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   643620篇
  免费   7024篇
  国内免费   1874篇
化学   343286篇
晶体学   9402篇
力学   28690篇
综合类   25篇
数学   78875篇
物理学   192240篇
  2021年   5048篇
  2020年   5816篇
  2019年   6223篇
  2018年   8164篇
  2017年   8017篇
  2016年   12418篇
  2015年   7859篇
  2014年   11895篇
  2013年   28773篇
  2012年   22044篇
  2011年   26808篇
  2010年   18965篇
  2009年   18477篇
  2008年   24796篇
  2007年   24793篇
  2006年   22948篇
  2005年   20650篇
  2004年   19092篇
  2003年   16948篇
  2002年   16693篇
  2001年   18283篇
  2000年   14115篇
  1999年   11067篇
  1998年   9374篇
  1997年   9136篇
  1996年   8896篇
  1995年   8067篇
  1994年   8096篇
  1993年   7728篇
  1992年   8750篇
  1991年   8653篇
  1990年   8341篇
  1989年   8025篇
  1988年   8182篇
  1987年   7972篇
  1986年   7571篇
  1985年   9885篇
  1984年   10204篇
  1983年   8335篇
  1982年   8477篇
  1981年   8394篇
  1980年   8045篇
  1979年   8380篇
  1978年   8760篇
  1977年   8620篇
  1976年   8605篇
  1975年   7910篇
  1974年   7988篇
  1973年   8130篇
  1972年   5729篇
排序方式: 共有10000条查询结果,搜索用时 10 毫秒
111.
112.
It is now commonly accepted that cosmic γ-ray bursts (GRBs) are of cosmological origin. This conclusion is based on the statistical analysis of GRBs and the measurements of line redshifts in GRB optical afterglows, i.e., in the so-called long GRBs. In this review, the models of radiation and models of GRB sources are considered. In most of these models, if not in all of them, the isotropic radiation cannot provide the energy release necessary for the appearance of a cosmological GRB. No correlation is noted between the redshift, the GRB-spectrum shape, and the total detected energy. The comparison between data obtained in the Soviet experiment KONUS and the American experiment BATSE shows that they substantially differ in statistical properties and the detection of hard x-ray lines. The investigation of hard gamma (0.1–10 GeV) afterglows, the measurement of prompt optical spectra during the GRB detection, and the further investigation of hard x-ray lines is of obvious importance for gaining insight into the GRB origin. Observations of two bright optical GRB afterglows point to the fact that an initially bright optical flare is directly related to the GRB itself, and the subsequent weak and much more continuous optical radiation is of a different nature. The results of observations of optical GRB afterglows are discussed. They point to the fact that the GRBs originate in distant galaxies with a high matter density, where intense star formation takes place. The interaction of the cosmological GRB radiation with a dense surrounding molecular cloud results in the appearance of long-duration (up to 10 years) weak optical afterglows associated with the heating and reradiation of gas. Results of 2D numerical simulation of the heating and reradiation of gas in various variants of the relative disposition of GRB and molecular clouds are presented. In conclusion, the possible relation between the so-called short GRBs and recurrent sources of soft γ rays in our Galaxy, the so-called “soft gamma repeaters,” is discussed.  相似文献   
113.
114.
In the frame of classical SOBOLEV spaces the FREDHOLM property will be characterized for a class of singular integro-differential operators on the positive halfaxis. A symbol calculus moreover permits to specify an index formula and a special FREDHOLM inverse.  相似文献   
115.
The thermal and dielectric behaviors of poly(vinylidene fluoride-trifluoroethylene) copolymers near the ferroelectric-to-paraelectric phase transition are investigated for samples with 20, 25, 30, and 40 mol% trifluoroethylene (TrFE). The data suggest that the transition becomes continuous for a particular composition near 50 mol% TrFE. Experimental data are sensitive to thermal history (kinetics of crystallization, and kinetics and cycling over the structural transition). It is found that several anomalies are present at the structural change, and in particular the 30 mol% TrFE sample shows the most marked anomalies. These phenomena can be attributed to defects, but another possibility would be the existence of an intemediate supplementary phase. Both hypotheses are discussed.  相似文献   
116.
In recent years there has emerged significant interest in low pressure radio frequency (rf) glow discharges which are used widely particulary in IC fabrication. Various parameters of the rf glow discharge have been found to be useful for its electrical characterization; however, there is no uniformity and agreement. Extensive experimental investigations on various discharge systems have shown, that the self-bias on the rf driven electrode, the complex conductivity and the breakdown characteristic are preferable parameters of rf discharges. Advantageously the self-bias and the complex conductivity should be presented in dependence on the pressure and the applied rf voltage. The discharge current cannot be measured quite accurately due to currents via leaky capacitors and the deviations from a sinusoidal form of the current due to nonlinearities.  相似文献   
117.
118.
The electro-optic response of ferroelectric smectic C* liquid crystals has been studied. Anomalous switching behaviour of such materials which possess a negative dielectric anisotropy has been reported. These materials show a minimum in response time at a sufficiently high field. We present results showing the dependency of this minimum upon spontaneous polarisation and the effect of AC bias. Calculations based upon the equation of motion of the director around the cone are presented which describe this effect and its dependence on the relative magnitudes of the spontaneous polarization and dielectric anisotropy of the material. Good agreement with the experimental results is found.  相似文献   
119.
120.
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