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   7943篇
  免费   1356篇
  国内免费   2064篇
测绘学   841篇
大气科学   1638篇
地球物理   1621篇
地质学   3672篇
海洋学   1438篇
天文学   399篇
综合类   738篇
自然地理   1016篇
  2024年   50篇
  2023年   109篇
  2022年   364篇
  2021年   407篇
  2020年   394篇
  2019年   404篇
  2018年   424篇
  2017年   375篇
  2016年   439篇
  2015年   427篇
  2014年   474篇
  2013年   538篇
  2012年   544篇
  2011年   566篇
  2010年   479篇
  2009年   478篇
  2008年   437篇
  2007年   419篇
  2006年   366篇
  2005年   342篇
  2004年   269篇
  2003年   205篇
  2002年   218篇
  2001年   240篇
  2000年   236篇
  1999年   273篇
  1998年   228篇
  1997年   220篇
  1996年   210篇
  1995年   182篇
  1994年   175篇
  1993年   148篇
  1992年   138篇
  1991年   121篇
  1990年   84篇
  1989年   78篇
  1988年   63篇
  1987年   50篇
  1986年   30篇
  1985年   24篇
  1984年   23篇
  1983年   16篇
  1982年   28篇
  1981年   14篇
  1980年   7篇
  1979年   8篇
  1977年   5篇
  1976年   8篇
  1973年   4篇
  1958年   3篇
排序方式: 共有10000条查询结果,搜索用时 109 毫秒
731.
前陆盆地类型及其沉积动力学研究综述   总被引:17,自引:2,他引:15  
从前陆盆地的特点及类型入手,综述了前陆盆地研究的热点内容,最新方法及其沉积动力学进展状况,揭示了前陆背景下盆地充填序列的构成及内部演化特征,指出了盆地的沉积-地层格架与冲断造山带的幕式活动之间的响应关系。  相似文献   
732.
陈健云  林皋 《岩土力学》1998,19(3):14-19
研究了文献[2]提出的结线动力无穷元的特性及其参数确定。由于这种单元将衰减函数定义在无穷向结线上,从而不仅可同时考虑多种波动形式,而且对于不同介质,不必通过改变节点坐标分布的形式实现介质间的过渡,而直接以结线上参数的改变来实现,因而可以更好地模拟无穷波动场,使用起来更方便.更容易推广。  相似文献   
733.
In three polished thin sections of Yamato 791717 (CO3). fifty-five Ca, Al-rich inclusions were found, which include two hibonite-bearing, eight melilite-rich and forty-five spinel-pyroxene inclusions. Based on the petrography and mineral chemistry of the inclusions, it is proposed that the melilite-rich inclusions and spinel-pyroxene inclusions condensed in the solar nebula, and the hibonite-bearing inclusions crystallized from melts. The heavy alteration of the inclusions in Yamato 791717, which probably took place under a very oxidizing condition in the solar nebular, is also confirmed. Project supported by the National Natural Science Foundation of China (Grant No. 49673200). and by the Japanese Society for Promotion of Sciences (JSPS).  相似文献   
734.
Models of corundum origin from alkali basaltic terrains: a reappraisal   总被引:10,自引:0,他引:10  
Corundums from basalt fields, particularly in Australia and Asia, include a dominant blue-green-yellow zoned “magmatic” suite (BGY suite) and subsidiary vari-coloured “metamorphic” suites. The BGY corundums have distinctive trace element contents (up to 0.04 wt% Ga2O3 and low Cr/Ga and Ti/Ga ratios <1). Different melt origins for BGY corundums are considered here from their inclusion and intergrowth mineralogy, petrologic associations and tectonic setting. Analysed primary inclusion minerals (over 100 inclusions) cover typical feldspars, zircon and Nb-Ta oxides and also include hercynite-magnetite, gahnospinel, rutile-ilmenite solid solution, calcic plagioclase, Ni-rich pyrrhotite, thorite and low-Si and Fe-rich glassy inclusions. This widens a previous inclusion survey; New England, East Australia corundums contain the most diverse inclusion suite known from basalt fields (20 phases). Zircon inclusion, intergrowth and megacryst rare earth element data show similar patterns, except for Eu which shows variable depletion. Temperature estimates from magnetite exsolution, feldspar compositions and fluid inclusion homogenization suggest that some corundums crystallized between 685–900 °C. Overlap of inclusion Nb, Ta oxide compositions with new comparative data from niobium-yttrium-fluorine enriched granitic pegmatites favour a silicate melt origin for the corundums. The feasibility of crystallizing corundum from low-volume initial melting of amphibole-bearing mantle assemblages was tested using the MELTS program on amphibole-pyroxenite xenolith chemistry from basalts. Corundum appears in the calculations at 720–880 °C and 0.7–1.1 GPa with residual feldspathic assemblages that match mineral compositions found in corundums and their related xenoliths. A model that generates melts from amphibole-bearing lithospheric mantle during magmatic plume activity is proposed for BGY corundum formation. Received: 3 January 1997 / Accepted: 8 July 1998  相似文献   
735.
