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   14674篇
  免费   3063篇
  国内免费   3995篇
测绘学   1396篇
大气科学   3182篇
地球物理   3578篇
地质学   7524篇
海洋学   2136篇
天文学   485篇
综合类   1473篇
自然地理   1958篇
  2024年   60篇
  2023年   245篇
  2022年   708篇
  2021年   807篇
  2020年   667篇
  2019年   778篇
  2018年   845篇
  2017年   791篇
  2016年   892篇
  2015年   802篇
  2014年   923篇
  2013年   1048篇
  2012年   1010篇
  2011年   1020篇
  2010年   1020篇
  2009年   960篇
  2008年   944篇
  2007年   889篇
  2006年   731篇
  2005年   656篇
  2004年   529篇
  2003年   500篇
  2002年   585篇
  2001年   584篇
  2000年   481篇
  1999年   529篇
  1998年   416篇
  1997年   378篇
  1996年   330篇
  1995年   304篇
  1994年   256篇
  1993年   223篇
  1992年   182篇
  1991年   125篇
  1990年   103篇
  1989年   97篇
  1988年   71篇
  1987年   46篇
  1986年   30篇
  1985年   36篇
  1984年   21篇
  1983年   25篇
  1982年   13篇
  1981年   16篇
  1980年   9篇
  1979年   11篇
  1978年   10篇
  1977年   5篇
  1958年   12篇
  1957年   4篇
排序方式: 共有10000条查询结果,搜索用时 31 毫秒
11.
ABSTRACT

High performance computing is required for fast geoprocessing of geospatial big data. Using spatial domains to represent computational intensity (CIT) and domain decomposition for parallelism are prominent strategies when designing parallel geoprocessing applications. Traditional domain decomposition is limited in evaluating the computational intensity, which often results in load imbalance and poor parallel performance. From the data science perspective, machine learning from Artificial Intelligence (AI) shows promise for better CIT evaluation. This paper proposes a machine learning approach for predicting computational intensity, followed by an optimized domain decomposition, which divides the spatial domain into balanced subdivisions based on the predicted CIT to achieve better parallel performance. The approach provides a reference framework on how various machine learning methods including feature selection and model training can be used in predicting computational intensity and optimizing parallel geoprocessing against different cases. Some comparative experiments between the approach and traditional methods were performed using the two cases, DEM generation from point clouds and spatial intersection on vector data. The results not only demonstrate the advantage of the approach, but also provide hints on how traditional GIS computation can be improved by the AI machine learning.  相似文献   
12.
创新型企业作为塑造创新地理格局的重要力量,其区位选择的外部特征及内在机理亟须予以系统化研究。基于对安徽省创新型企业的细分行业与空间建库,采用核密度估计和地理探测器等方法,对细分行业下的创新型企业空间集聚特征及影响因素进行研究。结果表明:(1)安徽省创新型企业类型以先进制造和自动化为主,并以生物与新医药、新材料、电子信息为辅;(2)创新型企业空间集聚的不均衡特征显著,呈现出“一核一带多节点”的集聚分布特征,且合肥、芜湖是两个重要集聚区;不同细分行业视角下创新型企业的空间分布形态各异,可归纳为点-轴式、极核式、双核式及多核分散式等4种空间组织形态。(3)创新型因子对于创新型企业的空间集聚最为重要,但传统型和政策型因子的重要性仍不容忽视。其中,产业基础、人力资本、创新投入是最核心的因素,但各行业创新型企业的影响因素作用力则表现出一定的异质性。  相似文献   
13.
以FeCl3?6H2O、NiCl2?6H2O、MgCl2?6H2O为原料,以NaOH为沉淀剂采用水热法合成了镁镍铁水滑石 (MgNiFe-LDH),通过X射线衍射 (XRD)、傅里叶变换红外光谱 (FTIR) 和扫描电镜 (SEM) 分析了MgNiFe-LDH结构及形貌,探讨了不同陈化时间和水热温度对MgNiFe-LDH合成的影响。将制得的MgNiFe-LDH添加至聚丙烯 (PP) 中,制备MgNiFe-LDH/PP复合材料,通过对材料的加速老化测其力学性能,研究了添加MgNiFe-LDH前后材料力学性能的差异。研究结果表明,当Mg2+:Ni2+:Fe3+=2:1:1,反应温度为140℃、陈化时间为24 h时,合成的MgNiFe-LDH为片状,形貌较为规整,颗粒粒径约为2μm;经加速老化后,填充MgNiFe-LDH 复合材料的抗老化性能优于纯PP,当MgNiFe-LDH的填充量为6 wt% 复合材料拉伸强度不变,可明显提高PP的抗老化性能。  相似文献   
14.
1 Introduction The Qinghai-Tibet Plateau, known as the highest plateau with the most complex topography in the world, covers an area of more than 200km2, with a mean elevation of more than 4000m a.s.l. (Ye and Gao, 1979). Surrounded by the Earth’s highest mountains, such as the Himalayas, Pamir, Kunlun Mountains, the plateau plays a significant role in climate change in China even in the world, thus attracted great attention of researchers. Up to now, many achievements have been gained by…  相似文献   
15.
