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   411886篇
  免费   4321篇
  国内免费   1099篇
化学   204807篇
晶体学   5929篇
力学   19441篇
综合类   7篇
数学   59532篇
物理学   127590篇
  2020年   1988篇
  2019年   1970篇
  2018年   10978篇
  2017年   11855篇
  2016年   7916篇
  2015年   4159篇
  2014年   4569篇
  2013年   14127篇
  2012年   15052篇
  2011年   25653篇
  2010年   15534篇
  2009年   15465篇
  2008年   22773篇
  2007年   26313篇
  2006年   12413篇
  2005年   18293篇
  2004年   13603篇
  2003年   12200篇
  2002年   10072篇
  2001年   10284篇
  2000年   7997篇
  1999年   6157篇
  1998年   4945篇
  1997年   4752篇
  1996年   4923篇
  1995年   4458篇
  1994年   4196篇
  1993年   4011篇
  1992年   4504篇
  1991年   4367篇
  1990年   4079篇
  1989年   3906篇
  1988年   4203篇
  1987年   3868篇
  1986年   3751篇
  1985年   5407篇
  1984年   5491篇
  1983年   4453篇
  1982年   4827篇
  1981年   4870篇
  1980年   4623篇
  1979年   4760篇
  1978年   4766篇
  1977年   4676篇
  1976年   4657篇
  1975年   4558篇
  1974年   4402篇
  1973年   4605篇
  1972年   2595篇
  1971年   1898篇
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
181.
182.
183.
We consider the growth of a spherical crystal in a supersaturatedsolution. In the first part, existence and uniqueness resultsfor radially symmetric growth are obtained, provided that thesupersaturation is not too large; conversely, when the far-fieldsupersaturation exceeds a critical value, it is shown that theradially symmetric solution ceases to exist in finite time.In the second part, we examine the linear stability of a radiallysymmetric similarity solution (in which the radius grows ast?) to shape perturbations. The results are compared with previousquasi-static analyses, and, in particular, the critical radiusat which the crystal becomes unstable is found to be largerfor small supersaturations, but smaller for large supersaturations,than those predicted by the quasi-static analysis  相似文献   
184.
185.
We report morphologic changes of metallic surfaces at the onset of ablation, starting from gentle ablation to the emergence of ablation craters. The evolution of both observed melting zones and of ablation craters therein are investigated in dependence of the ablation laser fluence for nanosecond ultraviolet laser pulses. Further, consequences of crater formation for cluster synthesis within the released atomic vapor are pointed out. PACS 52.38.Mf; 79.20.Ds; 65.40.De  相似文献   
186.
We show that every composition operator which is an isometry of the Dirichlet space is induced by a univalent full map of the disk into itself that fixes the origin. This is an analogue of the Hardy space result for inner functions due to Nordgren. The proof relies on the Stone-Weierstrass theorem and the Riesz representation theorem.

  相似文献   

187.
Abstract Under a suitable ellipticity condition, we show that classical SG-pseudodifferential operators of nonnegative order possess complex powers. We show that the powers are again classical and derive an explicit formula for all homogeneous components. Keywords: Complex power, Weighted symbols, Noncompact manifolds  相似文献   
188.
The interferometric intensity patterns from a 2D shearing interferometer are shown and discussed. The intensity patterns can be obtained in two different approaches incorporating differential and extended wavefront controlled displacements. The reliable directional sensitivity of this interferometer allows the optimization of the measurement parameters to estimate the wavefront of the intensity patterns by regularization techniques.  相似文献   
189.
Well-Posedness by Perturbations of Variational Problems   总被引:3,自引:0,他引:3  
In this paper, we consider the extension of the notion of well-posedness by perturbations, introduced by Zolezzi for optimization problems, to other related variational problems like inclusion problems and fixed-point problems. Then, we study the conditions under which there is equivalence of the well-posedness in the above sense between different problems. Relations with the so-called diagonal well-posedness are also given. Finally, an application to staircase iteration methods is presented.  相似文献   
190.
The mass power spectrum for a Universe dominated by the Chaplygin gas is evaluated numerically from scales of the order of the Hubble horizon to 100 Mpc. The results are compared with a pure baryonic Universe and a cosmological constant model. In all three cases, the spectrum increases with k, the wavenumber of the perturbations. The slope of the spectrum is higher for the baryonic model and smaller for the cosmological constant model, the Chaplygin gas interpolating these two models. The results are analyzed in terms of the sound velocity of the Chaplygin gas and the moment the Universe begins to accelerate.  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