Based on the method of "two-dimensional depth structure of the crust" proposed by Horiuchi et al., about 5000 arrival times of 303 local shallow earthquakes recorded by the Beijing Seismographic Network from 1990 ~ 1993 are used to investigate the depth distribution of Moho discontinuity beneath Beijing and its adjacent area. We simultaneously determined the hypocenter parameters and P- and S-wave station corrections. The data of the North China Network were also investigated. The results are as follows: (1) The depth distribution of Moho discontinuity becomes shallower from the northwest to the southeast, i.e., in Zhangjiakou area, the Moho discontinuity is located at a depth range from 40~42 km. In the Beijing area, it is 36~39 km. However, at the eastern and southeastern part of this area, it is only 28-30 km and 30~32 km, respectively. (2) Beneath the Tangshan area, there is another elliptic interface shallower than the Moho discontinuity. Separately, its major and minor axis is approximately along  相似文献   
736.
北淮阳盆岭带的构造演化与铀成矿   总被引:1,自引:0,他引:1       下载免费PDF全文
北淮阳盆岭构造带是大别造山带的重要组成部分。佛子岭岩群代表了早古生代扬子地块北缘大别古岛弧弧前海盆的火山沉积建造,在加里东运动陆块对接过程中变形变质。石炭系梅山群具磨拉石建造特征。在华力西印支期陆内俯冲褶皱带的基础上,燕山期沿桐柏桐城断裂伸展北移,近东西向断陷盆地发育,形成盆岭构造景观。南侧大别山强烈隆升,铸就了现今大别山变质核杂岩构造格局。中生代岩浆活动是区内重要铀源,具有成矿潜力的地质体是响洪甸正长岩体和北带粗面质火山碎屑岩  相似文献   
737.
本文利用“八·五”短临预报的地震学攻关成果来分析福建地区的几个震例,检验其在福建地区的适用情况。  相似文献   
738.
分布于藏南江孜一带的上白垩统宗卓组沉积混杂堆积岩呈近东西向与雅鲁藏布江缝合带平行相伴,由“基质”、原地岩块、外来岩块三部分组成。“基质”以正常沉积的细碎屑岩为主;原地岩块是沉积物未完全固结时,由于重力或其它地质作用使之变形变位后形成的;外来岩块成分复杂、形态各异、大小悬殊,不同岩块中产晚三叠世—早白垩世的箭石、双壳类等化石。岩块间很少直接接触,地貌上明显突起,其变形变质程度与“基质”极不协调,它是早白垩世以来,喜马拉雅板片向冈底斯-念青唐古拉板片俯冲,于被动陆缘形成近东西向的狭长海槽,而仰冲板片受到强烈的破碎,大小不等的岩块滑落于海槽中构成的沉积混杂堆积岩。  相似文献   
739.
通过对比中国长白山区和朝鲜白头山区新生代火山岩系的层序和同位素年代学资料,首次编制出中朝边境地区新生代火山岩系分布图和新生代火山喷发阶段对比表。其岩石化学和地球化学演化趋势表明,该区新生代火山完全有可能再次喷发。  相似文献   
740.
Based on the statistics of the peaks in the random Gaussian field, we put forward a method to model the evolution of quasars, which are assumed to be a phenomenon of the early stages for some massive galaxies. Our calculations show that the cold-hot mixed dark matter model with h = 0.3 cannot match the observed quasar abundance at redshift z = 4.5, and other prevailing CDM models, such as the mixed dark matter model with h = 0.2, the tilted CDM models with n = 0.7 or 0.8, and the flat CDM models with = 0.6 or 0.7, are compatible with the observation of the abundance of QSOs on the range of z = 2-5.  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