全文获取类型
收费全文 | 308篇 |
免费 | 33篇 |
国内免费 | 42篇 |
专业分类
航空 | 232篇 |
航天技术 | 79篇 |
综合类 | 45篇 |
航天 | 27篇 |
出版年
2024年 | 1篇 |
2023年 | 8篇 |
2022年 | 10篇 |
2021年 | 4篇 |
2020年 | 9篇 |
2019年 | 19篇 |
2018年 | 31篇 |
2017年 | 19篇 |
2016年 | 13篇 |
2015年 | 14篇 |
2014年 | 19篇 |
2013年 | 6篇 |
2012年 | 9篇 |
2011年 | 21篇 |
2010年 | 16篇 |
2009年 | 10篇 |
2008年 | 16篇 |
2007年 | 11篇 |
2006年 | 18篇 |
2005年 | 25篇 |
2004年 | 10篇 |
2003年 | 11篇 |
2002年 | 8篇 |
2001年 | 5篇 |
2000年 | 7篇 |
1999年 | 21篇 |
1998年 | 7篇 |
1997年 | 1篇 |
1996年 | 1篇 |
1995年 | 7篇 |
1994年 | 14篇 |
1993年 | 1篇 |
1992年 | 2篇 |
1991年 | 3篇 |
1990年 | 3篇 |
1989年 | 1篇 |
1988年 | 2篇 |
排序方式: 共有383条查询结果,搜索用时 31 毫秒
11.
12.
阐述航空高压270V稀土永磁直流电动机的设计原则、工艺措施及计算和试验结果。解决了高空换向难题之后电动机能满足航空电机的技术要求,采用传统的有刷结构是完全可行的。 相似文献
13.
Profiles of the visible Fe X (6374 Å) coronal emission line as a function of height above the limb were obtained out to 1.16 solar radii in a coronal hole using the NSO/Sacramento Peak Observatory Coronagraph, Universal Spectrograph and a CCD camera. These are the first coronal line profiles obtained as a function of height in a coronal hole from the ground. Analysis of the line widths suggests a large component of nonthermal broadening which increases with height ranging from 40 to 60 km/s, depending upon the assumed temperature or thermal component of the profile. 相似文献
14.
过滤式阴极电弧沉积类金刚石薄膜工艺研究 总被引:3,自引:0,他引:3
研究了过滤式阴极电弧沉积系统的稳弧工艺参数,通过正交试验获得最佳稳弧参数。并且研究了弯管内置挡板对宏观粒子过滤效果的影响。采用喇曼光谱研究了偏压对生成的类金刚石薄膜性能的影响,证明-100V偏压下获得的类金刚石薄膜有最佳的SP3含量。扫描电镜测试表明,在(111)硅基片上获得致密的膜,但在高速钢基体上沉膜堆积现象比较严重,不易获得优质类金刚石膜。同时也给出了类金刚石的原子力显微照片(AFM),表明稳弧参数对类金刚石薄膜表面形貌有较大的影响。 相似文献
15.
T. Van Doorsselaere I. Arregui J. Andries M. Goossens S. Poedts 《Space Science Reviews》2005,121(1-4):79-89
We will discuss the observed, heavily damped transversal oscillations of coronal loops. These oscillations are often modeled
as transversal kink oscillations in a cylinder. Several features are added to the classical cylindrical model. In our models
we include loop curvature, longitudinal density stratification, and highly inhomogeneous radial density profiles.
In this paper, we will first give an overview of recently obtained results, both analytically and numerically. After that,
we shed a light on the computational aspects of the modeling process. In particular, we will focus on the parallellization
of the numerical codes. 相似文献
16.
Yihua Yan 《Space Science Reviews》2005,121(1-4):213-221
The coronal magnetic field configuration is important for understanding the energy storage and release processes that account
for flares and/or CMEs. Here we present a model which is based on the work for potential magnetic field problems that only
applies the condition at infinity with the boundary condition on the solar surface specified. We also discuss some recent
progress on general force-free field models. For some event analyses, we have employed MDI/SOHO longitudinal magnetogram insected
into the synoptic magnetogram to obtain whole boundary condition over the solar surface. Globally, the extrapolated global
magnetic field structures effectively demonstrate the case for the disk signature of the radio CMEs and the evolution of the
radio sources during the CME/flare processes. 相似文献
17.
分析了直流电阻分压箱的技术指标和校准水平,提出了等分测量的校准方法,进行了不确定度分析,给出了验证方法。结果表明:用该方法校准的分压箱,比率误差为10^-7量级。 相似文献
18.
电火花线切割加工中放电间隙电压变化特性 总被引:2,自引:0,他引:2
电火花线切割加工时工具(电极丝)和工件之间的放电电压是对放电加工过程进行实时检测的重要参数.本文在理论分析的基础上,采用正交试验设计,应用极差分析法和方差分析法定量研究了高速走丝电火花线切割加工中放电间隙电压量的变化特性与加工中峰值电流、工件厚度及切割方向之间的关系.研究的结果为准确检测高速走丝电火花线切割加工状态提供了依据. 相似文献
19.
20.
J. C. Raymond 《Space Science Reviews》1999,87(1-2):55-66
Order of magnitude variations in relative elemental abundances are observed in the solar corona and solar wind. The instruments
aboard SOHO make it possible to explore these variations in detail to determine whether they arise near the solar surface
or higher in the corona. A substantial enhancement of low First Ionization Potential (FIP) elements relative to high FIP elements
is often seen in both the corona and the solar wind, and that must arise in the chromosphere. Several theoretical models have
been put forward to account for the FIP effect, but as yet even the basic physical mechanism responsible remains an open question.
Evidence for gravitational settling is also found at larger heights in quiescent streamers. The question is why the heavier
elements don't settle out completely.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献