全文获取类型
收费全文 | 1481篇 |
免费 | 263篇 |
国内免费 | 378篇 |
专业分类
测绘学 | 69篇 |
大气科学 | 220篇 |
地球物理 | 346篇 |
地质学 | 928篇 |
海洋学 | 170篇 |
天文学 | 63篇 |
综合类 | 178篇 |
自然地理 | 148篇 |
出版年
2024年 | 8篇 |
2023年 | 29篇 |
2022年 | 60篇 |
2021年 | 66篇 |
2020年 | 51篇 |
2019年 | 82篇 |
2018年 | 79篇 |
2017年 | 68篇 |
2016年 | 77篇 |
2015年 | 64篇 |
2014年 | 74篇 |
2013年 | 72篇 |
2012年 | 71篇 |
2011年 | 97篇 |
2010年 | 81篇 |
2009年 | 89篇 |
2008年 | 72篇 |
2007年 | 69篇 |
2006年 | 67篇 |
2005年 | 52篇 |
2004年 | 46篇 |
2003年 | 43篇 |
2002年 | 41篇 |
2001年 | 48篇 |
2000年 | 61篇 |
1999年 | 87篇 |
1998年 | 67篇 |
1997年 | 69篇 |
1996年 | 55篇 |
1995年 | 58篇 |
1994年 | 50篇 |
1993年 | 47篇 |
1992年 | 19篇 |
1991年 | 22篇 |
1990年 | 22篇 |
1989年 | 11篇 |
1988年 | 16篇 |
1987年 | 6篇 |
1986年 | 4篇 |
1985年 | 5篇 |
1984年 | 3篇 |
1983年 | 3篇 |
1982年 | 3篇 |
1981年 | 3篇 |
1979年 | 1篇 |
1978年 | 1篇 |
1977年 | 1篇 |
1965年 | 1篇 |
1958年 | 1篇 |
排序方式: 共有2122条查询结果,搜索用时 250 毫秒
141.
侏罗系是四棵树凹陷油气勘探的重要目的层,进一步查明侏罗系油气来源,落实生烃中心,对今后勘探选区选带十分重要。本文在对侏罗系烃源岩有机质丰度、类型、成熟度以及埋藏史和生烃潜力分析的基础上,开展了原油分类、油源对比及油气运移分析研究。结果表明,下侏罗统八道湾组主要发育湖相泥岩和河沼—三角洲相煤系两类烃源岩,有机质类型较好,丰度较高,主体处于低成熟—成熟阶段,局部演化程度高,生气潜力大;八道湾组具晚期快速埋藏生烃特点,四棵树凹陷主体以生油为主;生物标志化合物特征及其指纹对比发现,中侏罗统头屯河组含A、B两类原油,A类原油主要源自八道湾组中段湖相泥岩,生油母质以低等水生生物为主,B类原油的生油母质主要为高等植物,应主要来自八道湾组上、下段煤系地层;据三环萜烷/五环三萜烷和重排甾烷/规则甾烷反映出的运移效应推断,卡因迪克构造带以南至西湖构造之间存在八道湾组烃源岩的生油中心,是卡6井区和西湖1井头屯河组原油的主要供烃区,该区域是今后侏罗系勘探的有利区带。 相似文献
142.
143.
The advantages of using unmanned underwater vehicles in coastal ocean studies are emphasized. Two types of representative vehicles, remotely operated vehicle (ROV) and autonomous underwater vehicle (AUV) from University of South Florida, are discussed. Two individual modular sensor packages designed and tested for these platforms and field measurement results are also presented. The bottom classification and albedo package, BCAP, provides fast and accurate estimates of bottom albedos, along with other parameters such as in-water remote sensing reflectance. The real-time ocean bottom optical topographer, ROBOT, reveals high-resolution 3-dimentional bottom topography for target identification. Field data and results from recent Coastal Benthic Optical Properties field campaign, 1999 and 2000, are presented. Advantages and limitations of these vehicles and applications of modular sensor packages are compared and discussed. 相似文献
144.
Rui-Xiang Chang Cheng-Gang Shu Jin-Liang Hou Shanghai Astronomical Observatory Chinese Academy of Sciences Shanghai CAS-Peking University Joint Beijing Astronomical Center Beijing 《中国天文和天体物理学报》2002,2(3)
Based on a physical treatment of the star formation law similar to that given by Efstathiou, we have improved our two-component chemical evolution model for the Milky Way disk. Two gas infall rates are compared, one exponential, one Gaussian. It is shown that the star formation law adopted in this paper depends more strongly on the gas surface density than that in Chang et al. It has large effects on the history of star formation and gas evolution of the whole disk. In the solar neighborhood, the history of chemical evolution and star formation is not sensitive to whether the infall rate is Gaussian or exponential. For the same infall time scale, both forms predict the same behavior for the current properties of the Galactic disk. The model predictions do depend on whether or not the infall time scale varies with the radius, but current available observations cannot decide which case is the more realistic. Our results also show that it would be inadequate to describe the gradient evolution along the Gala 相似文献
145.
