全文获取类型
收费全文 | 2510篇 |
免费 | 315篇 |
国内免费 | 453篇 |
专业分类
测绘学 | 184篇 |
大气科学 | 50篇 |
地球物理 | 593篇 |
地质学 | 1216篇 |
海洋学 | 219篇 |
天文学 | 590篇 |
综合类 | 153篇 |
自然地理 | 273篇 |
出版年
2024年 | 9篇 |
2023年 | 12篇 |
2022年 | 63篇 |
2021年 | 57篇 |
2020年 | 65篇 |
2019年 | 78篇 |
2018年 | 58篇 |
2017年 | 74篇 |
2016年 | 85篇 |
2015年 | 83篇 |
2014年 | 105篇 |
2013年 | 135篇 |
2012年 | 100篇 |
2011年 | 88篇 |
2010年 | 95篇 |
2009年 | 119篇 |
2008年 | 129篇 |
2007年 | 200篇 |
2006年 | 171篇 |
2005年 | 135篇 |
2004年 | 156篇 |
2003年 | 153篇 |
2002年 | 142篇 |
2001年 | 106篇 |
2000年 | 123篇 |
1999年 | 96篇 |
1998年 | 88篇 |
1997年 | 92篇 |
1996年 | 71篇 |
1995年 | 73篇 |
1994年 | 64篇 |
1993年 | 62篇 |
1992年 | 47篇 |
1991年 | 29篇 |
1990年 | 24篇 |
1989年 | 25篇 |
1988年 | 24篇 |
1987年 | 20篇 |
1986年 | 11篇 |
1985年 | 5篇 |
1984年 | 1篇 |
1982年 | 1篇 |
1981年 | 1篇 |
1978年 | 1篇 |
1977年 | 1篇 |
1954年 | 1篇 |
排序方式: 共有3278条查询结果,搜索用时 62 毫秒
11.
G. A. Krasinsky 《Celestial Mechanics and Dynamical Astronomy》2002,84(1):27-55
Differential equations describing the tidal evolution of the earth's rotation and of the lunar orbital motion are presented in a simple close form. The equations differ in form for orbits fixed to the terrestrial equator and for orbits with the nodes precessing along the ecliptic due to solar perturbations. Analytical considerations show that if the contemporary lunar orbit were equatorial the evolution would develop from an unstable geosynchronous orbit of the period about 4.42 h (in the past) to a stable geosynchronous orbit of the period about 44.8 days (in the future). It is also demonstrated that at the contemporary epoch the orbital plane of the fictitious equatorial moon would be unstable in the Liapunov's sense, being asymptotically stable at early stages of the evolution. Evolution of the currently near-ecliptical lunar orbit and of the terrestrial rotation is traced backward in time by numerical integration of the evolutional equations. It is confirmed that about 1.8 billion years ago a critical phase of the evolution took place when the equatorial inclination of the moon reached small values and the moon was in a near vicinity of the earth. Before the critical epoch t
cr
two types of the evolution are possible, which at present cannot be unambiguously distinguished with the help of the purely dynamical considerations. In the scenario that seems to be the most realistic from the physical point of view, the evolution also has started from a geosynchronous equatorial lunar orbit of the period 4.19 h. At t < t
cr
the lunar orbit has been fixed to the precessing terrestrial equator by strong perturbations from the earth's flattening and by tidal effects; at the critical epoch the solar perturbations begin to dominate and transfer the moon to its contemporary near-ecliptical orbit which evolves now to the stable geosynchronous state. Probably this scenario is in favour of the Darwin's hypothesis about originating the moon by its separation from the earth. Too much short time scale of the evolution in this model might be enlarged if the dissipative Q factor had somewhat larger values in the past than in the present epoch. Values of the length of day and the length of month, estimated from paleontological data, are confronted with the results of the developed model. 相似文献
12.
Andreas Burkert 《Astrophysics and Space Science》2003,284(2):697-700
The puzzling correlation between the spin parameter λ of galactic disks and the disk-to-halo mass fraction f
disk is investigated. It is shown that such a correlation arises naturally from large uncertainties in determining the virial
masses of dark matter halos. This result indicates that halo properties derived from fits to observed rotation curves are
still very uncertain. An analysis of λ versus f
disk as function of the adopted halo virial mass shows that for reasonable halo concentrations f
disk ≈ 0.01 - 0.07 which is significantly smaller than the universal baryon fraction. Most of the available gas either never settled
into the galactic disks or was ejected subsequently.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
13.
In this paper the tidal phenomena on the Earth are concisely specified, including solid tides, ocean tides and atmospheric tides due to the luni-solar tide-generating force, and the Earth pole tide due to the motion of the Earth's rotation axis (polar motion); as well as their effects on the Earth rotation. The outcomes of scientific researches of Chinese astronomers on these topics are described in some detail. These researches deal with the mechanisms responsible for tidal effects on the earth rotation, and on the measurements of the Earth rotation parameters. Finally, the effects discovered by Chinese researchers on the measurements of the period and change in period of pulsars are discussed. These effects are very small in magnitude but not negligible. 相似文献
14.
15.
16.
