全文获取类型
收费全文 | 5289篇 |
免费 | 1012篇 |
国内免费 | 1364篇 |
专业分类
测绘学 | 342篇 |
大气科学 | 1205篇 |
地球物理 | 1265篇 |
地质学 | 2931篇 |
海洋学 | 557篇 |
天文学 | 200篇 |
综合类 | 495篇 |
自然地理 | 670篇 |
出版年
2024年 | 28篇 |
2023年 | 112篇 |
2022年 | 270篇 |
2021年 | 320篇 |
2020年 | 235篇 |
2019年 | 288篇 |
2018年 | 358篇 |
2017年 | 318篇 |
2016年 | 321篇 |
2015年 | 270篇 |
2014年 | 317篇 |
2013年 | 278篇 |
2012年 | 302篇 |
2011年 | 351篇 |
2010年 | 339篇 |
2009年 | 284篇 |
2008年 | 220篇 |
2007年 | 251篇 |
2006年 | 232篇 |
2005年 | 196篇 |
2004年 | 134篇 |
2003年 | 125篇 |
2002年 | 154篇 |
2001年 | 130篇 |
2000年 | 167篇 |
1999年 | 237篇 |
1998年 | 162篇 |
1997年 | 185篇 |
1996年 | 165篇 |
1995年 | 164篇 |
1994年 | 133篇 |
1993年 | 164篇 |
1992年 | 100篇 |
1991年 | 78篇 |
1990年 | 56篇 |
1989年 | 50篇 |
1988年 | 41篇 |
1987年 | 33篇 |
1986年 | 21篇 |
1985年 | 15篇 |
1984年 | 8篇 |
1983年 | 8篇 |
1982年 | 12篇 |
1981年 | 3篇 |
1980年 | 6篇 |
1979年 | 5篇 |
1963年 | 1篇 |
1958年 | 14篇 |
1954年 | 1篇 |
1947年 | 1篇 |
排序方式: 共有7665条查询结果,搜索用时 0 毫秒
71.
72.
鄂西地区完整灰岩地层的视电阻率、密度、声波、自然伽马等曲线形态受灰岩胶结物质成份和泥质含量影响并具有一定的规律性,当灰岩地层受到构造、溶蚀作用产生破碎带、岩溶、裂隙等不良地质体或存在地下含水体时,各测井物理参数发生变化并在曲线形态上呈现异常反映,据此可以对不良地质体的位置、规模、类型进行准确判断。测井技术在鄂西地区灰岩地区隧道深孔勘探中的应用,补充、验证了钻探资料,为隧道设计、施工提供了可靠的依据。 相似文献
73.
74.
湖北宜昌石板溪金矿区断层空间结构及其控矿规律研究 总被引:1,自引:0,他引:1
断层空间结构包括变形结构和几何结构两部分。本文在解析石板溪金矿区主要断层变形结构和几何结构的基础上,探讨了其空间结构模式和控矿规律。 相似文献
75.
76.
Gui Liu Yongsheng Zhou Changrong He Wenming Yao Junlai Liu Yuanyuan Zhang 《Geological Journal》2016,51(1):92-112
We performed deformation experiments on a foliated mylonite under high temperature and pressure conditions in this study. To investigate the effect of pre‐existing fabric on the rheology of rocks, our samples were drilled from natural mylonite with the cylinder axis parallel to the foliation (PAR) and perpendicular to the foliation (PER). We performed 25 tests on seven PAR samples and 21 tests on seven PER samples at temperatures ranging from 600 to 890 °C, confining pressures ranging from 800 to 1400 MPa, and steady‐state strain rates of 1 × 10−4, 1 × 10−5 and 2.5 × 10−6 s−1. In the temperatures of 600–700 °C, the deformation is accommodated by semi‐brittle flow, with the average stress exponent being 6–7 assuming power law flow; in the temperature range of 800–890 °C, deformation is mainly by plastic flow, with an average stress exponent of n = 3 and activation energies of Q = 354 ± 52 kJ/mol (PER and PAR samples). The experimental results show that the strengths of PER samples are higher than those of PAR samples. Deformation microstructures have been studied by optical and electron microscopy. The original foliation of PER samples is destroyed by deformation and replaced by a new foliation, but the deformation of PAR samples followed the original foliation. Electron backscatter diffraction (EBSD) measurements show a strong lattice preferred orientation (LPO) of the quartz c axis fabrics of the starting samples and deformed PER and PAR samples. However, the c axis fabric of quartz in experimentally deformed PER and PAR samples varied with temperature and strain rate is different from that seen in the starting mylonite sample. The initial quartz c axis fabric of the starting mylonite sample has been transformed into a new fabric during experimental deformation. Dehydration melting of biotite and hornblende occurred in both PER and PAR samples at temperatures of 800–890 °C. Copyright © 2014 John Wiley & Sons, Ltd. 相似文献
77.
