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   463篇
  免费   96篇
  国内免费   50篇
测绘学   89篇
大气科学   10篇
地球物理   214篇
地质学   140篇
海洋学   35篇
天文学   52篇
综合类   31篇
自然地理   38篇
  2023年   6篇
  2022年   7篇
  2021年   11篇
  2020年   9篇
  2019年   25篇
  2018年   8篇
  2017年   24篇
  2016年   17篇
  2015年   25篇
  2014年   21篇
  2013年   66篇
  2012年   31篇
  2011年   20篇
  2010年   28篇
  2009年   34篇
  2008年   31篇
  2007年   27篇
  2006年   25篇
  2005年   33篇
  2004年   16篇
  2003年   15篇
  2002年   17篇
  2001年   16篇
  2000年   14篇
  1999年   15篇
  1998年   18篇
  1997年   4篇
  1996年   7篇
  1995年   7篇
  1994年   4篇
  1993年   6篇
  1992年   6篇
  1990年   4篇
  1989年   5篇
  1988年   1篇
  1987年   4篇
  1986年   1篇
  1982年   1篇
排序方式: 共有609条查询结果,搜索用时 15 毫秒
1.
姜杰  汪景琇 《天文学进展》2005,23(2):121-134
太阳发电机理论主要解释太阳磁场的起源和演化,是太阳物理中最基本、最重要的问题之一.对它的研究不仅具有重要的科学价值,而且对空间天气的预测和空间技术的发展有一定的影响.随着日震学的发展,该理论也得到了很大改进。从相关观测入手,综述了发电机理论需解释的观测事实,以及为发电机理论提供约束的太阳内部动力学结构;介绍了基本理论和近来的主流模型,并指出尚待解决的问题和进一步的努力方向。  相似文献   
2.
We consider the evolution of certain low-mass binaries, incorporating models of (a) internal evolution, (b) tidal friction, (c) dynamo activity driven by an elementary α,Ω dynamo, (d) stellar wind driven by the activity, and (e) magnetic braking as a consequence of wind and poloidal dynamo-generated magnetic field. In some circumstances the stellar wind is found to remove mass on a nuclear timescale, as is necessary to explain some observed systems. We can hope that various uncertainties in the model may be clarified by a careful comparison of the models with such observed quantities as rotation periods. These are modified by processes (a), (b) and (e). Assuming that stellar evolution is slow, rotation rate should in some circumstances represent a balance between magnetic braking trying to slow the star down and tidal friction trying to spin it up. Preliminary attempts are promising, but indicate that some fine tuning is necessary. When there is a third body present, in an orbit which is inclined but not necessarily of short period, the eccentricity of a close binary can be strongly modified by ‘Kozai cycles’. We show that this may complicate attempts to account for spin rates of stars in close binaries.  相似文献   
3.
CygX—1硬态高能光子的时延   总被引:1,自引:1,他引:0  
屈进禄  李惕碚 《天文学报》2001,42(2):140-147
硬X射线和软射线光子的时延时研究主能辐射的一个重要方面,傅里叶交叉谱常常被用于教育处硬软光子之间的时延,但是交叉说示能在高于30Hz的傅里叶频率上从CygX-1测量到有统计意义的快速光变,由李惕培在时域上发展的交叉相关函方法能有效测量不同时间尺度上的时延,利用此交叉相关分析方法,讨论了不同观测时期CygX-1硬态高能光子时延 的性质,分析结果表明,CygX-1硬态在短的尺度(<0.1秒)上存存在有意义的时间延迟,并将短时间尺度上的观测结果和各种CygX-1硬态模型进行了比较讨论。  相似文献   
4.
珠江口河流输沙、河口沉积与粒度信息之间的联系   总被引:2,自引:0,他引:2  
河口三角洲地区泥沙供应充分,是现代沉积速率较高的区域。快速沉积的泥沙包含高分辨率的环境信息。采用放射性同位素测年方法研究了珠江口伶仃洋大铲湾海域6个柱样的现代沉积速率,以2mm的间隔分析了其中2个柱样上部的粒度,并对其平均粒径和珠江流域的年输沙量进行了快速傅里叶变换,以期获取河流泥沙供应、河口沉积速率和沉积物垂向粒度变化的对应关系。结果表明,大铲湾海域的沉积速率为1~3cm/a,受动力条件和泥沙供应条件的影响显著。2个柱样的平均粒径的最显著重现周期与珠江年输沙量的周期性有较好的对应关系,并可能反映了季节的、年的和多年的沉积速率信息。对于每年沉积厚度在厘米级的环境,以毫米级的高分辨率进行粒度分析,有可能揭示出沉积物供应的季节变化和年际变化。本研究亦可为其他河口的相关工作提供借鉴。  相似文献   
5.
