全文获取类型
收费全文 | 2248篇 |
免费 | 468篇 |
国内免费 | 755篇 |
专业分类
测绘学 | 25篇 |
大气科学 | 192篇 |
地球物理 | 222篇 |
地质学 | 2104篇 |
海洋学 | 274篇 |
天文学 | 1篇 |
综合类 | 147篇 |
自然地理 | 506篇 |
出版年
2024年 | 18篇 |
2023年 | 42篇 |
2022年 | 94篇 |
2021年 | 85篇 |
2020年 | 85篇 |
2019年 | 117篇 |
2018年 | 96篇 |
2017年 | 109篇 |
2016年 | 126篇 |
2015年 | 111篇 |
2014年 | 153篇 |
2013年 | 131篇 |
2012年 | 209篇 |
2011年 | 175篇 |
2010年 | 157篇 |
2009年 | 143篇 |
2008年 | 150篇 |
2007年 | 175篇 |
2006年 | 184篇 |
2005年 | 158篇 |
2004年 | 126篇 |
2003年 | 102篇 |
2002年 | 100篇 |
2001年 | 70篇 |
2000年 | 82篇 |
1999年 | 96篇 |
1998年 | 64篇 |
1997年 | 65篇 |
1996年 | 48篇 |
1995年 | 41篇 |
1994年 | 42篇 |
1993年 | 41篇 |
1992年 | 20篇 |
1991年 | 12篇 |
1990年 | 7篇 |
1989年 | 11篇 |
1988年 | 7篇 |
1987年 | 5篇 |
1986年 | 4篇 |
1985年 | 5篇 |
1984年 | 2篇 |
1979年 | 2篇 |
1977年 | 1篇 |
排序方式: 共有3471条查询结果,搜索用时 31 毫秒
91.
对吉林南部地区煤矿主采煤层中的As、B、Ba、Cd、Cu、Hg、Pb、Se、Sr等微量元素的分析结果表明,太原组与山西组由于成煤环境不同,微量元素组成及含量存在一定的差异:太原组原煤中As、B、Hg、Pb、Se、Zn的含量明显高于山西组,山西组原煤中Ba、Cr、Cu、Mn、V的含量明显高于太原组。吉南煤区原煤中As、B、Hg、Pb、Se明显高于地壳元素平均值,呈富集状态,Co、Cd与地壳平均值接近,其他元素均亏损。与全国煤中微量元素相比,该区原煤中As、Ba、Co、Cr、Cu、Hg、Ni、Pb、Se、V、Zn的含量高于全国平均值,B、Mn、Sr含量低于全国平均值。微量元素赋存状态及相关分析表明,Fe与亲硫有害元素As、Cu、Hg、Pb、Se具有显著相关关系,说明煤中黄铁矿及其他硫化物是许多有害微量元素的重要载体。 相似文献
92.
根据岩石地层学、地貌学、孢粉学特征,将河南平顶山地区的第四系划分为4个岩石地层单位,由老到新分别为鲁山组、下汤组、社旗组和马塘组。鲁山组分布于前隆起岗地,为冲洪积成因,形成于225×104aB.P.。下汤组具二元结构,组成河流Ⅳ级阶地,属河流冲积成因,形成于64×104aB.P.。社旗组具二元结构特征,组成河流Ⅲ级阶地,属河流冲积成因,形成年代大于5.42×104aB.P.。马塘组也具二元结构特征,组成河流Ⅱ级阶地,属河流冲积成因,形成于2×104aB.P.。岩石地层单位的划分为探讨黄河—淮河冲积平原及南阳盆地的形成与演化提供了基础性资料。 相似文献
93.
94.
95.
Charnockitic magmatism in southern India 总被引:2,自引:0,他引:2
Large charnockite massifs cover a substantial portion of the southern Indian granulite terrain. The older (late Archaean to
early Proterozoic) charnockites occur in the northern part and the younger (late Proterozoic) charnockites occur in the southern
part of this high-grade terrain. Among these, the older Biligirirangan hill, Shevroy hill and Nilgiri hill massifs are intermediate
charnockites, with Pallavaram massif consisting dominantly of felsic charnockites. The charnockite massifs from northern Kerala
and Cardamom hill show spatial association of intermediate and felsic charnockites, with the youngest Nagercoil massif consisting
of felsic charnockites. Their igneous parentage is evident from a combination of features including field relations, mineralogy,
petrography, thermobarometry, as well as distinct chemical features. The southern Indian charnockite massifs show similarity
with high-Ba-Sr granitoids, with the tonalitic intermediate charnockites showing similarity with high-Ba-Sr granitoids with
low K2O/Na2O ratios, and the felsic charnockites showing similarity with high-Ba-Sr granitoids with high K2O/Na2O ratios. A two-stage model is suggested for the formation of these charnockites. During the first stage there was a period
of basalt underplating, with the ponding of alkaline mafic magmas. Partial melting of this mafic lower crust formed the charnockitic
magmas. Here emplacement of basalt with low water content would lead to dehydration melting of the lower crust forming intermediate
charnockites. Conversely, emplacement of hydrous basalt would result in melting at higher {ie565-01} favoring production of
more siliceous felsic charnockites. This model is correlated with two crustal thickening phases in southern India, one related
to the accretion of the older crustal blocks on to the Archaean craton to the north and the other probably related to the
collision between crustal fragments of East and West Gondwana in a supercontinent framework. 相似文献
96.
