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   25451篇
  免费   438篇
  国内免费   315篇
测绘学   722篇
大气科学   1798篇
地球物理   4876篇
地质学   8804篇
海洋学   2299篇
天文学   6341篇
综合类   51篇
自然地理   1313篇
  2021年   199篇
  2020年   237篇
  2019年   301篇
  2018年   606篇
  2017年   586篇
  2016年   728篇
  2015年   419篇
  2014年   698篇
  2013年   1311篇
  2012年   804篇
  2011年   1049篇
  2010年   963篇
  2009年   1262篇
  2008年   1132篇
  2007年   1160篇
  2006年   1129篇
  2005年   841篇
  2004年   842篇
  2003年   764篇
  2002年   717篇
  2001年   622篇
  2000年   641篇
  1999年   565篇
  1998年   554篇
  1997年   523篇
  1996年   398篇
  1995年   397篇
  1994年   409篇
  1993年   315篇
  1992年   310篇
  1991年   259篇
  1990年   311篇
  1989年   271篇
  1988年   258篇
  1987年   279篇
  1986年   237篇
  1985年   318篇
  1984年   340篇
  1983年   332篇
  1982年   316篇
  1981年   251篇
  1980年   270篇
  1979年   217篇
  1978年   207篇
  1977年   216篇
  1976年   181篇
  1975年   191篇
  1974年   179篇
  1973年   168篇
  1972年   114篇
排序方式: 共有10000条查询结果,搜索用时 84 毫秒
41.
42.
43.
44.
This paper proposes a multi‐level parallelized substructuring–frontal combined algorithm for the analysis of the problem of thermo/hydraulic/mechanical behaviour of unsaturated soil. Temperature, displacement, pore water pressure and pore air pressure are treated as the primary variables in a non‐linear analysis. Details are given firstly of the substructuring–frontal combined approach. The incorporation of the algorithm in a multi‐level parallel strategy is then discussed. The parallel processing can thus be carried out at different substructural levels. The method thus developed impacts, in a positive way, on both computer storage requirement and execution time. Copyright © 2003 John Wiley & Sons, Ltd.  相似文献   
45.
46.
47.
48.
Abstract— In 2006, the Stardust spacecraft will return to Earth with cometary and perhaps interstellar dust particles embedded in silica aerogel collectors for analysis in terrestrial laboratories. These particles will be the first sample return from a solid planetary body since the Apollo missions. In preparation for the return, analogue particles were implanted into a keystone of silica aerogel that had been extracted from bulk silica aerogel using the optical technique described in Westphal et al. (2004). These particles were subsequently analyzed using analytical techniques associated with the use of a nuclear microprobe. The particles have been analyzed using: a) scanning transmission ion microscopy (STIM) that enables quantitative density imaging; b) proton elastic scattering analysis (PESA) and proton backscattering (PBS) for the detection of light elements including hydrogen; and c) proton‐induced X‐ray emission (PIXE) for elements with Z > 11. These analytical techniques have enabled us to quantify the composition of the encapsulated particles. A significant observation from the study is the variable column density of the silica aerogel. We also observed organic contamination within the silica aerogel. The implanted particles were then subjected to focused ion beam (FIB) milling using a 30 keV gallium ion beam to ablate silica aerogel in site‐specific areas to expose embedded particles. An ion polished flat surface of one of the particles was also prepared using the FIB. Here, we show that ion beam techniques have great potential in assisting with the analysis and exposure of Stardust particles.  相似文献   
49.
Using photoclinometry, topographic profiles across europan ridges have been produced. These profiles allow the identification of bulges in the terrain adjacent to the ridges. The bulges are assumed to have been produced by flexure of the elastic lithosphere due to the load of the ridges, which lie along cracks in the crust. The distance from the crack to these “fore-bulges” depends on the thickness of the elastic plate being flexed. Based on a survey of ridges in Galileo images with resolution <300 m/pixel, the thickness of the elastic lithosphere has been determined by this method at a wide variety of sites along the leading and trailing hemispheres of Europa. The average thickness is about 200 m. The elastic lithosphere underneath smooth dilational bands tends to be thicker than plains morphology, an effect that is pronounced at Thynia Linea and Astypalaea Linea. Among the ridges investigated here, more recent loading correlates with a thicker elastic lithosphere, which may either reflect an intrinsically thicker layer, or less viscous relaxation over the shorter time period.  相似文献   
50.
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