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   67010篇
  免费   10415篇
  国内免费   14341篇
测绘学   7853篇
大气科学   6362篇
地球物理   12164篇
地质学   37423篇
海洋学   10416篇
天文学   7197篇
综合类   3302篇
自然地理   7049篇
  2024年   290篇
  2023年   952篇
  2022年   2685篇
  2021年   3416篇
  2020年   2811篇
  2019年   3226篇
  2018年   3518篇
  2017年   3328篇
  2016年   3357篇
  2015年   3369篇
  2014年   3778篇
  2013年   5047篇
  2012年   4786篇
  2011年   5079篇
  2010年   4789篇
  2009年   4866篇
  2008年   4702篇
  2007年   4580篇
  2006年   4415篇
  2005年   3397篇
  2004年   2684篇
  2003年   1995篇
  2002年   2114篇
  2001年   1859篇
  2000年   1561篇
  1999年   845篇
  1998年   629篇
  1997年   556篇
  1996年   469篇
  1995年   383篇
  1994年   399篇
  1993年   312篇
  1992年   335篇
  1991年   296篇
  1990年   353篇
  1989年   228篇
  1988年   228篇
  1987年   274篇
  1986年   226篇
  1985年   323篇
  1984年   290篇
  1983年   268篇
  1982年   282篇
  1981年   207篇
  1980年   244篇
  1979年   211篇
  1978年   211篇
  1977年   168篇
  1975年   174篇
  1973年   166篇
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
71.
基于 SRP 概念模型的祁连山地区生态脆弱性评价   总被引:1,自引:0,他引:1       下载免费PDF全文
基于生态敏感性-生态恢复力-生态压力度(SRP)概念模型,从地形、气候、植被和社会经济 因子选取 8 个评价指标,利用遥感和 GIS 技术,采用主成分分析方法求取权重,对祁连山地区启动 水源涵养区生态环境保护和综合治理规划研究前后近 10 a 的生态脆弱性程度进行系统、定量地评 估,旨在揭示生态脆弱性的分布特征、时空演变及动因,为区域生态保护、资源利用和可持续发展 提供参考。结果表明:(1)从研究区生态脆弱性分布来看,祁连山地区主要以轻度和重度脆弱为 主,脆弱性程度从西北向东南地区逐渐减弱,西北地区植被覆盖度小,海拔高,生态环境较为恶劣 是导致脆弱性程度较高的原因;(2)祁连山地区 3 期生态脆弱程度呈逐渐下降趋势,综合指数分别 为 3.307、3.118 和 3.103;2005 年 生 态 脆 弱 性 较 高 ,极 度 脆 弱 面 积 为 28 610 km2,2010 年 下 降 为 11 723 km2,2015 年降低为 6 174 km2,极度脆弱面积逐渐减少;(3)从祁连山地区生态脆弱性演变动 因来看,8 个指标对生态脆弱性影响均较为显著,但在不同的时间影响程度各不相同,2005—2015 年 3 期数据中对生态脆弱性影响最大的均为植被指数,降水次之,地形因子影响最小。总体来看, 近年来祁连山地区生态脆弱性程度有所降低,但仍然需要加强保护力度,促进生态环境可持续 发展。  相似文献   
72.
Abstract— Active capture is a new process for the incorporation of large quantities of heavy noble gases into growing surfaces. Adsorption in the conventional sense involves surface bonding by polarization (Van der Waals forces). What is referred to as “anomalous adsorption” of heavy noble gases involves chemical bonds and can occur when other (more chemically active) species are not available to preempt sites with unfilled bonds. Anomalous adsorption has been observed under conditions of fracture, vacuum deposition and ionizing radiation. Active capture depends upon anomalous adsorption to retain noble gases on a surface long enough to be captured in a growing surface film as it is deposited. The fundamental principle may be the impingement onto the growing film with sufficient energy to liberate surface electrons (work function energy of a few electronvolts) so that they are retained by anomalous adsorption long enough to be entrapped in the growing surface. Trapping efficiencies of ?1% have been observed for Kr and Xe in laboratory experiments, implying a fundamentally new mechanism for the incorporation of heavy noble gases onto surfaces. It may play a role in explaining the large concentrations of planetary noble gases contained in phase‐Q.  相似文献   
73.
74.
The magnetic-field distribution outside a flat, infinitely conductive unbounded disk in the field of a point magnetic dipole is determined. A relationship is established between the problem of magnetic-field determination and the problem of the flow of an ideal incompressible fluid around an infinitely thin disk.  相似文献   
75.