97.
Curie-point depth from spectral analysis of magnetic data in central-southern Europe 总被引:3,自引:0,他引:3
The basal depth of the outer layer with internal magnetic sources was calculated from magnetic data available within a roughly 500 km wide and 1200 km long area, running from central Germany to southern Italy. The dataset, deriving from different aeromagnetic surveys, is reduced to the reference altitude of 3000 m a.s.l. and a reference year of 1980.0. The adopted method, which transforms the spatial data into the frequency domain, provides a relationship between the two-dimensional spectrum of the magnetic anomalies and the top and centroid depths of the magnetic sources. The magnetic layer bottom depth (MLBD) thus obtained is 29-33 km deep in the stable areas (central Europe Variscan units, Corsica-Sardinia Variscan block) and corresponds to the Moho, having an average temperature of 560 °C. From the Alps to the Apennines, MLBD ranges between 22 and 28 km and is clearly shallower than the Moho. In these units, the wide variation of MLBD appears to be compatible with the presence of shallow magnetised bodies, consisting of lower crustal rocks (Ivrea-Verbano zone), ophiolitic units (Penninic zone and Voltri Massif) and intrasedimentary basic volcanic bodies (Po Basin). An average value of 25 km can be attributed to MLBD, which corresponds to a temperature of 550 °C. In the peri-Tyrrhenian zone and the Ligurian Sea, MLBD is below the Moho, which ranges from 17 to 20 km depth, and it has a temperature matching approximately to the Curie temperature of magnetite (580 °C). 相似文献
98.
Tiziana Tuvè Antonio Teramo Jesus Ibañez Carla Bottari Domenica Termini 《Pure and Applied Geophysics》2005,162(4):747-760
A modelling of the observed macroseismic intensity of historical and instrumental earthquakes in southern Spain is proposed, with the aim of determining the macroseismic parameters for seismic hazard evaluation in a region in which the characterization of intensity distribution of seismic events shows different levels of difficulty referable to the complex faults system of the area in study. The adopted procedure allows an analytical determination of epicenters and principal attenuation directions of earthquakes with a double level of verification with reference to the maximum shaking area and structural lineaments of the region, respectively. The analyses, carried out on a suitable number of events, highlight, therefore, some elements for a preliminary characterization of a seismic zonation on the basis of the consistency between seismic intensity distribution of earthquakes and corresponding structural framework. 相似文献
99.
研究区虎睛石矿床在地质特征、矿物组合、化学成分及琢雕效果等方面与国外虎睛石矿床是完全不同的,属于一种特殊的罕见类型。在分析虎睛石地质特征、开发利用现状的基础上,认为该区的虎睛石资源丰富,琢雕效果好,在国内外市场上具有一定的竞争力和良好的开发利用前景。 相似文献
100.
WANG Min 《中国地球化学学报》2005,24(4):297-305
Systematic microthermometric measurements of fluid inclusions in the PGE-polymetallic deposits hosted in the Lower Cambrian black rock series in southern China were performed, and the results suggest: (1) there exist two types of fluid inclusions. TypeⅠis of NaCl-H2O system with low-medium salinity, and its homogenization temperatures (Th) and salinities are 106.9- 286.4℃ and ( 0.8- 21.8) wt%NaCl eq. respectively; TypeⅡ is of CaCl2-NaCl-H2O system with medium-high salinities, and its homogenization temperatures and salinities range from 120.1℃ to 269.6℃ and ( 11.4- 31.4) wt%NaCl eq., respectively. The typeⅡ fluid inclusions have been discovered for the first time in this kind of deposits; (2) two generations of ore-forming fluids were recognized. Characteristics of fluid inclusions in the PGE-polymetallic ores and carbonate-quartz stockworks in the underlying phosphorites are almost of no difference, they may represent ore-forming fluids at the main metallogenic stage. The peak value of homogenization temperature of those fluid inclusions is about 170℃, while their salinities possess a remarkable bimodal distribution pattern with two peak values of (27-31) wt%NaCl eq. and (4-6) wt%NaCl eq. On the contrary, fluid inclusions in the carbonate-quartz veins in the hanging wall may represent ore-forming fluids at the post-metallogenetic stage. The homogenization temperatures and the peak values of salinities are mostly 130-170℃ and (12-14) wt%NaCl eq., respectively; (3) nobel gas isotopic composition analyses in combination with the microthermometric measurements of fluid inclusions suggest that the ore-forming fluids at the main metallogenetic stage were probably derived from mixing of basinal hot brines with the CaCl2-NaCl-H2O system and seawater with the NaCl-H2O system; (4) in the Early Cambrian, the basinal hot brines were trapped in the Caledonian basins, which were distributed along the southern margin of the Yangtze Craton, and where giant thick sediments were accumulated, and expelled and migrated laterally along the strata because of the pressure caused by overlying sediments. The basinal hot brines absorbed Ni, Mo, V, PGE from the surrounding rocks and were transformed into ore-bearing hydrothermal fluids with the CaCl2-NaCl-H2O system and medium-high salinities, then ascended along faults and mixed with seawater of the NaCl-H2O system, and finally PGE-polymetallic deposits or occurrences were formed in the black rock series. 相似文献