全文获取类型
收费全文 | 2302篇 |
免费 | 627篇 |
国内免费 | 486篇 |
专业分类
测绘学 | 40篇 |
大气科学 | 45篇 |
地球物理 | 172篇 |
地质学 | 2681篇 |
海洋学 | 197篇 |
天文学 | 1篇 |
综合类 | 110篇 |
自然地理 | 169篇 |
出版年
2024年 | 7篇 |
2023年 | 26篇 |
2022年 | 49篇 |
2021年 | 73篇 |
2020年 | 73篇 |
2019年 | 90篇 |
2018年 | 83篇 |
2017年 | 94篇 |
2016年 | 123篇 |
2015年 | 107篇 |
2014年 | 177篇 |
2013年 | 146篇 |
2012年 | 157篇 |
2011年 | 195篇 |
2010年 | 163篇 |
2009年 | 167篇 |
2008年 | 151篇 |
2007年 | 142篇 |
2006年 | 138篇 |
2005年 | 128篇 |
2004年 | 95篇 |
2003年 | 94篇 |
2002年 | 101篇 |
2001年 | 85篇 |
2000年 | 105篇 |
1999年 | 102篇 |
1998年 | 71篇 |
1997年 | 66篇 |
1996年 | 65篇 |
1995年 | 44篇 |
1994年 | 57篇 |
1993年 | 58篇 |
1992年 | 46篇 |
1991年 | 32篇 |
1990年 | 24篇 |
1989年 | 16篇 |
1988年 | 17篇 |
1987年 | 14篇 |
1986年 | 12篇 |
1985年 | 5篇 |
1984年 | 9篇 |
1983年 | 5篇 |
1976年 | 1篇 |
1973年 | 1篇 |
1954年 | 1篇 |
排序方式: 共有3415条查询结果,搜索用时 46 毫秒
101.
102.
为了加深对黄金带复杂断块油田进一步开发,针对该区断层复杂、储层变化大、油水关系复杂等特征,笔者综合运用岩心、分析化验及录井、测井资料,对其沉积特征、储层岩性、物性和非均质性进行详细研究。以JASON软件为平台,对含油砂体进行了追踪和预测,并在有利区提出井位部署,为该区的进一步开发提供了地质依据。 相似文献
103.
104.
闽西-赣南早-中侏罗世盆地及其火成岩特征 总被引:22,自引:3,他引:22
闽西-赣南地区早、中侏罗世陆相盆地带东起福建永定,经江西寻乌到龙南,断续延伸约250km,宽60~80km.受后期构造破坏和花岗岩浆侵入影响,现呈肢解散碎的残留盆地面貌.盆地边界特征和盆区岩层节理测量统计结果反映该区自晚三叠世以来,先后经历了近S-N向水平挤压(T3-J1E),S-N向垂向挤压、近E-W向水平伸展(J1L-J2),SE-NW向挤压(K1)和近E-W向挤压、S-N向伸展(K2)等复杂的演化过程.早-中侏罗世强烈的拉张-断陷作用导致盆区大量双峰式火山岩的喷发,其基性端员玄武岩的颗粒锆石U-Pb年龄值为170±1Ma,酸性端员流纹岩Rb-Sr等时线年龄为179Ma~165±2Ma.流纹岩具有高的SiO2、Al2O3、K2O含量,ANKC值>1.1;轻稀土富集、稀土总量高,铕亏损,具明显Eu负异常;富集Rb、Th,贫化Ba、Ti、P、Nb、Zr等特点,属富钾过铝火山岩类.与之共生的玄武岩则以富硅贫碱为特征,轻稀土轻度富集,铕异常不明显;弱富集Rb、Ba、Th、Ce,贫Nb、Zr、Y,配分样式呈上凸型,属拉斑系列玄武岩类,反映一种后造山的陆内裂谷环境.闽西-赣南地区盆山格局的形成经历过多期地球动力学演化前中生代近E-W向古亚洲构造域的基底阶段,晚三叠世-早侏罗世早期挤压造山阶段,早侏罗世晚期-中侏罗世裂谷盆地阶段,早白垩世太平洋构造域对本区的置换和改造阶段,包括早期的火山-岩浆活动和晚期的伸展断陷盆地作用. 相似文献
105.
