首页 | 本学科首页   官方微博 | 高级检索  
文章检索
  按 检索   检索词:      
出版年份:   被引次数:   他引次数: 提示:输入*表示无穷大
  收费全文   3691篇
  免费   531篇
  国内免费   315篇
测绘学   47篇
大气科学   26篇
地球物理   802篇
地质学   1458篇
海洋学   249篇
天文学   1482篇
综合类   120篇
自然地理   353篇
  2024年   9篇
  2023年   27篇
  2022年   44篇
  2021年   64篇
  2020年   65篇
  2019年   96篇
  2018年   71篇
  2017年   71篇
  2016年   90篇
  2015年   95篇
  2014年   176篇
  2013年   199篇
  2012年   164篇
  2011年   156篇
  2010年   152篇
  2009年   281篇
  2008年   266篇
  2007年   338篇
  2006年   248篇
  2005年   222篇
  2004年   183篇
  2003年   188篇
  2002年   162篇
  2001年   139篇
  2000年   159篇
  1999年   153篇
  1998年   147篇
  1997年   93篇
  1996年   96篇
  1995年   61篇
  1994年   57篇
  1993年   39篇
  1992年   46篇
  1991年   19篇
  1990年   45篇
  1989年   30篇
  1988年   30篇
  1987年   17篇
  1986年   11篇
  1985年   8篇
  1984年   3篇
  1982年   2篇
  1981年   4篇
  1980年   4篇
  1978年   4篇
  1954年   3篇
排序方式: 共有4537条查询结果,搜索用时 218 毫秒
81.
岩石受压破裂的ULF和LF电磁前兆信号   总被引:15,自引:1,他引:15  
实验观测到了4类岩性、18块样品在单轴压力下直至破裂发生全过程中的ULF和LF电磁前兆信号。这些不同频率的信号是零散出现的,其形态为一组组脉冲,宽度为4ms~16ms,幅度为0.1mV~1.4mV。实验发现具同一谐振频率的天线收到的信号频次与其相对于裂缝的位置和方位有关。结果还表明,电磁前兆信号的频度与岩样强度有关,抗压强度高的岩样电磁前兆信号多。微破裂可能产生了偶电层,在破裂过程中向外辐射,产生了LF频段的磁信号,ULF磁信号则主要由压磁效应产生。  相似文献   
82.
邓韫 《华南地震》2003,23(1):51-56
根据1900~2000年中国大陆、台湾及全球地层记录及前人的研究,论证了地层周期存在的可能性及形成机制。作者认为,是太阳活动、月球运动轨道及各行星运动轨道的周期性变化,通过磁力及万有引力改变地球内部物质的分布,从而引起地球自转速度的周期性变化,最终致使地展出现周期性的活跃期及平静期。  相似文献   
83.
Statistical analysis of the magnetic fabric of samples from several successive lava flows emplaced under similar conditions can allow determination of the mean flow direction when magnetic fabric data from individual flows do not lead to reliable results. A difference between the obtained flow direction and the present dip direction indicates that the flows were tilted after emplacement. For 2 successive series of flows on the Jeanne d’Arc Peninsula presently NNW dipping, this method shows lava emplacement along a SSW–NNE direction. This indicates a gentle tilting acquired during a period of weak deformation in the whole archipelago. Additionally, the magnetic fabric data allow the reconstruction of the different conditions of emplacement of these two series of lava flows and of formation of the local thick conglomerate interbedded between these series.  相似文献   
84.
Big perturbations of the magnetic field (amplitudes larger than 250 nT) are simply detected by subtracting the values of a model from the measurements of CHAMP satellite. Taking a full year of CHAMP data and organizing them in four subsets of three months length (spring, summer, autumn, winter), it is found that: (a) the two domains where such big perturbations mainly exist are limited, in both hemispheres, by a parallel of high latitude of the corrected geomagnetic coordinates system; (b) a conspicuous seasonal (annual) variation affects the density of the perturbations and is opposite in the two hemispheres. We hold that these perturbations are linked to the midday magnetic activity within the auroral zone, long ago described by one of us (Mayaud, 1956). The source of the perturbations observed at the satellite altitude would be field-aligned currents resulting from the penetration of the solar wind into the magnetospheric cusps. To cite this article: J.-L. Le Mouël et al., C. R. Geoscience 335 (2003).  相似文献   
85.
By analysing a series of four successive thin‐sections from a ceramic clay that was subjected to uniaxial compression, we were able to monitor the development of microstructures in a fine‐grained sediment. The artificially induced microstructures, such as unidirectional clay reorientations and linear and circular grain arrangements, are identical to features that have been observed in thin‐sections of subglacially deformed tills, and therefore may be used as representative analogues. We argue that the structures, reflecting slip, planar shear displacements as well as rotational movements, can be explained by assuming a Coulomb‐plastic response to imposed shear. We conclude that sediments subjected to subglacial deformation behave as Coulomb materials, at least during the final stages of the deformation. The present study bridges the gap between field studies, experimental studies and theoretical modelling. The microscopic observations assist in visualising inferred subglacial processes and facilitate up‐ and downscaling between diverse methodological approaches. Copyright © 2003 John Wiley & Sons, Ltd.  相似文献   
86.
