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   2094篇
  免费   321篇
  国内免费   464篇
测绘学   193篇
大气科学   195篇
地球物理   506篇
地质学   1022篇
海洋学   260篇
天文学   182篇
综合类   118篇
自然地理   403篇
  2024年   8篇
  2023年   20篇
  2022年   39篇
  2021年   59篇
  2020年   62篇
  2019年   82篇
  2018年   53篇
  2017年   79篇
  2016年   66篇
  2015年   98篇
  2014年   98篇
  2013年   132篇
  2012年   114篇
  2011年   117篇
  2010年   133篇
  2009年   138篇
  2008年   140篇
  2007年   135篇
  2006年   175篇
  2005年   136篇
  2004年   123篇
  2003年   98篇
  2002年   90篇
  2001年   99篇
  2000年   76篇
  1999年   81篇
  1998年   53篇
  1997年   47篇
  1996年   54篇
  1995年   45篇
  1994年   41篇
  1993年   38篇
  1992年   35篇
  1991年   27篇
  1990年   17篇
  1989年   15篇
  1988年   20篇
  1987年   7篇
  1986年   7篇
  1985年   6篇
  1984年   2篇
  1983年   2篇
  1982年   3篇
  1981年   4篇
  1980年   2篇
  1979年   1篇
  1954年   2篇
排序方式: 共有2879条查询结果,搜索用时 0 毫秒
11.
12.
球面似均匀格网的剖分方法及特征分析   总被引:2,自引:1,他引:2  
给出球面"似均匀格网"概念的内涵,并介绍3种常用的球面似均匀格网(三角形格网、菱形格网和六边形格网)的剖分方法.从几何上分析3种格网的单元特征及不同格网在不同领域的应用优势.通过对比得出3种格网的特征对照表及相互关系,即:三角形格网是最基本的球面剖分格网,球面六边形格网和菱形格网可以通过球面三角格网来生成,且这3种剖分格网各有优缺点并在一定条件下可以相互转换.  相似文献   
13.
14.
断裂构造的遥感研究方法综述   总被引:1,自引:0,他引:1  
断裂构造是一种基本的构造型式。断裂构造遥感研究是高新探测技术与地球科学的有机结合 ,是断裂构造常规研究方法的有益补充和向纵深拓展的必然趋势。该文从总体思路、具体内容、操作方法等各个不同角度系统地论述了断裂构造遥感研究的现状和发展趋势 ,并在断裂构造信息提取、光谱特征分析、空间结构分析 (包括分形分析 )等方面提出了一些观点。  相似文献   
15.
The occurrence of superluminal motion in extragalactic radio sources is believed to be quite common. Among others, the geometrical scattering of radio radiation can also cause superluminal expansion and or motion and halo formation, In this paper, the effectiveness of the stimulated Raman scattering in producing these features is investigated. The scattering medium is a plasma whose position, density and temperature decide the rate and angle of scattering. When the radiation from a stationary and constant source gets scattered from a stationary plasma, a halo is formed around the source. However, the scattering of a rotating radiation beam does produce superluminal motion of the virtual source. It is found that the plasma should have the characteristics of the emission-line regions and the intercloud medium in order to Raman scatter the radiation. Since the scattering is polarization dependent, it is possible to estimate the rotation of the electric vector along the direction of the apparent motion of a radio source.  相似文献   
16.
We present the results of our comparative timing and spectral analysis of the high and low (off) states in the X-ray pulsar Her X-1 based on data from the ART-P telescope onboard the Granat observatory. A statistically significant (several mCrab) persistent flux with a simple power-law spectrum was detected during the low state. The spectral slope changed from observation to observation by almost a factor of 2. Pulsations were detected only during the high state of the source, when its flux was a factor of ~25 larger than the low-state flux. The spectral shape of Her X-1 in its high state was complex, with the parameters depending on pulse phase.  相似文献   
17.
