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   7115篇
  免费   18篇
  国内免费   38篇
航空   3297篇
航天技术   2631篇
综合类   27篇
航天   1216篇
  2021年   67篇
  2019年   47篇
  2018年   141篇
  2017年   95篇
  2016年   82篇
  2015年   34篇
  2014年   158篇
  2013年   194篇
  2012年   185篇
  2011年   280篇
  2010年   188篇
  2009年   305篇
  2008年   360篇
  2007年   197篇
  2006年   170篇
  2005年   206篇
  2004年   206篇
  2003年   237篇
  2002年   144篇
  2001年   223篇
  2000年   149篇
  1999年   169篇
  1998年   198篇
  1997年   147篇
  1996年   185篇
  1995年   241篇
  1994年   216篇
  1993年   124篇
  1992年   182篇
  1991年   71篇
  1990年   67篇
  1989年   155篇
  1988年   60篇
  1987年   57篇
  1986年   73篇
  1985年   228篇
  1984年   174篇
  1983年   140篇
  1982年   178篇
  1981年   207篇
  1980年   63篇
  1979年   50篇
  1978年   59篇
  1977年   54篇
  1976年   46篇
  1975年   43篇
  1974年   52篇
  1972年   34篇
  1970年   40篇
  1969年   39篇
排序方式: 共有7171条查询结果,搜索用时 453 毫秒
321.
We analyzed high-angular rate streaks first recorded by OSIRIS-REx’s MapCam during a 2017 search for Earth Trojan asteroids. We interpret them as water-ice particles that translated across the imager’s field of view, originating from the spacecraft itself. Their translation velocities approximated 0.1–1?m/s based on reasonable conclusions about their range. Pursuing several lines of investigation to seek a coherent hypothesis, we conclude that the episodic releases of the water ice particles are associated with spacecraft attitudes that resulted in solar illumination of previously shadowed regions. This correlation suggests that the OSIRIS-REx spacecraft itself possesses micro-climatic zones consisting of hot regions and cold traps that may temporarily potentially pass volatiles back and forth before losing most of them.  相似文献   
322.
The distribution of chemical elements in the hot intracluster medium (ICM) retains valuable information about the enrichment and star formation histories of galaxy clusters, and on the feedback and dynamical processes driving the evolution of the cosmic baryons. In the present study we review the progresses made so far in the modelling of the ICM chemical enrichment in a cosmological context, focusing in particular on cosmological hydrodynamical simulations. We will review the key aspects of embedding chemical evolution models into hydrodynamical simulations, with special attention to the crucial assumptions on the initial stellar mass function, stellar lifetimes and metal yields, and to the numerical limitations of the modelling. At a second stage, we will overview the main simulation results obtained in the last decades and compare them to X-ray observations of the ICM enrichment patterns. In particular, we will discuss how state-of-the-art simulations are able to reproduce the observed radial distribution of metals in the ICM, from the core to the outskirts, the chemical diversity depending on cluster thermo-dynamical properties, the evolution of ICM metallicity and its dependency on the system mass from group to cluster scales. Finally, we will discuss the limitations still present in modern cosmological, chemical, hydrodynamical simulations and the perspectives for improving the theoretical modelling of the ICM enrichment in galaxy clusters in the future.  相似文献   
323.
324.
The vortical mixing concept in the ramjet channel is analyzed. The results of simulating the gasodynamic scheme permit the concept of increasing efficiency for ramjet operation to be substantiated.  相似文献   
325.
The bearing capacity of hybrid segmented bearings with different groove systems is compared. The research establishes that the system with a crescent groove has the best characteristics.  相似文献   
326.
This paper studies an auroral event using data from three spacecraft of the Cluster mission, one inside and two at the poleward edge of the bottom of the Auroral Acceleration Region (AAR). The study reveals the three-dimensional profile of the region’s poleward boundary, showing spatial segmentation of the electric potential structures and their decay in time. It also depicts localized magnetic field variations and field-aligned currents that appear to have remained stable for at least 80?s. Such observations became possible due to the fortuitous motion of the three spacecraft nearly parallel to each other and tangential to the AAR edge, so that the differences and variations can be seen when the spacecraft enter and exit the segmentations, hence revealing their position with respect to the AAR.  相似文献   
327.
328.
329.
330.
Space Science Reviews - Time measured by an ideal clock crucially depends on the gravitational potential and velocity of the clock according to general relativity. Technological advances in...  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