The anisotropy of magnetic susceptibility (AMS) of single crystals of biotite, muscovite and chlorite has been measured in order to provide accurate values of the magnetic anisotropy properties for these common rock-forming minerals. The low-field AMS and the high-field paramagnetic susceptibility are defined. For the high-field values, it is necessary to combine the paramagnetic deviatoric tensor obtained from the high-field torque magnetometer with the paramagnetic bulk susceptibility measured from magnetization curves of the crystals. This leads to the full paramagnetic susceptibility ellipsoid due to the anisotropic distribution of iron cations in the silicate lattice. The ellipsoid of paramagnetic susceptibility, which was obtained for the three phyllosilicates, is highly oblate in shape and the minimum susceptibility direction is subparallel to the crystallographic c-axes. The anisotropy of the susceptibility within the basal plane of the biotite has been evaluated and found to be isotropic within the accuracy of the instrumental measurements. The degree of anisotropy of biotite and chlorite is compatible with previously reported values while for muscovite the smaller than previously published values. The shape of the chlorite AMS ellipsoid for all the samples is near-perfect oblate in contrast with a wide distribution of oblate and prolate values reported in earlier studies. Reliable values are important for deriving models of the magnetic anisotropy where it reflects mineral fabrics and deformation of rocks.  相似文献   
87.
Low concentrate density from wet drum magnetic separators in dense medium circuits can cause operating difficulties due to inability to obtain the required circulating medium density and, indirectly, high medium solids losses. The literature is almost silent on the processes controlling concentrate density. However, the common name for the region through which concentrate is discharged—the squeeze pan gap—implies that some extrusion process is thought to be at work. There is no model of magnetics recovery in a wet drum magnetic separator, which includes as inputs all significant machine and operating variables.A series of trials, in both factorial experiments and in single variable experiments, was done using a purpose built rig which featured a small industrial scale (700 mm lip length, 900 mm diameter) wet drum magnetic separator. A substantial data set of 191 trials was generated in this work. The results of the factorial experiments were used to identify the variables having a significant effect on magnetics recovery.It is proposed, based both on the experimental observations of the present work and on observations reported in the literature, that the process controlling magnetic separator concentrate density is one of drainage. Such a process should be able to be defined by an initial moisture, a drainage rate and a drainage time, the latter being defined by the volumetric flowrate and the volume within the drainage zone. The magnetics can be characterised by an experimentally derived ultimate drainage moisture. A model based on these concepts and containing adjustable parameters was developed. This model was then fitted to a randomly chosen 80% of the data, and validated by application to the remaining 20%. The model is shown to be a good fit to data over concentrate solids content values from 40% solids to 80% solids and for both magnetite and ferrosilicon feeds.  相似文献   
88.
The polyphase evolution of the Seridó Belt (NE-Brazil) includes D1 crust formation at 2.3–2.1 Ga, D2 thrust tectonics at 1.9 Ga and crustal reworking by D3 strike-slip shear zones at 600 Ma. Microstructural investigations within mylonites associated with D2 and D3 events were used to constrain the tectono-thermal evolution of the belt. D2 shear zones commenced at deeper crustal levels and high amphibolite facies conditions (600–650 °C) through grain boundary migration, subgrain rotation and operation of quartz c-prism slip. Continued shearing and exhumation of the terrain forced the re-equilibration of high-T fabrics and the switching of slip systems from c-prism to positive and negative a-rhombs. During D3, enhancement of ductility by dissipation of heat that came from syn-D3 granites developed wide belts of amphibolite facies mylonites. Continued shearing, uplift and cooling of the region induced D3 shear zones to act in ductile-brittle regimes, marked by fracturing and development of thinner belts of greenschist facies mylonites. During this event, switching from a-prism to a-basal slip indicates a thermal path from 600 to 350 °C. Therefore, microstructures and quartz c-axis fabrics in polydeformed rocks from the Seridó Belt preserve the record of two major events, which includes contrasting deformation mechanisms and thermal paths.  相似文献   
89.
重磁遗传算法三维反演中高速计算及有效存储方法技术   总被引:13,自引:15,他引:13       下载免费PDF全文
将地下场源区域规则划分成很多小长方体单元,并且通过反演确定这些单元的物性变 化,勾画出场源的分布图像,这种方式逐步成为重磁反演,特别是三维反演的重要方向;遗 传算法等非线性技术进行该类反演将逐步成为发展趋势. 本文指出,在应用遗传算法进行该 类反演过程中,隐含着数据量较大时超常规的计算量,它已成为制约该类反演充分发挥作用 的瓶颈问题;同时,本文提出了针对性的分离并存储几何格架的计算策略、以及独特的几何 格架等效压缩存储技术,可以从根本上提高非线性反演计算速度,为该类反演的有效应用奠 定了坚实的基础.  相似文献   
90.
高岭石—莫来石反应系列:^27Al和^29SiMAS NMR研究   总被引:21,自引:2,他引:21  
郭九皋  何宏平 《矿物学报》1997,17(3):250-259
根据艰我国八个不同成因和特征的高岭土样品在450-1450℃热处理产物的MAS NMR谱和XRD,IR,DTA等研究结果,结合有关资料讨论了高岭石-莫来石反应序列的几个重要问题:1.高岭石的结构,尤其是五配位铝;2.980℃放热峰后的高温相是γ-Al2O3而不是Al-Si尖晶石;3.对于莫来石化过程,认为初始莫来石850-950℃变高岭石形成,二次莫来石由分凝的SiO2和γ-Al2O3在1200-  相似文献   
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号