In the atmospheric Čerenkov technique γ-rays are detected against the abundant background produced by hadronic showers. In order to improve the signal to noise ratio of theexperiment, it is necessary to reject a significant fraction of hadronic showers. Traditional background rejection methods based on image shape parameters have been extensively used for the data from imaging telescopes. However, non-imaging Čerenkov telescopes have to develop very different means of statistically identifying and removing cosmic ray events. Some of the parameters, which could be potentially important for non-imaging arrays, are the temporal and spectral differences, the lateral distributions and density fluctuations of Čerenkov photons generated by γ-ray and hadron primaries. Here we study the differences in fluctuations of Čerenkov photon density in the light pool at the observation level from showers initiated by photons and those initiated by protons or heavier nuclei. The database of simulated events for the PACT array has been used to evaluate the efficiency of the new technique. Various types of density fluctuations like the short range and medium range fluctuations as well as flatness parameter are studied. The estimated quality factors reflect the efficiencies with which the hadrons can be rejected from the data. Since some of these parameters are independent, the cuts may be applied in tandem and we demonstrate that the proton rejection efficiency of ∼90% can be achieved. Use of density fluctuations is particularly suited for wavefront sampling observations and it seems to be a good technique to improve the signal to noise ratio. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   
76.
中国1∶100万景观生态制图设计   总被引:5,自引:0,他引:5  
中国1∶100万景观生态图系借鉴国内外传统景观制图方法和制图规范,在遥感、地理信息系统先进技术的支持下,设计研制其制图方法、制图内容、样图和技术流程,同时提出初步的景观分类系统,为今后编制中国1∶100万景观生态图奠定基础。  相似文献   
77.
The explicit forms of the metric as well as the equations of motion in the first-order post-Newtonian approximation are worked out under several gauge conditions. It is noted that the so-called EIH (Einstein, Infeld, and Hoffman) equation of motion for an assembly ofN finite mass points mutually interacting via gravitation is identically obtained under three different gauge conditions, namely the harmonic gauge, Chandrasekhar gauge and a composite Chandrasekhar gauge used by Misneret al. (1970), even though the solutions for the metric are found to be all different. In one case the metric has a component apparently diverging, but finally generates regular affine connections so that the equations of motions become free from any singularity. By use of the Chandrasekhar gauge and his formulation, the second-order contribution to the acceleration of planets in the limit of test particle motion around the Sun has been calculated, the inclusion of which in the EIH set of the equations of motion would extend the relative accuracy of computing the total acceleration of any planet to better than one part in 1017.  相似文献   
78.
In astronomical photometry, the sensitivity of observations is limited by the dark counts of the photomultiplier tube. In the present work, the effect of dark count noise in photon counting systems is investigated by theory and experimental measurements. Dark counts are considered to be originating from two sources, namely: dc fluctuations and random pulses.Experimental measurements were carried out to determine noise effects in different operating regions of noise dominance. The results provide strong evidence that: in normal operating mode, where the effect of random pulses is dominant, dark counts do not follow Poisson statistics. The observed noise shows strong (1/f) power spectrum, where the observed noise power is found to increase with time of observation.The results are important in photon counting systems operating under dark count limited mode. The conclusions drawn can be useful in obtaining more accurate error estimates and in assessing astronomical photometric observations and data reduction techniques.  相似文献   
79.
80.
莱州湾南岸潍河下游地区咸水入侵灾害成因及特征   总被引:8,自引:1,他引:7  
通过对莱州湾南岸咸水入侵较严重地潍河下游地区晚更新世以来沉积特征及现代自然环境条件变化的分析,探讨了沉积相对咸水入侵产生及空间范围特征的环境机理。晚更新世以来的三次海平面升降变化造成了潍河下游地区海陆沉积环境交替,形成了巨厚的海陆交互相沉积层。海进时期,大面积的滨海平原被淹没,在近海平原洼地滞留的海水经过蒸发、浓缩变为卤水,成为咸水入侵的物源;海退后陆源碎屑在滨海地区沉积形成了巨厚的古河道砂层。20世纪70年代末期以来,随着对地下淡水的过度开采,淡咸水水头压力差减小.卤水通过古河道砂层快速南侵。通过对潍河下游地区100余个地质钻孔水化学连续监测资料分析,阐明了咸水入侵的特征,有针对性地提出了咸水入侵的防治措施。  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