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   330159篇
  免费   3053篇
  国内免费   937篇
化学   164959篇
晶体学   5374篇
力学   15534篇
综合类   7篇
数学   38483篇
物理学   109792篇
  2021年   3139篇
  2020年   3340篇
  2019年   3771篇
  2018年   5210篇
  2017年   5455篇
  2016年   7381篇
  2015年   4149篇
  2014年   7041篇
  2013年   15922篇
  2012年   12384篇
  2011年   14837篇
  2010年   11027篇
  2009年   10927篇
  2008年   13248篇
  2007年   13212篇
  2006年   12150篇
  2005年   10530篇
  2004年   9843篇
  2003年   8686篇
  2002年   8677篇
  2001年   10395篇
  2000年   7656篇
  1999年   5968篇
  1998年   4973篇
  1997年   4812篇
  1996年   4479篇
  1995年   3866篇
  1994年   3820篇
  1993年   3701篇
  1992年   4096篇
  1991年   4307篇
  1990年   4097篇
  1989年   4008篇
  1988年   3779篇
  1987年   3917篇
  1986年   3683篇
  1985年   4629篇
  1984年   4681篇
  1983年   3885篇
  1982年   3973篇
  1981年   3699篇
  1980年   3647篇
  1979年   3913篇
  1978年   3902篇
  1977年   3906篇
  1976年   3879篇
  1975年   3675篇
  1974年   3615篇
  1973年   3650篇
  1972年   2603篇
排序方式: 共有10000条查询结果,搜索用时 0 毫秒
181.
The sorption of carbon dioxide in glassy Poly(lactic acid) (PLA) films was studied by quartz crystal microbalance (QCM) at high pressures. Two thermal treatments, melted and quenched, were performed in PLA with two different L:D contents, 80:20 and 98:2, films and compared with a third thermal protocol, annealed, and used in a previous work. The results obtained show that for pressures higher than 2 MPa, the carbon dioxide solubility is larger in PLA 80:20 than in PLA 98:2, indicating that the L:D plays a dominant role on this property. The thermal treatments only affect the gas solubility in PLA 98:2. Sorption isotherms at temperatures 303, 313, and 323 K, below the glass transition temperature of the polymer, and pressures up to 5 MPa were measured and analyzed with three different models, the dual‐mode sorption model, the Flory–Huggins equation, and a modified dual‐mode sorption model where the Henry's law term was substituted by the Flory–Huggins equation. This last model performs especially well for CO2 in PLA 80:20, due to the convex upward curvature of the solubility isotherms for that system. © 2007 Wiley Periodicals, Inc. J Polym Sci Part B: Polym Phys 45: 616–625, 2007  相似文献   
182.
183.
The behavior of the intensity of anomalous and galactic cosmic rays in the outer heliosphere is compared. The previous hypothesis, according to which the lowest energy galactic cosmic rays affected by large-scale electric fields far beyond the termination shock wave of the solar wind may contribute to the behavior of the anomalous component intensity, is analyzed.  相似文献   
184.
185.
186.
187.
This article studies some geometrical aspects of the semidefinite linear complementarity problem (SDLCP), which can be viewed as a generalization of the well-known linear complementarity problem (LCP). SDLCP is a special case of a complementarity problem over a closed convex cone, where the cone considered is the closed convex cone of positive semidefinite matrices. It arises naturally in the unified formulation of a pair of primal-dual semidefinite programming problems. In this article, we introduce the notion of complementary cones in the semidefinite setting using the faces of the cone of positive semidefinite matrices and show that unlike complementary cones induced by an LCP, semidefinite complementary cones need not be closed. However, under R0-property of the linear transformation, closedness of all the semidefinite complementary cones induced by L is ensured. We also introduce the notion of a principal subtransformation with respect to a face of the cone of positive semidefinite matrices and show that for a self-adjoint linear transformation, strict copositivity is equivalent to strict semimonotonicity of each principal subtransformation. Besides the above, various other solution properties of SDLCP will be interpreted and studied geometrically.  相似文献   
188.
E. J. S. Lage 《Physica A》1987,140(3):629-636
We study critical dynamics of general q-state Potts models on d-dimensional hypercubic lattices. The master equation is formulated according to a theory recently presented by the author. A simple bond moving technique, followed by decimation, is used to obtain the dynamical exponents. Although this approximation yields poor results for the static exponents, the dynamic behaviour is closer to Monte Carlo simulations. We compare our results with those obtained with a different formulation of dynamics. A final discussion is included.  相似文献   
189.
使用美国甚大天线阵(VLA).对Markarian 8星系进行了多频观测.多频VLA观测表明,Markarian 8星系有三个主要的射电子成份,它们浸在一个弥漫的星系包层中.包层的射电谱是陡的非热谱.本文根据VLA观测确定了包层的物理参量,并讨论了包层中相对论性电子的可能起因.本文估计了包层非热辐射所要求的超新星爆发率.  相似文献   
190.
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