146.
147.
148.
Linking the Sulu UHP belt to the Korean Peninsula: Evidence from eclogite, Precambrian basement, and Paleozoic sedimentary basins 总被引:13,自引:0,他引:13
Mingguo Zhai Jinghui Guo Zhong Li Daizhao Chen Peng Peng Tiesheng Li Quanlin Hou Qicheng Fan 《Gondwana Research》2007,12(4):388-403
Considerable debate on whether and how the Sulu Orogenic Belt extends eastward to the Korean Peninsula has remained over the past decade. New results reported here include the following: (1) an eclogite and retrograded eclogite-bearing complex (Hongseong Complex) is discovered in South Korea, in which the eclogite occurs as lenses in circa 810–820 Ma granitic gneiss. SHRIMP zircon dating of the eclogite yields 230 Ma for the metamorphic age and 880 Ma for the protolith age; (2) The basement of the Rangnim, Gyeonggi and Yeongnam massifs have affinities to the basement of the North China Block (NCB). However the Gyeonggi Massif encloses a minor amount of large or small slabs of the Hongseong Complex that are similar to the rocks of the Sulu Belt. (3) Two main Paleozoic basins within the Rangnim and Gyeonggi massifs have a similar Paleozoic tectono-stratigraphy to the NCB. (4) The Imjingang and Ogcheon belts do not exhibit any metamorphic characteristics of collisional orogenic belts. Based on these facts, we propose a crustal-detachment and thrust model and suggest that the collision belt between the Yangtze Block (YB) and NCB (Sino–Korea Craton) is preserved along the western margin of the Korean Peninsula. The lower part of the UHP metamorphosed lithosphere of the YB was subducted under the Korean Peninsula and not uplifted to the surface. The lower crust of the YB (the Hongseong Complex) was detached from the subducted lithosphere and thrust over the Korean Peninsula, and inserted into the basement rocks of the Gyeonggi Massif. The upper crust of the YB possibly was detached from the lower crust and overthrusted along the Honam and Chugaryong shear zones. The Imjingang and Ogcheon belts possibly represent the detached upper crust of YB and their present occurrences are controlled by a Mesozoic strike–slip shear structure. All these detached lower and upper crustal slabs were strongly deformed during the Late Jurassic and Early Cretaceous tectonic event leading to their present geological distribution and characteristics. 相似文献
149.
150.
The Qolqoleh gold deposit is located in the northwestern part of the Sanandai‐Sirjan Zone, northwest of Iran. Gold mineralization in the Qolqoleh deposit is almost entirely confined to a series of steeply dipping ductile–brittle shear zones generated during Late Cretaceous–Tertiary continental collision between the Afro‐Arabian and the Iranian microcontinent. The host rocks are Mesozoic volcano‐sedimentary sequences consisting of felsic to mafic metavolcanics, which are metamorphosed to greenschist facies, sericite and chlorite schists. The gold orebodies were found within strong ductile deformation to late brittle deformation. Ore‐controlling structure is NE–SW‐trending oblique thrust with vergence toward south ductile–brittle shear zone. The highly strained host rocks show a combination of mylonitic and cataclastic microstructures, including crystal–plastic deformation and grain size reduction by recrystalization of quartz and mica. The gold orebodies are composed of Au‐bearing highly deformed and altered mylonitic host rocks and cross‐cutting Au‐ and sulfide‐bearing quartz veins. Approximately half of the mineralization is in the form of dissemination in the mylonite and the remainder was clearly emplaced as a result of brittle deformation in quartz–sulfide microfractures, microveins and veins. Only low volumes of gold concentration was introduced during ductile deformation, whereas, during the evident brittle deformation phase, competence contrasts allowed fracturing to focus on the quartz–sericite domain boundaries of the mylonitic foliation, thus permitting the introduction of auriferous fluid to create disseminated and cross‐cutting Au‐quartz veins. According to mineral assemblages and alteration intensity, hydrothermal alteration could be divided into three zones: silicification and sulfidation zone (major ore body); sericite and carbonate alteration zone; and sericite–chlorite alteration zone that may be taken to imply wall‐rock interaction with near neutral fluids (pH 5–6). Silicified and sulfide alteration zone is observed in the inner parts of alteration zones. High gold grades belong to silicified highly deformed mylonitic and ultramylonitic domains and silicified sulfide‐bearing microveins. Based on paragenetic relationships, three main stages of mineralization are recognized in the Qolqoleh gold deposit. Stage I encompasses deposition of large volumes of milky quartz and pyrite. Stage II includes gray and buck quartz, pyrite and minor calcite, sphalerite, subordinate chalcopyrite and gold ores. Stage III consists of comb quartz and calcite, magnetite, sphalerite, chalcopyrite, arsenopyrite, pyrrhotite and gold ores. Studies on regional geology, ore geology and ore‐forming stages have proved that the Qolqoleh deposit was formed in the compression–extension stage during the Late Cretaceous–Tertiary continental collision in a ductile–brittle shear zone, and is characterized by orogenic gold deposits. 相似文献