全文获取类型
收费全文 | 4209篇 |
免费 | 586篇 |
国内免费 | 339篇 |
专业分类
测绘学 | 57篇 |
大气科学 | 53篇 |
地球物理 | 1011篇 |
地质学 | 1527篇 |
海洋学 | 382篇 |
天文学 | 1607篇 |
综合类 | 128篇 |
自然地理 | 369篇 |
出版年
2024年 | 12篇 |
2023年 | 29篇 |
2022年 | 60篇 |
2021年 | 75篇 |
2020年 | 71篇 |
2019年 | 104篇 |
2018年 | 81篇 |
2017年 | 97篇 |
2016年 | 96篇 |
2015年 | 113篇 |
2014年 | 187篇 |
2013年 | 208篇 |
2012年 | 169篇 |
2011年 | 180篇 |
2010年 | 160篇 |
2009年 | 300篇 |
2008年 | 294篇 |
2007年 | 363篇 |
2006年 | 275篇 |
2005年 | 252篇 |
2004年 | 201篇 |
2003年 | 213篇 |
2002年 | 184篇 |
2001年 | 157篇 |
2000年 | 182篇 |
1999年 | 179篇 |
1998年 | 163篇 |
1997年 | 108篇 |
1996年 | 110篇 |
1995年 | 80篇 |
1994年 | 73篇 |
1993年 | 69篇 |
1992年 | 57篇 |
1991年 | 40篇 |
1990年 | 49篇 |
1989年 | 40篇 |
1988年 | 33篇 |
1987年 | 18篇 |
1986年 | 15篇 |
1985年 | 11篇 |
1984年 | 3篇 |
1983年 | 2篇 |
1982年 | 2篇 |
1981年 | 4篇 |
1980年 | 5篇 |
1979年 | 1篇 |
1978年 | 5篇 |
1954年 | 4篇 |
排序方式: 共有5134条查询结果,搜索用时 15 毫秒
71.
本文综述了1989年4月至1990年1月秦山核电站邻近水域生态调查结果,认为,该水域具暖温带强潮河口区生态特征。水体虽含丰富营养盐和充足溶解氧,由于同时存在着各种不利于生物繁殖生长的环境因子,表现为生物资源贫瘠、种类组成简单,测区所代表的强潮河口湾顶区属低生产力水域。 相似文献
72.
Makoto Yoshikawa 《Celestial Mechanics and Dynamical Astronomy》1992,54(1-3):287-290
Motions of asteroids in mean motion resonances with Jupiter are studied in three-dimensional space. Orbital changes of fictitious asteroids in the Kirkwood gaps are calculated by numerical integrations for 105 – 106 years. The main results are as follows: (1) There are various motions of resonant asteroids, and some of them are very complicated and chaotic and others are regular. (2) The eccentricity of some asteroids becomes very large, and the variation of the inclination is large while the eccentricity is large. (3) In the 3:1 resonance, there is a long periodic change in the variation of the inclination, when (7 : ) is a simple ratio (7: longitude of perihelion, : longitude of node). (4) In the 7:3 resonance, the variation of the inclination of some resonant asteroids is so large that prograde motion becomes retrograde. Some asteroids in the 7:3 resonance can collide with the Sun as well as with the inner planets. 相似文献
73.
74.
75.
直流输电线路对磁测的影响 总被引:3,自引:0,他引:3
越来越多的远距离、大容量直流输电线路投入运行对线路附近地区的磁测工作产生了不可忽视的影响。本文阐述了直流输电线路的结构、线路磁场特征及对以地质找矿为目的的磁测工作的影响。对直流输电线路磁场在磁测图中的特点也做了讨论,列举了直流输电线路影响的实例。 相似文献
76.
在工作程度高的地区如何筛选矿致磁异常 总被引:1,自引:0,他引:1
分析了在工作程度高的地区进一步筛选矿致磁异常的可能性;提出了在工作程度高的地区筛选矿致磁异常的优先顺序建议。 相似文献
77.
