首页 | 本学科首页   官方微博 | 高级检索  
文章检索
  按 检索   检索词:      
出版年份:   被引次数:   他引次数: 提示:输入*表示无穷大
  收费全文   10581篇
  免费   1913篇
  国内免费   2006篇
航空   9262篇
航天技术   1696篇
综合类   1619篇
航天   1923篇
  2024年   29篇
  2023年   182篇
  2022年   356篇
  2021年   403篇
  2020年   405篇
  2019年   421篇
  2018年   410篇
  2017年   426篇
  2016年   527篇
  2015年   492篇
  2014年   658篇
  2013年   551篇
  2012年   695篇
  2011年   821篇
  2010年   573篇
  2009年   643篇
  2008年   656篇
  2007年   670篇
  2006年   643篇
  2005年   557篇
  2004年   477篇
  2003年   450篇
  2002年   408篇
  2001年   369篇
  2000年   349篇
  1999年   269篇
  1998年   253篇
  1997年   233篇
  1996年   249篇
  1995年   184篇
  1994年   208篇
  1993年   182篇
  1992年   169篇
  1991年   168篇
  1990年   143篇
  1989年   133篇
  1988年   105篇
  1987年   19篇
  1986年   2篇
  1985年   2篇
  1984年   10篇
排序方式: 共有10000条查询结果,搜索用时 93 毫秒
991.
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   
992.
圆球绕流场的尾涡分析和升阻力研究   总被引:5,自引:0,他引:5  
采用自编的分块算法程序模拟了雷诺数在20~1000之间的圆球绕流场.在Re=25时捕捉到流动分离,与试验结果一致.对Re=250时稳态非对称尾流区内流体的输运情况进行研究,证实圆球绕流场中纵向对称面的存在.对于非稳态流动,主要研究了阻力和横向力的时间变化规律,并分析了频谱特征.计算发现横向合力主要在横截面上两个很窄的区间内偏移.经过几种不同涡定义方法的优劣测试,本文采用Hunt等人介绍的Q-定义方法对非稳态绕流场的尾涡结构进行了直观描述.  相似文献   
993.
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   
994.
我国物流标准化存在的问题及对策   总被引:1,自引:0,他引:1  
当前我国物流标准化存在以下问题:总体发展滞后、基础薄弱、体制"瓶颈"、采用国际标准少、对行政力量过于依赖,等等.解决的对策有:发挥政府部门作用、加快体系研究、借签国外经验、发挥行业协会作用、加大宣传力度,等等.  相似文献   
995.
低量值直流电流表检定及测量不确定度评定   总被引:1,自引:0,他引:1  
详细地叙述了利用XF1b型交、直流精密电表校验装置采用直流补偿法检定低量值直流电流表示值误差时所存在的问题,并提出一种改进线路。同时,按照JJF1059—1999《测量不确定度评定与表示》规范的要求对上述方法中所阐述的低量值直流电流表示值误差测量结果的不确定度进行了评定。  相似文献   
996.
To compute transonic flows over a complex 3D aircraft configuration, a viscous/inviscid interaction method is developed by coupling an integral boundary-layer solver with an Eluer solver in a "semi-inverse" manner. For the turbulent boundary-layer, an integral method using Green's lag equation is coupled with the outer inviscid flow. A blowing velocity approach is used to simulate the displacement effects of the boundary layer. To predict the aerodynamic drag, it is developed a numerical technique called far-field method that is based on the momentum theorem, in which the total drag is divided into three component drags, i.e. viscous, induced and wave-formed. Consequently, it can provide more physical insight into the drag sources than the often-used surface integral technique. The drag decomposition can be achieved with help of the second law of thermodynamics, which implies that entropy increases and total pressure decreases only across shock wave along a streamline of an inviscid non-isentropic flow. This method has been applied to the DLR-F4 wing/body configuration showing results in good agreement with the wind tunnel data.  相似文献   
997.
Non-thermal components are key ingredients for understanding clusters of galaxies. In the hierarchical model of structure formation, shocks and large-scale turbulence are unavoidable in the cluster formation processes. Understanding the amplification and evolution of the magnetic field in galaxy clusters is necessary for modelling both the heat transport and the dissipative processes in the hot intra-cluster plasma. The acceleration, transport and interactions of non-thermal energetic particles are essential for modelling the observed emissions. Therefore, the inclusion of the non-thermal components will be mandatory for simulating accurately the global dynamical processes in clusters. In this review, we summarise the results obtained with the simulations of the formation of galaxy clusters which address the issues of shocks, magnetic field, cosmic ray particles and turbulence.  相似文献   
998.
Microsoft Access 2000数据库作为常用的桌面数据库软件,在中小型的数据库系统中得到了广泛的应用。针对Access2000安全性能不高,探讨如何设置及提高Access2000的安全性方法。  相似文献   
999.
关于网络伦理问题的研究与思考   总被引:1,自引:0,他引:1  
人类进入21世纪,人们感受到了信息技术给人类的交往、学习、工作和生活带来极大便利,促进了人的全面发展和社会进步。但也出现了网络“道德真空”和“道德沦丧”,因此关于网络伦理问题的研究也就摆在了我们面前。  相似文献   
1000.
基于集群系统(CLUSTER),在Linux和MPI并行环境下,研究了带制退器的复杂膛口流场三维数值模拟并行算法。计算网格是三维多区结构化网格,数值格式采用Jameson格式及LU隐式分解方法。针对流场的复杂拓扑结构,建立分区信息文件记录各分区的相关信息,并提出了通过合并相邻网格分区的方法均衡各个进程的负载,提高程序的并行效率。在处理需要通讯的信息时,设计了自定义数据类型和"设置中间参数"相结合的方法,并通过动态分配内存减少了程序对计算机系统资源的占用。数值实验表明,本文设计的算法可以适应拓扑结构较复杂的流场,并能取得理想的并行效率,将有助于制退器性能的研究。  相似文献   
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号