大井锡多金属成矿地质特征及找矿方向探讨 总被引:2,自引:0,他引:2
内蒙古林西大井锡多金属矿是我国北方最大的锡多金属矿床,通过对其地质背景、成矿地质条件、富集规律、控矿因素的认识和分析,建立大井式的综合找矿标志,对指导矿区及其外围找矿,扩大矿产资源、发展地方经济,具有重要的意义。 相似文献
106.
沉积有机相是近年来国内外广泛运用于油气勘探的一种有效的研究方法。本文介绍了沉积有机相的概念、划分方案,及其在油气勘探、盆地分析和层序地层学中的应用,指出了沉积有机相与层序地层分析相结合对油气资源评价和预测烃源岩有广阔的发展前景。 相似文献
107.
CLIFFORD TOM N.; BARTON ERIKA S.; STERN RICHARD A.; DUCHESNE JEAN-CLAIR 《Journal of Petrology》2004,45(4):669-691
The O'okiep Copper District is underlain by voluminous 10351210Ma granite gneiss and granite with remnants of metamorphosedsupracrustal rocks. This assemblage was intruded by the 1030Ma copper-bearing Koperberg Suite that includes jotunite, anorthosite,biotite diorite and hypersthene-bearing rocks ranging from leuconoriteto hypersthenite. New sensitive high-resolution ion microprobeage data demonstrate the presence of 17002000 Ma zirconas xenocrysts in all of the intrusive rocks, and as detritalzircon in the metasediments of the Khurisberg Subgroup. Thesedata are consistent with published SmNd model ages ofc. 1700 Ma (TCHUR) and c. 2000 Ma (TDM) of many of the intrusivesthat support a major crust-forming event in Eburnian (Hudsonian)times. In addition, UThPb analyses of zirconsfrom all major rock units define two tectono-magmatic episodesof the Namaquan Orogeny: (1) the O'okiepian Episode (11801210Ma), represented by regional granite plutonism, notably theNababeep and Modderfontein Granite Gneisses and the Concordiaand Kweekfontein Granites that accompanied and outlasted (e.g.Kweekfontein Granite) regional tectonism [F2(D2)] and granulite-faciesmetamorphism (M2); (2) the Klondikean Episode (10201040Ma), which includes the intrusion of the porphyritic RietbergGranite and of the Koperberg Suite that are devoid of regionalplanar or linear fabrics. Klondikean tectonism (D3) is reflectedby major eastwest-trending open folds [F3(D3a)], andby localized eastwest-trending near-vertical ductilefolds [steep structures; F4(D3b)] whose formationwas broadly coeval with the intrusion of the Koperberg Suite.A regional, largely thermal, amphibolite- to granulite-faciesmetamorphism (M3) accompanied D3. This study demonstrates, interalia, that the complete spectrum of rock-types of the KoperbergSuite, together with the Rietberg Granite, was intruded in ashort time-interval (<10 Myr) at c. 1030 Ma, and that therewere lengthy periods of about 150 Myr of tectonic quiescencewithin the Namaquan Orogeny: (1) between the O'okiepian andKlondikean Episodes; (2) from the end of the latter to the formalend of Namaquan Orogenesis 800850 Ma ago. KEY WORDS: UPb, zircon; O'okiep, Namaqualand; granite plutonism; granulite facies; Koperberg Suite; Namaquan (Grenville) Orogeny 相似文献
108.
Indicator Simulation Accounting for Multiple-Point Statistics 总被引:7,自引:0,他引:7
Geostatistical simulation aims at reproducing the variability of the real underlying phenomena. When nonlinear features or large-range connectivity is present, the traditional variogram-based simulation approaches do not provide good reproduction of those features. Connectivity of high and low values is often critical for grades in a mineral deposit. Multiple-point statistics can help to characterize these features. The use of multiple-point statistics in geostatistical simulation was proposed more than 10 years ago, on the basis of the use of training images to extract the statistics. This paper proposes the use of multiple-point statistics extracted from actual data. A method is developed to simulate continuous variables. The indicator kriging probabilities used in sequential indicator simulation are modified by probabilities extracted from multiple-point configurations. The correction is done under the assumption of conditional independence. The practical implementation of the method is illustrated with data from a porphyry copper mine. 相似文献
109.
