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   172816篇
  免费   2376篇
  国内免费   725篇
化学   93052篇
晶体学   2260篇
力学   7676篇
综合类   7篇
数学   18204篇
物理学   54718篇
  2021年   1019篇
  2020年   1153篇
  2019年   1169篇
  2018年   1176篇
  2017年   1201篇
  2016年   2373篇
  2015年   1969篇
  2014年   2547篇
  2013年   7848篇
  2012年   6382篇
  2011年   8077篇
  2010年   4971篇
  2009年   5083篇
  2008年   7444篇
  2007年   7418篇
  2006年   7139篇
  2005年   6665篇
  2004年   5954篇
  2003年   5132篇
  2002年   5031篇
  2001年   6083篇
  2000年   4619篇
  1999年   3501篇
  1998年   2660篇
  1997年   2645篇
  1996年   2630篇
  1995年   2342篇
  1994年   2216篇
  1993年   2076篇
  1992年   2388篇
  1991年   2297篇
  1990年   2016篇
  1989年   1975篇
  1988年   2024篇
  1987年   1937篇
  1986年   1856篇
  1985年   2791篇
  1984年   2759篇
  1983年   2205篇
  1982年   2397篇
  1981年   2287篇
  1980年   2239篇
  1979年   2202篇
  1978年   2267篇
  1977年   2241篇
  1976年   2171篇
  1975年   2142篇
  1974年   2051篇
  1973年   2138篇
  1972年   1203篇
排序方式: 共有10000条查询结果,搜索用时 22 毫秒
101.
102.
Oxidation of the title compounds yields, besides the reported isoimides 3 and/or the amides 4 , also the imides 5 . The observed product dichotomy is considered as the result of an intramolecular nucleophilic attack on the aroyl group, of the pressumed zwitterionic intermediate 2 , by O or N present in the ambident N-aroylimine site of 2 . The results of AM1 calculations agree with the product studies and both permit the formulation of a set of rules correlating structure and selectivity.  相似文献   
103.
We describe a semi-analytical numerical method for coherent isotropic scattering time-dependent radiative transfer problems in slab geometry. This numerical method is based on a combination of two classes of numerical methods: the spectral methods and the Laplace transform (LTSN) methods applied to the radiative transfer equation in the discrete ordinates (SN) formulation. The basic idea is to use the essence of the spectral methods and expand the intensity of radiation in a truncated series of Laguerre polynomials in the time variable and then solve recursively the resulting set of “time-independent” SN problems by using the LTSN method. We show some numerical experiments for a typical model problem.  相似文献   
104.
Muon electron pairs were detected in an Al multiplate spark chamber, exposed to a neutrino beam from the CERN PS. The leptons were not accompanied by other particles, except occasionally by protons. The background came mainly from muon associated π0 production, with one decay gamma lost. It was determined empirically, together with the small contribution from υ e reactions. For electron energies above 2 GeV the background is 5.7±1.5 events, whereas 18 (μe)-candidates have been observed. Hence the effect is established, with a rate of about 10?4 as compared to the muonic reactions above 3 GeV. Charm creation as the origin of this (μe)-production process is excluded; heavy neutral lepton production does not fit the kinematics observed. Instead the events are compatible with the two-body decay of an object with variable invariant mass of order 1 GeV, possibly resulting from axion interactions.  相似文献   
105.
106.
Preface     
  相似文献   
107.
108.
TGA, DTA and DSC analyses indicate that benzotriazole is significantly more stable thermally than 1,2,3-triazole.  相似文献   
109.
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   
110.
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