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   45017篇
  免费   680篇
  国内免费   381篇
测绘学   1352篇
大气科学   3360篇
地球物理   9228篇
地质学   14730篇
海洋学   3943篇
天文学   10915篇
综合类   122篇
自然地理   2428篇
  2021年   358篇
  2020年   396篇
  2019年   480篇
  2018年   1028篇
  2017年   950篇
  2016年   1251篇
  2015年   724篇
  2014年   1196篇
  2013年   2208篇
  2012年   1314篇
  2011年   1750篇
  2010年   1570篇
  2009年   2189篇
  2008年   1899篇
  2007年   1921篇
  2006年   1809篇
  2005年   1374篇
  2004年   1385篇
  2003年   1280篇
  2002年   1315篇
  2001年   1138篇
  2000年   1088篇
  1999年   946篇
  1998年   939篇
  1997年   932篇
  1996年   763篇
  1995年   721篇
  1994年   681篇
  1993年   594篇
  1992年   519篇
  1991年   536篇
  1990年   513篇
  1989年   522篇
  1988年   474篇
  1987年   545篇
  1986年   502篇
  1985年   573篇
  1984年   717篇
  1983年   617篇
  1982年   589篇
  1981年   551篇
  1980年   477篇
  1979年   473篇
  1978年   491篇
  1977年   429篇
  1976年   367篇
  1975年   381篇
  1974年   346篇
  1973年   403篇
  1972年   301篇
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
101.
102.
103.
104.
Karst database development in Minnesota: design and data assembly   总被引:1,自引:0,他引:1  
The Karst Feature Database (KFD) of Minnesota is a relational GIS-based Database Management System (DBMS). Previous karst feature datasets used inconsistent attributes to describe karst features in different areas of Minnesota. Existing metadata were modified and standardized to represent a comprehensive metadata for all the karst features in Minnesota. Microsoft Access 2000 and ArcView 3.2 were used to develop this working database. Existing county and sub-county karst feature datasets have been assembled into the KFD, which is capable of visualizing and analyzing the entire data set. By November 17 2002, 11,682 karst features were stored in the KFD of Minnesota. Data tables are stored in a Microsoft Access 2000 DBMS and linked to corresponding ArcView applications. The current KFD of Minnesota has been moved from a Windows NT server to a Windows 2000 Citrix server accessible to researchers and planners through networked interfaces.  相似文献   
105.
106.
107.
108.
Authigenic iron and titanium oxides occur in three main textural varieties in the St. Bees Sandstone, a Triassic red bed succession in Cumbria. These are: (a) overgrowths of haematite, titaniferous haematite, anatase, and rutile which generally occur on detrital host grains of similar compositions. The overgrowths may occur as syntaxial rim cements or rhombohedral and prismatic projections and are always in optical continuity, (b) discrete crystals of anatase (including octahedrite) and haematite 10-40 μm in size occur in pore spaces, and (c) fine grained ( < 1 μm) pigmentary haematite occurs as grain coatings around detrital grains and in the interstitial matrix. The euhedral nature and pore-filling habit clearly indicate the authigenic origin of these iron- and titanium oxides. All three textural varieties are believed to have been precipitated from ground waters containing dissolved ferrous and titanium ions. These ions were derived from the intrastratal solution of detrital iron and titanium bearing grains including ferromagnesian silicates and iron-titanium oxides. The precipitation of iron oxides from migrating ground waters in the manner described here goes some way to explaining how thick, uniformly red successions can be formed.  相似文献   
109.
In the present paper revised distances of optical objects from radio sources of the 5C2 survey are given. A statistical investigation of the data is given for blue objects and galaxies by the statistical method of the “first neighbour”. The identification rate on blue plates for both the blue objects and galaxies amounts to about 40% out of the total number of 26 identifications. For every blue object and galaxy which are proposed as an identification the statistical reliability is given.  相似文献   
110.
Plates of the Tautenburg Schmidt can be calibrated with the aid of a beam-splitting prisma only if Schraffierkassette plates are used. The effects of image structure, scintillation and intermittence on in-focus images are different for the main component and the prismatic companion. Therefore, such plates cannot be used to set up a photometric scale.  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