全文获取类型
收费全文 | 789篇 |
免费 | 122篇 |
国内免费 | 165篇 |
专业分类
航空 | 542篇 |
航天技术 | 295篇 |
综合类 | 95篇 |
航天 | 144篇 |
出版年
2024年 | 4篇 |
2023年 | 7篇 |
2022年 | 18篇 |
2021年 | 31篇 |
2020年 | 39篇 |
2019年 | 45篇 |
2018年 | 70篇 |
2017年 | 49篇 |
2016年 | 51篇 |
2015年 | 27篇 |
2014年 | 44篇 |
2013年 | 43篇 |
2012年 | 40篇 |
2011年 | 61篇 |
2010年 | 51篇 |
2009年 | 53篇 |
2008年 | 59篇 |
2007年 | 44篇 |
2006年 | 63篇 |
2005年 | 49篇 |
2004年 | 30篇 |
2003年 | 37篇 |
2002年 | 17篇 |
2001年 | 14篇 |
2000年 | 17篇 |
1999年 | 9篇 |
1998年 | 15篇 |
1997年 | 13篇 |
1996年 | 13篇 |
1995年 | 12篇 |
1994年 | 16篇 |
1993年 | 6篇 |
1992年 | 9篇 |
1991年 | 6篇 |
1990年 | 6篇 |
1989年 | 4篇 |
1988年 | 2篇 |
1984年 | 2篇 |
排序方式: 共有1076条查询结果,搜索用时 640 毫秒
31.
惯性测量单元(IMU)是位置姿态系统(POS)的核心部分,IMU的精度很大程度上决定着POS精度.由于高精度光纤陀螺(FOG)的光纤线圈对磁场敏感,基于高精度FOG的IMU精度会受磁场影响而降低.本文研究了FOG磁敏感性机理,通过实验得出高精度光纤IMU对磁场敏感的结论.采用电磁场有限元分析软件Ansoft Maxwe... 相似文献
32.
进气条件对压气机中介机匣流场影响的试验研究 总被引:5,自引:1,他引:5
以某压气机中介机匣为试验研究对象,通过改变来流径向分布与马赫数,建立了评估中介机匣气动性能的进口约束条件。在同步测量轴向流路离散压力参数的基础上,分析了中介机匣内部流场对进气条件的稳态响应。研究结果表明:进气条件对中介机匣流动损失影响较大,与均匀进气相比,进气畸变会增大弯曲流道内部径向压力梯度,影响流道曲率与流向压力梯度对附面层的控制效果;支板尾流对通道主流的干扰导致下游平直流道上部区域流场恶化,而进气畸变会加剧支板尾迹的影响;随着进口马赫数的增大,中介机匣总压损失系数与总压畸变强度呈现出不同的增长趋势,其出口流场径向分布对马赫数变化的气动敏感性较高。 相似文献
33.
DAI Yao TAN Wei SUN Qi SUN Chang-qing 《中国航空学报》2006,19(B12):248-251
Usually, it is very difficult to find out an analytical solution to thermal conduction problems during high temperature welding. Therefore, as an important numerical approach, the method of lines (MOLs) is introduced to solve the temperature field characterized by high gradients. The basic idea of the method is to semi-discretize the governing equation of the problem into a system of ordinary differential equations (ODEs) defined on discrete lines by means of the finite difference method, by which the thermal boundary condition with high gradients are directly embodied in formulation. Thus the temperature field can be obtained by solving the ODEs. As a numerical example, the variation of an axisymmetrical temperature field along the plate thickness can be obtained. 相似文献
34.
A. G. Yahnin I. V. Despirak A. A. Lubchich B. V. Kozelov N. P. Dmitrieva M. A. Shukhtina H. K Biernat 《Space Science Reviews》2006,122(1-4):97-106
Although the auroral substorm has been long regarded as a manifestation of the magnetospheric substorm, a direct relation
of active auroras to certain magnetospheric processes is still debatable. To investigate the relationship, we combine the
data of the UV imager onboard the Polar satellite with plasma and magnetic field measurements by the Geotail spacecraft. The
poleward edge of the auroral bulge, as determined from the images obtained at the LHBL passband, is found to be conjugated
with the region where the oppositely directed fast plasma flows observed in the near-Earth plasma sheet during substorms are
generated. We conclude that the auroras forming the bulge are due to the near-Earth reconnection process. This implies that
the magnetic flux through the auroral bulge is equal to the flux dissipated in the magnetotail during the substorm. Comparison
of the magnetic flux through the auroral bulge with the magnetic flux accumulated in the tail lobe during the growth phase
shows that these parameters have the comparable values. This is a clear evidence of the loading–unloading scheme of substorm
development. It is shown that the area of the auroral bulge developing during substorm is proportional to the total (magnetic
plus plasma) pressure decrease in the magnetotail. These findings stress the importance of auroral bulge observations for
monitoring of substorm intensity in terms of the magnetic flux and energy dissipation. 相似文献
35.
Coronal mass ejections and post-shock streams driven by them are the most efficient drivers of strong magnetospheric activity,
magnetic storms. For this reason there is considerable interest in trying to make reliable forecasts for the effects of CMEs
as much in advance as possible. To succeed this requires understanding of all aspects related to CMEs, starting from their
emergence on the Sun to their propagation to the vicinity of the Earth and to effects within the magnetosphere. In this article
we discuss some recent results on the geoeffectivity of different types of CME/shock structures. A particularly intriguing
observation is that smoothly rotating magnetic fields within CMEs are most efficient in driving storm activity seen in the
inner magnetosphere due to enhanced ring current, whereas the sheath regions between the shock and the ejecta tend to favour
high-latitude activity. 相似文献
36.
基于磁悬浮助推技术概念研究方案建立了一套悬浮加速缩比试验系统.从整体缩比模型振动试验出发,主要研究悬浮质量以及悬浮刚度对整体系统动态性能的影响,并在进行缩比单元动态试验结论的基础上,建立试验模型的加速试验动态采集系统,对整体模型进行运行性能试验.在试验基础上提出了提高磁悬浮推进系统运行稳定性的依据,并据此提出相应可行的解决方案设想.通过模型加速试验并采集试验数据定性分析磁浮系统的综合运动性能,以更好地评估系统稳定特性和品质,也为进一步研究磁悬浮助推发射的气动、分离系统稳定性和可靠性提供参考. 相似文献
37.
文章在介绍某型电压限定器工作原理的基础上,阐述了利用集成电路技术和自动控制技术进行该型电压限定器国产化研制的方法,给出了电压限定器探测及延时电路、均衡控制电路、防止误动作保护电路的详细设计方案,解决了激磁控制、均衡控制、故障鉴别等国产化研制过程中遇到的问题,保证了新研制产品与原有进口产品的可互换使用,提高了设备的工作可靠性。 相似文献
38.
39.
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
40.
建立正确合理的重力梯度测量模型对于实现重力梯度测量具有重要作用。本文从动力学基本原理和牛顿第二定律出发,推导了加速度计敏感轴分别沿转盘切线方向和转盘转轴方向安装时,加速度计的输出与重力梯度张量间的关系式,式中的各项均具有对应的物理含义,可通过直接测量或计算得到。本文还利用仿真模型对新的重力梯度全张量的测量方式的可行性进行了分析,结果表明,利用新的测量方式计算得到的“伪测量值”与理论计算值间的误差小于1E,证明该测量方式是可行的。最后,论文讨论了这种新测量方式在实际应用中可能出现的问题及解决方案。 相似文献