全文获取类型
收费全文 | 929篇 |
免费 | 138篇 |
国内免费 | 143篇 |
专业分类
航空 | 566篇 |
航天技术 | 324篇 |
综合类 | 115篇 |
航天 | 205篇 |
出版年
2024年 | 1篇 |
2023年 | 11篇 |
2022年 | 17篇 |
2021年 | 21篇 |
2020年 | 30篇 |
2019年 | 51篇 |
2018年 | 67篇 |
2017年 | 57篇 |
2016年 | 44篇 |
2015年 | 42篇 |
2014年 | 50篇 |
2013年 | 33篇 |
2012年 | 59篇 |
2011年 | 77篇 |
2010年 | 53篇 |
2009年 | 64篇 |
2008年 | 60篇 |
2007年 | 46篇 |
2006年 | 73篇 |
2005年 | 51篇 |
2004年 | 41篇 |
2003年 | 41篇 |
2002年 | 28篇 |
2001年 | 24篇 |
2000年 | 26篇 |
1999年 | 15篇 |
1998年 | 19篇 |
1997年 | 11篇 |
1996年 | 11篇 |
1995年 | 18篇 |
1994年 | 15篇 |
1993年 | 14篇 |
1992年 | 7篇 |
1991年 | 9篇 |
1990年 | 8篇 |
1989年 | 8篇 |
1988年 | 3篇 |
1987年 | 2篇 |
1986年 | 1篇 |
1984年 | 2篇 |
排序方式: 共有1210条查询结果,搜索用时 31 毫秒
161.
H.N. Wang Y.M. Cui R. Li L.Y. Zhang H. Han 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,42(9):1464-1468
Nowadays operational models for solar activity forecasting are still based on the statistical relationship between solar activity and solar magnetic field evolution. In order to set up this relationship, many parameters have been proposed to be the measures. Conventional measures are based on the sunspot group classification which provides limited information from sunspots. For this reason, new measures based on solar magnetic field observations are proposed and a solar flare forecasting model supported with an artificial neural network is introduced. This model is equivalent to a person with a long period of solar flare forecasting experience. 相似文献
162.
依据光学电子学的相关原理,针对烟草行业自动生产过程中对传感器的需要,研制了WL10型近红外反射光电传感器,并成功地应用于烟草行业的生产线上。 相似文献
163.
二值箝位电路的理论分析及仿真研究 总被引:1,自引:0,他引:1
在CCD焦面驱动电路设计中,经常要求产生在两个指定电平间振荡的信号,二值箝位电路以其简单的拓扑结构、稳定的性能表现而得到应用。尽管二值箝位电路的稳态输出仅受拓扑结构影响,而与初始条件无关,然而其暂态输出会随着初始条件以及拓扑结构的不同而有所差异,造成二值箝位电路设计及其应用的复杂性,文章深入地研究二值箝位电路不同的拓扑结构以及不同的输入条件对其输出的影响,给出了各种情况下的仿真结果,并针对仿真结果给出了定量和定性的分析。 相似文献
164.
王友敬 《中国民航学院学报》1998,16(4):21-26
就磁转速表活动系统的动态特性以及在附加交变力矩的作用下,指针摆动随转速变化的规律,从理论上进行了分析,并结合实际探讨了指针摆动的故障原因。 相似文献
165.
M. Tátrallyay G. Erdős A. Balogh I. Dandouras 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(10):1537-1544
Two orbits were selected in January–February 2006 when the separation between the Cluster spacecraft was large and mirror type magnetic field fluctuations were observed by all spacecraft in different regions of the terrestrial magnetosheath. Minimum variance analysis was applied to find the mirror type fluctuations, and the amplitude of the fluctuations was determined individually. Mirror mode structures are moving along the streamlines frozen in the plasma. A model was developed for the calculation of plasma flowtime from the bow shock to the observation point. The growth rate of the field strength perturbations was estimated by comparing the amplitudes of fluctuations observed simultaneously at distant locations (∼10,000 km) based on the assumption that δB ∼ exp(γt). The obtained growth rate values were about an order of magnitude smaller than those provided by linear models and they decreased in the inner regions of the magnetosheath, indicating some saturation in the growth of the waves when proceeding towards the magnetopause. The results of these two case studies suggest that mirror type fluctuations originate from the compression region downstream of the quasi-perpendicular bow shock, and the growth of the fluctuations cannot be described by linear approximations. 相似文献
166.
Large-scale Coronal Heating, Clustering of Coronal Bright Points, and Concentration of Magnetic Flux
By combining quiet-region Fe XII coronal images from SOHO/EIT with magnetograms from NSO/Kitt Peak and from SOHO/MDI, we show
that the population of network coronal bright points and the magnetic flux content of the network are both markedly greater
under the bright half of the large-scale quiet corona than under the dim half. These results (1) support the view that the
heating of the entire corona in quiet regions and coronal holes is driven by fine-scale magnetic activity (microflares, explosive
events, spicules) seated low in the magnetic network, and (2) suggest that this large-scale modulation of the magnetic flux
and coronal heating is a signature of giant convection cells.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
167.
任可 《航空精密制造技术》2012,48(4):61-62
针对某型通航飞机地面测试中发现失速警告不工作的故障,分析该失速警告系统各组成部分的结构、原理、功能、走线,制定具体排故程序逐步判断查找出故障原因电子线路故障,并对故障原因进行了分析。 相似文献
168.
在飞机地面通常检查时,磁差给定器磁偏差值往往设定为当地磁差,才能得到正确的航向。校正磁罗差时,只有将磁差给定器设定为000.0,不然罗差计算会大大溢出指标。文章通过磁罗差校正的原理和校正方法的论述,进一步分析了校罗差时将磁偏给定器设定为000.0的工作机理。 相似文献
169.
介绍了一种新型电工钢片磁性能无损检测传感器及其测量原理 ,同时讨论了该传感器的设计原则并给出了典型数据及仿真测试结果 相似文献
170.
S.W. Kahler B.R. Ragot 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
A current serious limitation on the studies of solar energetic particle (SEP) events is that their properties in the inner heliosphere are studied only through in situ spacecraft observations. Our understanding of spatial distributions and temporal variations of SEP events has come through statistical studies of many such events over several solar cycles. In contrast, flare SEPs in the solar corona can be imaged through their radiative and collisional interactions with solar fields and particles. We suggest that the heliospheric SEPs may also interact with heliospheric particles and fields to produce signatures which can be remotely observed and imaged. A challenge with any such candidate signature is to separate it from that of flare SEPs. The optimum case for imaging high-energy (E > 100 MeV) heliospheric protons may be the emission of π0-decay γ-rays following proton collisions with solar wind (SW) ions. In the case of E > 1 MeV electrons, gyrosynchrotron radio emission may be the most readily detectible remote signal. In both cases we may already have observed one or two such events. Another radiative signature from nonthermal particles may be resonant transition radiation, which has likely already been observed from solar flare electrons. We discuss energetic neutrons as another possible remote signature, but we rule out γ-ray line and 0.511 MeV positron annihilation emission as observable signatures of heliospheric energetic ions. We are already acquiring global signatures of large inner-heliospheric SW density features and of heliosheath interactions between the SW and interstellar neutral ions. By finding an appropriate observable signature of remote heliospheric SEPs, we could supplement the in situ observations with global maps of energetic SEP events to provide a comprehensive view of SEP events. 相似文献