The cytotoxic activities of HPBL were determined by 3-(4,5-dimethylthiazol-2-yl)-2,5-diphenyl tetrazolium bromide (MTT); the percentages of T and NK cells subsets were detected by flow cytometry; mRNA expression of interleukin (IL)-2, tumor necrosis factor (TNF)-α and interferon (IFN)-γ were examined by real time quantitative RT-PCR (qRT-PCR); and these cytokines protein levels in supernatant of cultured cells were assayed by enzyme-linked immunosorbent assays (ELISA). The results showed that the cytotoxic activity of HPBL, mRNA expression of IL-2, IFN-γ and TNF-α in HPBL and their protein levels in supernatant were significantly increased at 24 h after exposure to 0.05 Gy 12C6+ ions radiation and the effects were stronger than observed for X-ray exposure. However, there was no significant change in the percentage of T and NK cells subsets of HPBL. These results suggested that 0.05 Gy high linear energy transfer (LET) 12C6+ radiation was a more effective approach to host immune enhancement than that of low LET X-ray. We conclude that cytokines production might be used as sensitive indicators of acute response to LDI. 相似文献
32.
用共振Rayleigh散射(RRS)光谱研究了酸性磺酞类染料溴甲酚绿和溴酚蓝分别与奈替米星的相互作用.溴甲酚绿和溴酚蓝在酸性介质中分别与奈替米星相互作用,导致RRS光谱显著增强,最大的RRS峰分别位于606nm和572nm处,散射强度与奈替米星的质量浓度在一定的范围内成正比.此方法具有很高的灵敏度,对于奈替米星的检测限(3σ)分别为30ng/mL和10ng/mL,据此发展了一种测定奈替米星的新方法. 相似文献
33.
34.
Using empirical velocity distributions derived from UVCS and SUMER ultraviolet spectroscopy, we construct theoretical models
of anisotropic ion temperatures in the polar solar corona. The primary energy deposition mechanism we investigate is the dissipation
of high frequency (10-10000 Hz) ion-cyclotron resonant Alfvén waves which can heat and accelerate ions differently depending
on their charge and mass. We find that it is possible to explain the observed high perpendicular temperatures and strong anisotropies
with relatively small amplitudes for the resonant waves. There is suggestive evidence for steepening of the Alfvén wave spectrum
between the coronal base and the largest heights observed spectroscopically. Because the ion-cyclotron wave dissipation is
rapid, even for minor ions like O5+, the observed extended heating seems to demand a constantly replenished population of waves over several solar radii. This
indicates that the waves are generated gradually throughout the wind rather than propagated up from the base of the corona.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
35.
本文作者所设计的实验是利用光学中全反射衰减特性方法测量在介质上蒸镀的金属薄膜的厚度和各种频率下的复介电常数等物理性质,它可以精确测定100~1000范围内金属膜层的厚度和ε(ω)值,以及一些其它性质,是研究固体表面物理的一种有效的方法和技术。 相似文献
36.
37.
38.
Pekka Janhunen Annika Olsson Christopher T. Russell Harri Laakso 《Space Science Reviews》2006,122(1-4):89-95
Auroral emission caused by electron precipitation (Hardy et al., 1987, J. Geophys. Res. 92, 12275–12294) is powered by magnetospheric driving processes. It is not yet fully understood how the energy transfer mechanisms
are responsible for the electron precipitation. It has been proposed (Hasegawa, 1976, J. Geophys. Res. 81, 5083–5090) that Alfvén waves coming from the magnetosphere play some role in powering the aurora (Wygant et al., 2000, J. Geophys. Res. 105, 18675–18692, Keiling et al., 2003, Science
299, 383–386). Alfvén-wave-induced electron acceleration is shown to be confined in a rather narrow radial distance range of
4–5 R
E
(Earth radii) and its importance, relative to other electron acceleration mechanisms, depends strongly on the magnetic disturbance
level so that it represents 10% of all electron precipitation power during quiet conditions and increased to 40% during disturbed
conditions. Our observations suggest that an electron Landau resonance mechanism operating in the “Alfvén resonosphere” is
responsible for the energy transfer. 相似文献
39.
40.
蔡霞 《西安航空技术高等专科学校学报》2004,22(5):39-40,49
关于公差原则中的相关要求的计算问题 ,本文提出了两种方法 :计算法和图解法。运用这两种方法可以简化此类问题的计算过程 ,准确求得计算结果。 相似文献