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   26398篇
  免费   4705篇
  国内免费   3902篇
化学   19291篇
晶体学   526篇
力学   1362篇
综合类   327篇
数学   2912篇
物理学   10587篇
  2024年   71篇
  2023年   441篇
  2022年   733篇
  2021年   882篇
  2020年   954篇
  2019年   1050篇
  2018年   846篇
  2017年   856篇
  2016年   1220篇
  2015年   1268篇
  2014年   1466篇
  2013年   1910篇
  2012年   2432篇
  2011年   2437篇
  2010年   1858篇
  2009年   1825篇
  2008年   2024篇
  2007年   1735篇
  2006年   1731篇
  2005年   1539篇
  2004年   1230篇
  2003年   971篇
  2002年   1046篇
  2001年   817篇
  2000年   670篇
  1999年   581篇
  1998年   394篇
  1997年   307篇
  1996年   281篇
  1995年   232篇
  1994年   217篇
  1993年   181篇
  1992年   123篇
  1991年   154篇
  1990年   90篇
  1989年   70篇
  1988年   66篇
  1987年   38篇
  1986年   52篇
  1985年   52篇
  1984年   24篇
  1983年   21篇
  1982年   18篇
  1981年   22篇
  1980年   11篇
  1979年   14篇
  1978年   11篇
  1977年   8篇
  1957年   5篇
  1936年   4篇
排序方式: 共有10000条查询结果,搜索用时 0 毫秒
41.
Based on the studies on the source regions of a group of coronal mass ejections, we have identified two types of large-scale magnetic structures, and suggested that they are intrinsic components of solar magnetism, their destabilization, expansion, and eruption into the interplanetary space are the basic physical processes which lead to the coronal mass ejections. These two types of large-scale structures are giant magnetic loops connecting the two active belts on the opposite hemispheres of the Sun, and the giant filaments (filament channels) and their related magnetic structures. The latter often appear as two parallel rows of sunspots and plage fields, which align side by side in the full disk daily and synoptic magnetograms. The magnetic neutral lines of these large-scale structures are usually longer than 50 heliographic degrees. We name this type of structure “super A configuration”. Sometimes, they are shown as very long filaments and related large-scale magnetic fields. As these magnetic structures are of very large scale, they extend to a great altitude into the corona, they are not easily recognized in magnetic field observations which are usually aimed at solar flare studies. To identify these large-scale structures becomes a key to understanding and predicting coronal mass ejections.  相似文献   
42.
双轴晶体Nd^3+:KGd(WO4)2的非偏振吸收光谱研究   总被引:1,自引:0,他引:1  
报道了用三个方向相互垂直的非偏振吸收光谱测量计算Judd-Ofelt参数从而算出双轴晶体Nd3+KGd(WO4)2的荧光寿命、荧光分支比和发射截面的方法。得到的荧光寿命为119μs,平均发射截面为2.3×10-19cm2。  相似文献   
43.
In 1991, we developed a new type of quasi-optical power combiner, called a compound quasi-optical power combiner, at Ka-band. In this paper, the circuit of such a compound quasi-optical power combiner is analysed. Its equivalent circuit model is proposed. The circuit equations, the balance condition, the injection locking and the stabilized condition of the compound quasi-optical power combiner are studed by the equivalent circuit model. As an example, a compound quasi-optical power combiner which consists of two single—cavity, two—device power combiners is analysed  相似文献   
44.
用600keV的Kr~ 离子轰击Al/Cr双层薄膜样品进行界面原子反应及相互混合的研究。实验样品是在单晶硅上蒸镀约500nm厚的铝膜,相继再蒸上所需厚度的铬膜而制成的。轰击剂量为2.0×10~(15)-2.5×10~(16)Kr~ /cm~2。用2.0MeVa粒子对轰击前后的样品进行了卢瑟福背散射(RBS)分析,发现界面处有明显的原子混合存在;当轰击剂量≥1.0×10~(16)Kr~ /cm~2时,RBS谱出现有明显的坪台,经拟合计算和x射线衍射(XRD)测量证实确有化合物Al_(13)Cr_2存在;还分别得到了原子混合量及混合效率与轰击剂量的关系;最后对界面处的原子混合机制进行了讨论。  相似文献   
45.
The centrosymmetric structure of {Cd[S2CN(CH2Ph)2]2}2 features both bridging and chelating dithiocarbamate ligands so that a square pyramidal S5 coordination geometry results. Copyright © 2004 John Wiley & Sons, Ltd.  相似文献   
46.
In the crystal of the title compound, the quinone fragment of the host (1) participates in weak D-A interactions with a neighboring naphthalene moiety of 1 and with the guest molecule via fairly short intermolecular face-to-face contacts. An intermolecular electrostatic interaction between a quinone-oxygen atom and a neighboring quinone ring is suggested by short O...C contacts. There exist several C-H...O hydrogen bonds, one of which seems to contribute to the formation of a centrosymmetric dimer of 1.  相似文献   
47.
48.
49.
年龄相关的种群扩散系统的最优分布控制   总被引:5,自引:1,他引:4  
本文讨论年龄相关的种群扩散系统的最优分布控制 ,证明了最优分布控制的存在性 ,得到了分布控制为最优的充分必要条件及确定最优控制的最优性组 .  相似文献   
50.
Applying the approximate Fokker-Planck equation we derived, we obtain the analytic expression of thestationary laser intensity distribution Pst(Ⅰ) by studying the single-mode laser cubic model subject to colored cross-correlation additive and multiplicative noise, each of which is colored. Based on it, we discuss the effects on the stationarylaser intensity distribution Pst(Ⅰ) by cross-correlation between noises and “color“ of noises (non-Markovian effect) whenthe laser system is above the threshold. In detail, we analyze two cases: One is that the three correlation-times (i.e.the self-correlation and cross-correlation times of the additive and multiplicative noise) are chosen to be the same value(τ1 = τ2 = τ3 = τ). For this case, the effect of noise cross-correlation is investigated emphatically, and we detect thatonly when λ≠ 0 can the noise-induced transition occur in the Pst(Ⅰ) curve, and only when τ≠ 0 and λ≠ 0, can the“reentrant noise-induced transition“ occur. The other case is that the three correlation times are not the same value,τ1 ≠τ2 ≠τ3. For this case, we find that the noise-induced transition occurring in the Pst (Ⅰ) curve is entirely differentwhen the values of τ1, τ2, and τ3 are changed respectively. In particular, when τ2 (self-correlation time of additivenoise) is changing, the ratio of the two maximums of the Pst(Ⅰ) curve R exhibits an interesting phenomenon, “reentrantnoise-induced transition“, which demonstrates the effect of noise “color“ (non-Markovian effect).  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