利用引入水稳定同位素循环的ECHAM4、GISS E、HadCM3、MUGCM以及iAWBM的模拟数据,分析了全球降水中稳定同位素效应的空间分布特征,对不同模式的模拟结果之间以及模拟结果与GNIP(Global Network of Isotopes in Precipitation)的实际监测结果之间进行了比较,旨在对稳定同位素大气环流模式的模拟有效性进行评价,改善对水循环中水稳定同位素效应的理解和认识。结果显示,5个模式均很好地再现了全球降水中平均δ18O和平均δ18O季节差的空间分布特征,降水中稳定同位素的温度效应、降水量效应的分布特点以及全球大气水线GMWL(Global Meteoric Water Line)均被很好地模拟出。比较而言,ECHAM4模拟的降水中的平均δ18O以及δ18O平均季节差的空间分布与GNIP的实际分布最接近,拟合水平也最高;ECHAM4、GISS E、MUGCM和iAWBM再现全球温度效应空间分布的能力较强,拟合水平大致相当;由iAWBM模拟的降水量效应空间分布与实际分布之间的相关性最强,5个模式模拟的与实测的δ18O/P相关系数符号相同的站点数大致位于同一水平;GISS E和iAWBM模拟的全球大气水线与实测的GMWL最接近。 相似文献
78.
Xisheng Xu William L. Griffin Xi Ma Suzanne Y. O’Reilly Zhenyu He Chengli Zhang 《Mineralogy and Petrology》2009,97(1-2):43-59
The "Taihua Group" is a collective term for a series of old terranes scattered along the southern margin of the North China Craton. The timing of formation and thermal overprinting of the Taihua Group have long been contentious, and its relationship with the Qinling orogenic belt has been unclear. In this study, new data from integrated in-situ U–Pb dating and Hf isotope analysis of zircons from an amphibolite (from the Xiong’ershan terrane) and a biotite gneiss (from the Lantian-Xiaoqinling terrane) indicate that the Upper Taihua Group formed during the Paleoproterozoic (2.3–2.5 Ga) and thus was originally part of the southern edge of North China Craton, detached during the Mesozoic Qinling orogeny and displaced about 100 km north from its original location. This suggests that the Taihua Group became part of the tectonic terrane associated with the Qinling orogeny and now forms part of the overthrust basement section of the Qinling belt. Before the Qinling orogeny, the Taihua Group was metamorphosed at 2.1 Ga. The initial Hf-isotope compositions of zircons, together with positive εNd(t) values for the whole-rocks, imply that the original magmas were derived from a juvenile source with some assimilation of an Archean crustal component. 相似文献
79.
Jian-Qing Feng Jian-Jun Liu Fei He Wei Yan Xin Ren Xu Tan Ling-Ping He Bo Chen Wei Zuo Wei-Bin Wen Yan Su Yong-Liao Zou Chun-Lai Li 《中国天文和天体物理学报》2014,(12)
The Extreme Ultraviolet Camera(EUVC) onboard the Chang'e-3(CE-3)lander is used to observe the structure and dynamics of Earth's plasmasphere from the Moon. By detecting the resonance line emission of helium ions(He+) at 30.4 nm, the EUVC images the entire plasmasphere with a time resolution of 10 min and a spatial resolution of about 0.1 Earth radius(RE) in a single frame. We first present details about the data processing from EUVC and the data acquisition in the commissioning phase, and then report some initial results, which reflect the basic features of the plasmasphere well. The photon count and emission intensity of EUVC are consistent with previous observations and models, which indicate that the EUVC works normally and can provide high quality data for future studies. 相似文献
80.
The IRAS and 2MASS associations for 193 T Tauri stars are identified in this paper. From the color–color diagrams and spectral index, it is found that the IR excesses for most samples are due to thermal emission from the circumstellar material, as suggested previously. It is also found that the IR excesses at IRAS region for few T Tauri stars and the near-IR excesses for some T Tauri stars are likely attributed to free-free emission or free-bound emission from the circumstellar ionized gas. Moreover, It is found in deredened J–H versus H–K color–color diagram that there is a slight separation in different spectral groups. The T Tauri stars locus equation in J–H versus H–K color–color diagram for our sample is also presented. 相似文献