全文获取类型
收费全文 | 1220篇 |
免费 | 162篇 |
国内免费 | 302篇 |
专业分类
航空 | 767篇 |
航天技术 | 455篇 |
综合类 | 137篇 |
航天 | 325篇 |
出版年
2024年 | 2篇 |
2023年 | 20篇 |
2022年 | 37篇 |
2021年 | 55篇 |
2020年 | 48篇 |
2019年 | 63篇 |
2018年 | 66篇 |
2017年 | 62篇 |
2016年 | 67篇 |
2015年 | 71篇 |
2014年 | 87篇 |
2013年 | 87篇 |
2012年 | 103篇 |
2011年 | 103篇 |
2010年 | 89篇 |
2009年 | 105篇 |
2008年 | 76篇 |
2007年 | 62篇 |
2006年 | 61篇 |
2005年 | 43篇 |
2004年 | 40篇 |
2003年 | 31篇 |
2002年 | 42篇 |
2001年 | 29篇 |
2000年 | 21篇 |
1999年 | 19篇 |
1998年 | 17篇 |
1997年 | 18篇 |
1996年 | 27篇 |
1995年 | 26篇 |
1994年 | 27篇 |
1993年 | 20篇 |
1992年 | 21篇 |
1991年 | 8篇 |
1990年 | 7篇 |
1989年 | 11篇 |
1988年 | 4篇 |
1987年 | 2篇 |
1984年 | 7篇 |
排序方式: 共有1684条查询结果,搜索用时 15 毫秒
101.
针对实际结构有限元模型(FEM)的建模误差通常仅存在于局部区域,提出了一种对局部结构单独进行模型修正的方法。首先,根据频响函数(FRF)解耦理论得到由残余结构频响函数与包含待修正参数的局部结构动刚度所重构的整体结构频响函数的拟合值,然后通过迭代优化使其与测量值的残差最小化,从而得到参数的极大似然估计。在此基础上,将残差关于参数的灵敏度以局部结构动力学矩阵表示,建立了模型修正的基本方程,利用整体结构的测试数据即可直接对分离出来的局部结构进行模型修正。最后,对喷气式飞机和三角机翼飞机分别进行了数值模拟和实验研究,验证了所提方法的可行性和有效性。结果表明,所提方法可以成功地用于仅局部区域含有建模误差的实际结构有限元模型的修正,修正后的有限元模型的动态特性与实际结构有较好的一致性。 相似文献
102.
G. Stratta A. Pozanenko J.L. Atteia A. Klotz S. Basa B. Gendre F. Verrecchia M. Boër S. Cutini M. Henze S. Holland M. Ibrahimov F. Ienna I. Khamitov S. Klose V. Rumyantsev V. Biryukov F. Vachier S. Arnouts D. Perley 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The detection of a bright optical emission measured with good temporal resolution during the prompt phase makes GRB 060111B a rare event that is especially useful for constraining theories of the prompt optical emission. Comparing this burst with other GRBs with evidence of optical peaks, we find that the optical peak epoch (tp) is anti-correlated with the high energy burst energetic assuming an isotropic energy release (Eiso) in agreement with Liang et al. (2009), and that the steeper is the post-peak afterglow decay, the less is the agreement with the correlation. GRB 060111B is among the latters and it does not match the correlation. The Cannonball scenario is also discussed and we find that this model cannot be excluded for GRB 060111B. 相似文献
103.
Electromagnetic emission induced during concrete fracturing is of great significance to health monitoring of concrete structures.A coupled stress-electricity model is established by analyzing the interaction between stress and electricity during concrete fracturing.And based on this model,the electromagnetic radiation parameters are calculated.The theoretical calculation is well coincident with experimental results.This work provides theoretical support for concrete testing system. 相似文献
104.
噪声污染已成为世界三大污染之一.在工业企业中机床噪声是重要的噪声污染源之一.本文主要从机床的齿轮传动、轴承的选用和齿轮箱的结构等方面对机床噪声产生的影响以及提出相应的降噪措施进行了探讨.从而降低机床噪声,保障工人身心健康,改善车间工作环境. 相似文献
105.
106.
本文分析喷气动力装置的红外辐射源,并讨论抑制红外辐射的技术途径.喷气动力装置的红外辐射来源于燃烧引起的高温,并可区分为两大类:固体表面的辐射和热喷流的辐射.一般而言,抑制红外辐射可从以下三个方面着手:(1)用冷却或绝热的方法降低辐射表面的温度,或通过蔽挡阻止红外辐射的传播;(2)加速喷气流与周围空气的混合,使喷流温度快速降低;(3)降低燃烧产物中辐射成分的浓度. 相似文献
107.
为了确定温度传感器辐射修正校准的准确性,需要对温度传感器辐射修正校准结果进行对比及不确定度分析。本文介绍了在热校准风洞中进行温度传感器辐射修正校准的结果,并做了对比研究和不确定度分析。 相似文献
108.
109.
S. W. Kahler 《Space Science Reviews》2007,129(4):359-390
Electrons with near-relativistic (E≳30 keV, NrR) and relativistic (E≳0.3 MeV) energies are often observed as discrete events in the inner heliosphere following solar transient activity. Several
acceleration mechanisms have been proposed for the production of those electrons. One candidate is acceleration at MHD shocks
driven by coronal mass ejections (CMEs) with speeds ≳1000 km s−1. Many NrR electron events are temporally associated only with flares while others are associated with flares as well as with
CMEs or with radio type II shock waves. Since CME onsets and associated flares are roughly simultaneous, distinguishing the
sources of electron events is a serious challenge. On a phenomenological basis two classes of solar electron events were known
several decades ago, but recent observations have presented a more complex picture. We review early and recent observational
results to deduce different electron event classes and their viable acceleration mechanisms, defined broadly as shocks versus
flares. The NrR and relativistic electrons are treated separately. Topics covered are: solar electron injection delays from
flare impulsive phases; comparisons of electron intensities and spectra with flares, CMEs and accompanying solar energetic
proton (SEP) events; multiple spacecraft observations; two-phase electron events; coronal flares; shock-associated (SA) events;
electron spectral invariance; and solar electron intensity size distributions. This evidence suggests that CME-driven shocks
are statistically the dominant acceleration mechanism of relativistic events, but most NrR electron events result from flares.
Determining the solar origin of a given NrR or relativistic electron event remains a difficult proposition, and suggestions
for future work are given. 相似文献
110.