Transformation of garnet epidote amphibolite to eclogite, western Dabie Mountains, China 总被引:8,自引:0,他引:8
Omphacite and garnet coronas around amphibole occur in amphibolites in the Hong'an area, western Dabie Mountains, China. These amphibolites consist of an epidote–amphibolite facies assemblage of amphibole, garnet, albite, clinozoisite, paragonite, ilmenite and quartz, which is incompletely overprinted by an eclogite facies assemblage of garnet, omphacite and rutile. Coronas around amphibole can be divided into three types: an omphacite corona; a garnet–omphacite–rutile corona; and, a garnet–omphacite corona with less rutile. Chemographic analysis for local reaction domains in combination with petrographical observations show that reactions Amp + Ab + Pg = Omp +Czo + Qtz + H2O, and Amp + Ab = Omp ± Czo + Qtz + H2O may lead to the development of omphacite coronas. The garnet–omphacite–rutile corona was formed from the reaction Amp + Ab + Czo + Ilm ± Qtz = Omp + Grt + Rt + H2O. In garnet–omphacite coronas, the garnet corona grew during an early stage of epidote amphibolite facies metamorphism, whereas omphacite probably formed by the reactions forming the omphacite corona during the eclogite facies stage. It is estimated that these reactions occurred at 0.8–1.4 GPa and 480–610 °C using the garnet–clinopyroxene thermometer and omphacite barometer in the presence of albite. 相似文献
110.
Ingrid M. Kjarsgaard M.Beth McClenaghan Bruce A. Kjarsgaard Larry M. Heaman 《Lithos》2004,77(1-4):705-731
Sixteen kimberlite boulders were collected from three sites on the Munro and Misema River Eskers in the Kirkland Lake kimberlite field and one site on the Sharp Lake esker in the Lake Timiskaming kimberlite field. The boulders were processed for heavy-mineral concentrates from which grains of Mg-ilmenite, chromite, garnet, clinopyroxene and olivine were picked, counted and analyzed by electron microprobe. Based on relative abundances and composition of these mineral phases, the boulders could be assigned to six mineralogically different groups, five for the Kirkland Lake area and one for the Lake Timiskaming area. Their indicator mineral composition and abundances are compared to existing data for known kimberlites in both the Kirkland Lake and Lake Timiskaming areas. Six boulders from the Munro Esker form a compositionally homogeneous group (I) in which the Mg-ilmenite population is very similar to that of the A1 kimberlite, located 7–12 km N (up-ice), directly adjacent to the Munro esker in the Kirkland Lake kimberlite field. U–Pb perovskite ages of three of the group I boulders overlap with that of the A1 kimberlite. Three other boulders recovered from the same localities in the Munro Esker also show some broad similarities in Mg-ilmenite composition and age to the A1 kimberlite. However, they are sufficiently different in mineral abundances and composition from each other and from the A1 kimberlite to assign them to different groups (II–IV). Their sources could be different phases of the same kimberlite or—more likely—three different, hitherto unknown kimberlites up-ice of the sample localities along the Munro Esker in the Kirkland Lake kimberlite field. A single boulder from the Misema River esker, Kirkland Lake, has mineral compositions that do not match any of the known kimberlites from the Kirkland Lake field. This suggests another unknown kimberlite exists in the area up-ice of the Larder Lake pit along the Misema River esker. Six boulders from the Sharp Lake esker, within the Lake Timiskaming field, form a homogeneous group with distinct mineral compositions unmatched by any of the known kimberlites in the Lake Timiskaming field. U–Pb perovskite age determinations on two of these boulders support this notion. These boulders are likely derived from an unknown kimberlite source up-ice from the Seed kimberlite, 4 km NW of the Sharp Lake pit, since indicator minerals with identical compositions to those of the Sharp Lake boulders have been found in till samples collected down-ice from Seed. Based on abundance and composition of indicator minerals, most importantly Mg-ilmenite, and supported by U–Pb age dating of perovskite, we conclude that the sources of 10 of the 16 boulders must be several hitherto unknown kimberlite bodies in the Kirkland Lake and Lake Timiskaming kimberlite fields. 相似文献