The analytical method (AM) for separation of composite waves is presented based on the Hilbert transform. It is ap-plicable to both regular and irregular trains of waves. The wave data series measured with two wave gauges in the experi-ments are separated into two series of incident and reflected waves. Then, the reflection coefficient can be easily ob-tained. The arrival of reflected waves can also be detected for improveraent of the accuracy of the reflection coefficient. The reflection performance of the physical model can be estimated exactly without calculation of wave height and phase difference. Numerical samples developed to test the method are proved to be accurate. Physical experiments are conduct-ed and compared with Goda s method and satisfactory results are obtained.  相似文献   
6.
An iterative algorithm to calculate mutual correlation using hierarchical key points and the search space mark principle is proposed. An effective algorithm is designed to improve the matching speed. By hierarchical key point algorithm and mutual correlation coefficients of the matching images, the important points can be iteratively calculated in the images hierarchically, and the correlation coefficient can be obtained with satisfactory precision. Massive spots in the parameter space which are impossible to match can be removed by the search space mark principle. Two approximate continuities in the correlation image matching process, the image gray level distribution continuity and the correlation coefficient value in the parameter space continuity, are considered in the method. The experiments show that the new algorithm can greatly enhance matching speed and achieve accurate matching results.  相似文献   
7.
RUSLE及其影响因子的快速计算分析   总被引:4,自引:0,他引:4  
RUSLE是目前应用最广泛的土壤侵蚀模型。虽然是一种经验模型,但是其影响因子计算仍然非常复杂,满足不了区域土壤侵蚀的快速提取要求。针对这种状况,文章在介绍RUSLE手册中每个影响因子计算方式基础上,分析总结了可进行快速计算的方法,实验表明,采用文章推荐的因子计算方式,可达到快速有效的目的。  相似文献   
8.
We investigate the global evolution of a turbulent protoplanetary disk incorporating the effects of Maxwell stress due to a large-scale magnetic field permeating the disk. A magnetic field is produced continuously by an dynamo and the resultant Maxwell stress assists the viscous stress in p roviding the means for disk evolution. The most striking feature of magnetized disk evolution is the presence of the surface density bulge located in the magnetic gap, the region of the disk where the degree of ionization is too low to allow for coupli ng between the magnetic field and the gas. The bulge persists for a time of the order of 105–106 yr. The presence and persistence of the surface density bulge may have important implications for the process of planet formation and the overall characteristics of resultant planetary systems.Operated by USRA under contract No. NASW-4574 with NASA.  相似文献   
9.
本文通过对1982年磁扰期间琼中、北京两站地磁X分量变化的分析,证实了磁层-电离层电动耦合对中纬电离层电流的影响.分析发现:磁静、磁扰条件下的平均日变化中,两站X分量变化在白天有反向的趋势.这表明它们分处于与动力效应对应的电离层发电机电流圈中心之南北两侧.在磁暴主相期间,X分量变化形态与之明显不同,两站地磁南北分量有同向变化,且变幅相近,甚至有时北京站△X更大.对环电流能量增长指数R小于-25nT/h的21次事件所作的时序叠加分析(以R最负时为零时)进一步证明,这种同向变化是普遍存在的.两站零时之△X大小相近,相关系数高达0.98.该同向变化与R指数突然变负密切相关. 以上对比表明,与发电机电流造成两站X分量反向变化不同,同向变化是磁层源高纬扰动电流向中低纬直接穿透的结果.本文对动力和电动耦合两种过程的不同进行了初步讨论.  相似文献   
10.
Spectral simulation has gained application in building geologic models due to the advantage of better honoring the spatial continuity of petrophysical properties, such as reservoir porosity and shale volume. Distinct from sequential simulation methods, spectral simulation is a global algorithm in the sense that a global density spectrum is calculated once and the inverse Fourier transform is performed on the Fourier coefficient also only once to generate a simulation realization. The generated realizations honor the spatial continuity structure globally over the whole field instead of only within a search neighborhood, as with sequential simulation algorithms. However, the disadvantage of global spectral simulation is that it traditionally cannot account for the local information such as the local continuity trends, which are often observed in reservoirs and hence are important to be accounted for in geologic models. This disadvantage has limited wider application of spectral simulation in building geologic models. In this paper, we present ways of conditioning geologic models to the relevant local information. To account for the local continuity trends, we first scale different frequency components of the original model with local-amplitude spectrum ratios that are specific to the local trend. The sum of these scaled frequency components renders a new model that displays the desired local continuity trend. The implementation details of this new method are discussed and examples are provided to illustrate the algorithm.  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