Dynamic recrystallization near the brittle-plastic transition in naturally and experimentally deformed quartz aggregates 总被引:1,自引:0,他引:1
The electron backscattering diffraction technique (EBSD) was used to analyze bulging recrystallization microstructures from naturally and experimentally deformed quartz aggregates, both of which are characterized by porphyroclasts with finely serrated grain boundaries and grain boundary bulges set in a matrix of very fine recrystallized grains. For the Tonale mylonites we investigated, a temperature range of 300–380 °C, 0.25 GPa confining pressure, a flow stress range of ~ 0.1–0.2 GPa, and a strain rate of ~ 10− 13 s− 1 were estimated. Experimental samples of Black Hills quartzite were analyzed, which had been deformed in axial compression at 700 °C, 1.2–1.5 GPa confining pressure, a flow stress of ~ 0.3–0.4 GPa, a strain rate of ~ 10− 6 s− 1, and to 44% to 73% axial shortening. Using orientation imaging we investigated the dynamic recrystallization microstructures and discuss which processes may contribute to their development. Our results suggest that several deformation processes are important for the dismantling of the porphyroclasts and the formation of recrystallized grains. Grain boundary bulges are not only formed by local grain boundary migration, but they also display a lattice misorientation indicative of subgrain rotation. Dynamic recrystallization affects especially the rims of host porphyroclasts with a hard orientation, i.e. with an orientation unsuitable for easy basal slip. In addition, Dauphiné twins within porphyroclasts are preferred sites for recrystallization. We interpret large misorientation angles in the experimental samples, which increase with increasing strain, as formed by the activity of fluid-assisted grain boundary sliding. 相似文献
17.
对华南前寒武系变质岩浆杂岩稀有气体He、Ne、Ar和Xe的系统研究表明:扬子克拉通基底为含高3He的下地壳"原始岩石层",(3He/4He)×10-6比值为2.8~4.6;而华夏板块基底变质岩浆杂岩则是在缺乏3He、低(3He/4He)×10-8比值(3.15~17.7)的构造环境下形成的大陆中-上地壳变质岩浆杂岩层,反映出两者基底性质迥然不同。华南中-新生代爆破岩筒He同位素组成相反,相对稳定的扬子克拉通(3He/4He)×10-8比值仅0.18~4.22,而郯庐-四会-吴川断裂以东,中-新生代活动地块(太平洋构造域)(3He/4He)×10-8比值高达3.7~20.5。He同位素表明郯庐-四会-吴川断裂带为切割深至地幔的边界深大断裂,是扬子克拉通与华夏板块间的边界且控制了燕山期火山-侵入岩浆向西扩展。Ar同位素组成表明华南大陆中-新生代地幔形成接近"均一"的地幔组份。136Xe/130Xe-129Xe/130Xe相关组份表明它们具有地幔柱岩石同位素组成特征。 相似文献
18.
From the experimental studies in recent years, it has become known that when a wave breaks directly on a vertical faced coastal structure, high magnitude impact pressures are produced. The theoretical and experimental studies show that the dynamic response of such structures under wave impact loading is closely dependent on the magnitude and duration of the load history. The dynamic analysis and design of a coastal structure can be succeeded provided the design load history for the wave impact is available. Since these types of data are very scarce, it is much more convenient to follow a method which is based on static analysis for the dynamic design procedure. Therefore, to facilitate the dynamic design of a vertical plate that is exposed to breaking wave impact, a multiplication factor called “dynamic magnification factor” is herein presented which is defined as the ratio of the maximum value of the dynamic response to that found by static analysis. The computational results of the present study show that the dynamic magnification factor is a useful ratio to transfer the results of static analysis to the dynamic design of a coastal plate for the maximum impact pressure conditions of pmax/γH0≤18. 相似文献
19.
对广东三水盆地上白垩统三水组、大 山组、古新统莘庄组及始新统 心组、宝月组的系统的古地磁研究结果表明:(1)旋转运动是该区构造运动的主要形式,顺时针旋转盆地拉张发育,这时针旋转盆地挤压衰亡,发育的程度与旋转角度有关;(2)始新世该区旋转方向由顺时针旋转变为道时针旋转,对应于太平洋-库拉板块对欧亚板块作用方向的改变,说明三水盆地的形成发育与太平洋-库拉板块对欧亚板块的作用密切相关;(3)三水盆地所在的华南地块从晚白垩世至始新世在纬向上不存在明显的运动,一直停留在略低于现今纬度的位置上。 相似文献
20.
东太平洋地区DSDP573孔始新世末期的微玻璃陨石 总被引:5,自引:1,他引:5
通过研究 DSDP5 73孔的岩心样品 ,首次在该孔始新世与渐新世的界线地层含金属粘土层中发现了微玻璃陨石 ,且主要富集在其底部。一个样品 (5 g)中最多可达 12粒。这些微玻璃陨石主要呈球形、椭球形。用电子探针测试了其化学成分 ,Si O2 含量为 2 9.6 4%~ 5 8.93%,Al2 O3 为 3.42 %~ 2 0 .96 %,Fe O为 9.98%~ 2 9.5 5 %,Mg O为 4.32 %~ 16 .0 5 %,Ir为 0 .0 6 %~ 0 .81%。总体来说 ,微玻璃陨石的化学成分变化较大 ,可能与靶岩的成分变化较大有关。始新世末期北美微玻璃陨石场的展布方向约为 2 5 0°,这与太平洋板块运动方向改变所需要的矢量变化(2 45°)仅相差 5°,推测很可能是始新世末期陨星的撞击引起了太平洋板块在该时期的运动方向由 NNW突然变为NWW。 相似文献