Large scale seismic anisotropy in the Earth's mantle is likely dynamically supported by the mantle's deformation; therefore, tomographic imaging of 3-D anisotropic mantle seismic velocity structure is an important tool to understand the dynamics of the mantle. While many previous studies have focused on special cases of symmetry of the elastic properties, it would be desirable for evaluation of dynamic models to allow more general axis orientation. In this study, we derive 3-D finite-frequency surface wave sensitivity kernels based on the Born approximation using a general expression for a hexagonal medium with an arbitrarily oriented symmetry axis. This results in kernels for two isotropic elastic coefficients, three coefficients that define the strength of anisotropy, and two angles that define the symmetry axis. The particular parametrization is chosen to allow for a physically meaningful method for reducing the number of parameters considered in an inversion, while allowing for straightforward integration with existing approaches for modelling body wave splitting intensity measurements. Example kernels calculated with this method reveal physical interpretations of how surface waveforms are affected by 3-D velocity perturbations, while also demonstrating the non-linearity of the problem as a function of symmetry axis orientation. The expressions are numerically validated using the spectral element method. While challenges remain in determining the best inversion scheme to appropriately handle the non-linearity, the approach derived here has great promise in allowing large scale models with resolution of both the strength and orientation of anisotropy.  相似文献   
18.
在介绍鄂尔多斯盆地吴堡地区延长组长6段沉积特征的基础上,探讨了该储层物性特征、浊积岩特征、浊积岩分布规律及其对油藏的影响,明确了浊流沉积的石油地质意义.结果表明:鄂尔多斯盆地吴堡地区长6段以发育长石砂岩为主,填隙物成分有方解石、绿泥石、白云母以及少量的石英加大、长石加大等,砂岩储集层孔隙结构具有很强的非均质性;吴堡地区长6期湖盆沉降趋于稳定,是三角洲的高建设时期;多水系、多物源的三角洲前缘沉积为深湖浊积扇沉积提供了充足的物质基础;在吴堡地区东北部三角洲前缘水下分流河道前端发育深湖浊积扇沉积,可区分出中心微相和边缘微相两个沉积微相带,其中浊积扇中心微相以细砂岩、粉砂岩与暗色泥岩呈砂泥互层;从平面上看,浊积岩砂体非均质性在侧向上逐渐变弱,砂体底部发育厚度较大、成熟度较高的暗色湖相沉积的烃源岩,深湖相的暗色泥岩含有丰富的烃源岩,而浊积岩砂体是由深湖相的暗色泥岩构成,孔渗物性好的区域易于形成良好的上倾尖灭的透镜状岩性油藏.  相似文献   
19.
We investigate a scenario of photon scattering by electrons within a relativistic outflow. The outflow is composed of discrete shells with different speeds. One shell emits radiation for a short duration. Some of this radiation is scattered by the shell(s) behind. We calculate in a simple two-shell model the observed scattered flux density as a function of the observed primary flux density, the normalized arrival time delay between the two emission components, the Lorentz factor ratio of the two shells and the scattering shell's optical depth. Thomson scattering in a cold shell and inverse Compton scattering in a hot shell are both considered. The results of our calculations are applied to the gamma-ray bursts and the afterglows. We find that the scattered flux from a cold slower shell is small and likely to be detected only for those bursts with very weak afterglows. A hot scattering shell could give rise to a scattered emission as bright as the X-ray shallow decay component detected in many bursts, on a condition that the isotropically equivalent total energy carried by the hot electrons is large, ∼1052–1056 erg. The scattered emission from a faster shell could appear as a late short γ-ray/MeV flash or become part of the prompt emission depending on the delay of the ejection of the shell.  相似文献   
20.
黄蓉  王辉  王蕙  南耀明  赵赫然  段雅楠 《中国沙漠》2013,33(6):1782-1788
为探讨华家岭低效防护林带改造对土壤的改良效果,在华家岭地区选取生长不良的低效杨树纯林和改造后的云杉纯林、云杉×杨树、云杉×油松、云杉×落叶松混交林5种典型林带类型,对其土壤理化性状进行对比研究。结果表明:(1)云杉纯林及其混交林土壤的平均容重、平均毛管孔隙度、总孔隙度、通气度与杨树纯林的差异显著(p<0.05),经过低效林改造后的云杉纯林及其混交林较杨树纯林的土壤容重有所下降,孔隙度和通气性有所提高\.(2)除速效P外,各林型的土壤速效N、速效K、全N、全P、全K和有机质含量随土层深度的增加而降低;云杉纯林及其混交林的土壤有机质含量、速效N、P、K和全量N、P、K养分均高于杨树纯林,pH值低于杨树纯林\.(3)云杉纯林及其混交林的有机质含量和全N含量与容重和总孔隙度的相关性较杨树纯林的好,云杉纯林及其混交林对土壤理化性能的改良作用优于杨树纯林。  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