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   4620篇
  免费   747篇
  国内免费   815篇
测绘学   825篇
大气科学   399篇
地球物理   1155篇
地质学   1495篇
海洋学   582篇
天文学   1029篇
综合类   309篇
自然地理   388篇
  2024年   19篇
  2023年   50篇
  2022年   132篇
  2021年   152篇
  2020年   183篇
  2019年   236篇
  2018年   162篇
  2017年   192篇
  2016年   239篇
  2015年   253篇
  2014年   279篇
  2013年   298篇
  2012年   260篇
  2011年   273篇
  2010年   224篇
  2009年   336篇
  2008年   286篇
  2007年   374篇
  2006年   329篇
  2005年   257篇
  2004年   244篇
  2003年   224篇
  2002年   166篇
  2001年   177篇
  2000年   135篇
  1999年   134篇
  1998年   129篇
  1997年   63篇
  1996年   79篇
  1995年   37篇
  1994年   47篇
  1993年   55篇
  1992年   36篇
  1991年   29篇
  1990年   26篇
  1989年   17篇
  1988年   12篇
  1987年   10篇
  1986年   9篇
  1985年   5篇
  1984年   2篇
  1983年   2篇
  1982年   2篇
  1981年   2篇
  1980年   3篇
  1977年   1篇
  1954年   2篇
排序方式: 共有6182条查询结果,搜索用时 234 毫秒
1.
New Earth observation missions and technologies are delivering large amounts of data. Processing this data requires developing and evaluating novel dimensionality reduction approaches to identify the most informative features for classification and regression tasks. Here we present an exhaustive evaluation of Guided Regularized Random Forest (GRRF), a feature selection method based on Random Forest. GRRF does not require fixing a priori the number of features to be selected or setting a threshold of the feature importance. Moreover, the use of regularization ensures that features selected by GRRF are non-redundant and representative. Our experiments based on various kinds of remote sensing images, show that GRRF selected features provides similar results to those obtained when using all the available features. However, the comparison between GRRF and standard random forest features shows substantial differences: in classification, the mean overall accuracy increases by almost 6% and, in regression, the decrease in RMSE almost reaches 2%. These results demonstrate the potential of GRRF for remote sensing image classification and regression. Especially in the context of increasingly large geodatabases that challenge the application of traditional methods.  相似文献   
2.
3.
4.
We present the preliminary results of a study of how small stellar systems merge to form larger ones. As we display the families of galaxies in the μe - Re plane (effective surface brightness versus effective radius) we realize that different morphological types occupy different loci, evidencing the different physical mechanisms operating in each family. As proposed by Capaccioli et al. (1992) this diagram is the logical equivalent of the HR diagram for stars. Here we take some initial steps in understanding of how we can establish the evolutionary tracks, solely due to dynamical processes, in the μe - Re plane, ultimately making a dwarf elliptical to turn into a normal elliptical galaxy. This revised version was published online in August 2006 with corrections to the Cover Date.  相似文献   
5.
1 Introduction Inrecentyearstherehasbeengrowingresearchin terestinthetwo dimensional (2 D )systemtheory .The 2 Dsystemsmayfindapplicationsinareassuchasmarineseismicdataprocessingandimageprocessing .Althoughmoreandmorevaluableresultshavebeengained ,mos…  相似文献   
6.
王晓彬  张西亮 《天文学报》2006,47(2):202-211
小行星自转参数的资料不仅可以为小行星碰撞演化提供数据,还可以为太阳系的演化研究提供依据.利用云南天文台1米望远镜对主带碳类小行星(360)Carlova进行了新的CCD测光观测,结合前人的测光资料,利用Epoch-方法对(360)的自转参数进行了反演计算,得到该小行星自转的恒星周期为0.25780417±0.00000003天,自转轴的黄道坐标为(95°±3,°40°±1°).新的结果与前人的结果相比较为一致,其精度稍高于以前的估算结果.  相似文献   
7.
8.
9.
The star WR 7a, also known as SPH 2, has a spectrum that resembles that of V Sagittae stars although no O  vi emission has been reported. The Temporal Variance Spectrum – TVS – analysis of our data shows weak but strongly variable emission of O  vi lines which is below the noise level in the intensity spectrum.
Contrary to what is seen in V Sagittae stars, optical photometric monitoring shows very little, if any, flickering. We found evidence of periodic variability. The most likely photometric period is   P phot= 0.227(±14) d  , while radial velocities suggest a period of   P spec= 0.204(±13) d  . One-day aliases of these periods can not be ruled out. We call attention to similarities with HD 45166 and DI Cru (= WR 46), where multiple periods are present. They may be associated to the binary motion or to non-radial oscillations.
In contrast to a previous conclusion by Pereira et al., we show that WR 7a contains hydrogen. The spectrum of the primary star seems to be detectable as the N  v 4604 Å  absorption line is visible. If so, it means that the wind is optically thin in the continuum and that it is likely to be a helium main sequence star.
Given the similarity to HD 45166, we suggests that WR 7a may be a qWR – quasi Wolf–Rayet – star. Its classification is WN4h/CE in the Smith, Shara & Moffat three-dimensional classification system.  相似文献   
10.
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