邹平铜矿处于齐河-广饶深大断裂带南部的邹平火山岩盆地中,形成于破火山口火山通道充填的石英正长闪长岩岩颈中央上部,包括伟晶岩型铜矿和细脉浸染状斑铜矿床两种类型。前者矿体较小,但品位高;后者品位较低,但规模中等。含矿石英正长闪长岩等密度小、磁性弱,故在火山岩系中呈现高背景重力场上的重力低和杂乱高磁场背景中的低负异常,即“重磁同低”,且高极化。重磁同低异常区和高极化率异常带,是本区寻找铜矿的有利部位。 相似文献
78.
S. I. Mayr H. Burkhardt Yu. Popov A. Wittmann 《International Journal of Earth Sciences》2008,97(2):385-399
Internal surface, formation factor, Nuclear Magnetic Resonance (NMR)-T2 relaxation times and pore radius distributions were
measured on representative core samples for the estimation of hydraulic permeability. Permeability is estimated using various
versions of the classic Kozeny–Carman-equation (K–C) and a further development of K–C, the fractal PaRiS-model, taking into
account the internal surface. In addition to grain and pore size distribution, directly connected to permeability, internal
surface reflects the internal structure (“micro morphology”). Lithologies could be grouped with respect to differences in
internal surface. Most melt rich impact breccia lithologies exhibit large internal surfaces, while Tertiary post-impact sediments
and Cretaceous lithologies in displaced megablocks display smaller internal surfaces. Investigations with scanning electron
microscopy confirm the correlation between internal surface and micro morphology. In addition to different versions of K–C,
estimations by means of NMR, pore radius distributions and some gas permeability measurements serve for cross-checking and
calibration. In general, the different estimations from the independent methods and the measurements are in satisfactory accordance.
For Tertiary limestones and Suevites bulk with very high porosities (up to 35%) permeabilites between 10−14 and 10−16 m2 are found, whereas in lower Suevite, Cretaceous anhydrites and dolomites, bulk permeabilites are between 10−15 and 10−23 m2. 相似文献
79.
The Glueckstadt Graben of the North-German Basin: new insights into the structure from 3D and 2D gravity analyses 总被引:1,自引:0,他引:1
Tamara Yegorova Yuriy Maystrenko Ulf Bayer Magdalena Scheck-Wenderoth 《International Journal of Earth Sciences》2008,97(5):915-930
The structure of the Glueckstadt Graben has been investigated by use of 3D gravity backstripping technique and by 2D gravity
and magnetic modelling. Subtracting the gravity effects of the Meso-Cenozoic sediments together with Permian salt reveals
a positive residual anomaly within the Glueckstadt Graben. This anomaly includes two local maxima over the Westholstein and
Eastholstein Troughs. The 2D gravity models point to the presence of a high-density body within the lower crust of the Glueckstadt
Graben. In addition, the results of 2D magnetic modelling indicate that the central part of the high-density body is overlain
by an area with high susceptibility. Most probable, the formation of this high-density body is a result of complex poly-phase
tectonic history of the study area. Finally, the results of gravity modelling indicate that Permian salt is not homogeneous.
3D gravity analysis and, especially, 2D gravity modelling have distinguished the differences in degree of salt saturation
in salt-rich bodies, and elucidate the proportion of Rotliegend salt. 相似文献
80.
The planet Mars lacks, today, a planetary, dynamic magnetic field, but strong, intense, localized magnetic fields of lithospheric origin, one to two orders of magnitude larger than the terrestrial lithospheric field, are present. This lithospheric magnetic field is the result of magnetization processes in the presence of a magnetic dynamo and of demagnetization processes after the dynamo shutdown, such as impact or volcanoes. This crude scenario can be more accurately specified by interpreting global and local models of the current magnetic field of Mars. Some specific areas are studied, including the intensely magnetized Terra Sirenum, as well as the magnetic anomaly associated with Apollinaris Patera. Magnetic minerals could be of primary and/or secondary origin; this latter would imply an early hydration of a basaltic crust. A scenario, in which Mars experienced a major polar wander due to the Tharsis bulge, prior to the cessation of its dynamo, is proposed and discussed. 相似文献