Using the decimetric (700–1500 MHz) radio spectrometer and the synchronous observational system with high temporal resolution at four frequencies (1420, 2130, 2840 and 4260 MHz) of Yunnan Observatory, two rare events were observed on 2001 June 24 and 1990 July 30. The former was a small radio burst exhibiting pulsations with short periods (about 29, 40 and 100 ms) in the impulsive phase. The latter was a large radio burst, which at 2840 MHz produced radio pulsations with period of about 30 ms. This paper focuses on pulsations with very short periods in the range of 29–40 ms. The mechanism of generation of such pulsations may be modulation of radio radiation by the periodic trains of whistler packets originating in unstable regions of the corona. Alternatively, these pulsations can be attributed to wave-wave non-linear interactions of electrostatic upper hybrid waves driven by beams of precipitating electrons in flaring loops.  相似文献   
16.
定性分析协方差方法及其改进型在AR(P)参数估计中的应用,提供了一种估计参数的计算机上机流程图,比较了协方差方法及其改进型谱估计结果。  相似文献   
17.
讲述了同步广播卫星电视时间信号的测量方法和测量结果,获得了CCTV1、CCTV2通过同一颗卫星(亚太-1A)转播的时延差值为16333μs,测量精度在10ns以内;CCTV2、CCTV4分别经两颗卫星(亚太-1A、亚洲-Ⅱ)转播,在陕西天文台卫星地面接收站时延差值为1644.20μs,精度为50μs,并分析了影响时延差值和精度的原因。同时测量了地方电视台转播亚太-1A的CCTV信号与直接接收亚太-1A的CCTV信号的时延差值,其测量精度为0.1μs。这些结果为利用同步广播卫星的电视信号进行高精度的时间服务提供了参考依据。  相似文献   
18.
Spencer  John  Buie  Marc  Young  Leslie  Guo  Yanping  Stern  Alan 《Earth, Moon, and Planets》2003,92(1-4):483-491
Development of the New Horizons mission to Pluto and the Kuiper Belt is now fully funded by NASA (Stern and Spencer, this volume). If all goes well, New Horizons will be launched in January 2006, followed by a Jupiter gravity assist in 2007, with Pluto arrival expected in either 2015 or 2016, depending on the launch vehicle chosen. A backup launch date of early 2007, without a Jupiter flyby, would give a Pluto arrival in 2019 or 2020. In either case, a flyby of at least one Kuiper Belt object (KBO) is planned following the Pluto encounter, sometime before the spacecraft reaches a heliocentric distance of 50 AU, in 2021 or 2023 for the 2006 launch, and 2027 or 2029 for the 2007 launch. However, none of the almost 1000 currently-known KBOs will pass close enough to the spacecraft trajectory to be targeted by New Horizons, so the KBO flyby depends on finding a suitable target among the estimated 500,000 KBOs larger than 40 km in diameter. This paper discusses the issues involved in finding one or more KBO targets for New Horizons. The New Horizons team plans its own searches for mission KBOs but will welcome other U.S, or international team who wish to become involved in exchange for mission participation at the KBO.  相似文献   
19.
CARBON DYNAMICS OF WETLAND IN THE SANJIANG PLAIN   总被引:2,自引:0,他引:2  
1INTRODUCTIONWetlandsplayanimportant roleintheprocessofcar-bonstorage.Thetotalcarbonstoredindifferentkindsofwetlandsisabout15%-35%ofthetotalcarboninthegloballandsoils(POSTetal.,1982;GORHAM,1991).Inaddition,wetlandsaresignificantnaturalsources fortheatmospheric CH4 (MOORE,1994).It isestimatedthatabout110×1012gCH4 originates fromanaerobicdecompositioninthenaturalwetlands,CH4 emission fromthenaturalwetlandsis15%-30%oftheglobalCH4 emission andtheCH4 emission from thepeat land at hi…  相似文献   
20.
Wang  M.  Xie  R.X.  Duan  C.C.  Yan  Y.H.  Sych  R.A.  Altyntsev  A.T. 《Solar physics》2003,212(2):407-424
A type IV radio burst accompanied by several normal- and reverse-drifting type III bursts, multiple long-term quasi-periodic pulsations and spikes was observed with the radio spectrometers (1.0–2.0 and 2.6–3.8 GHz) at National Astronomical Observatories of China (NAOC) on 23 September 1998. In combination with the images of Siberian Solar Radio Telescope (SSRT) of Russia, the complex and multiple magnetic structures inferred from the radio bursts reveal the existence of both large-scale and small-scale magnetic structures. This event suggests that the geometries of coronal magnetic fields contain multiple discrete electron acceleration/injection sites at different heights, and extended open and closed magnetic field lines. It can be shown that the energetic electrons gain access to open, diverging and closed field lines thus producing different types of radio bursts. From the characteristics of position, polarization, dispersion and displacement of the sources, the model of the type IV event is supported, which involves synchrotron emission from the electrons confined by the rapid scattering through the interaction of hydromagnetic wave with particles.  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