全文获取类型
收费全文 | 8178篇 |
免费 | 1418篇 |
国内免费 | 2170篇 |
专业分类
测绘学 | 843篇 |
大气科学 | 1684篇 |
地球物理 | 1662篇 |
地质学 | 3892篇 |
海洋学 | 1510篇 |
天文学 | 400篇 |
综合类 | 746篇 |
自然地理 | 1029篇 |
出版年
2024年 | 68篇 |
2023年 | 169篇 |
2022年 | 403篇 |
2021年 | 441篇 |
2020年 | 432篇 |
2019年 | 422篇 |
2018年 | 450篇 |
2017年 | 393篇 |
2016年 | 474篇 |
2015年 | 449篇 |
2014年 | 498篇 |
2013年 | 557篇 |
2012年 | 550篇 |
2011年 | 569篇 |
2010年 | 496篇 |
2009年 | 483篇 |
2008年 | 436篇 |
2007年 | 421篇 |
2006年 | 362篇 |
2005年 | 342篇 |
2004年 | 270篇 |
2003年 | 207篇 |
2002年 | 225篇 |
2001年 | 240篇 |
2000年 | 237篇 |
1999年 | 272篇 |
1998年 | 231篇 |
1997年 | 219篇 |
1996年 | 210篇 |
1995年 | 184篇 |
1994年 | 176篇 |
1993年 | 150篇 |
1992年 | 139篇 |
1991年 | 121篇 |
1990年 | 84篇 |
1989年 | 80篇 |
1988年 | 63篇 |
1987年 | 50篇 |
1986年 | 30篇 |
1985年 | 26篇 |
1984年 | 23篇 |
1983年 | 18篇 |
1982年 | 28篇 |
1981年 | 14篇 |
1980年 | 7篇 |
1979年 | 9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 0 毫秒
991.
氧化铬柱支撑蒙脱石的制备研究 总被引:4,自引:1,他引:3
以浙江和新疆的膨润土为原料合成了氧化铝柱支撑蒙脱石,成柱溶液以Na2CO3为碱水解铝盐溶液制得。因为制备含有大聚羟基铬阳离子的成柱溶液是获得具有大的基面间距的柱支撑粘土的关键,我们详细研究了CO32-/Cr3+值、水解温度和水解时间对所得柱支撑蒙脱石性质的影响。聚羟基铬阳离子通过阳离子交换引入蒙脱石,所得产物用X射线衍射分析和BET氮比表面等方法研究。所得氧化铝柱支撑蒙脱石(简称Cr-mont)的基面间距为2.55nm,BET氮比表面积为190~230m2/g。 相似文献
992.
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
993.
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
994.
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
995.
Models of corundum origin from alkali basaltic terrains: a reappraisal 总被引:10,自引:0,他引:10
F. Lin Sutherland Paul W. O. Hoskin C. Mark Fanning Robert R. Coenraads 《Contributions to Mineralogy and Petrology》1998,133(4):356-372
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
996.
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
997.
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
998.
999.
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
1000.
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