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   585606篇
  免费   61948篇
  国内免费   77892篇
测绘学   49164篇
大气科学   66325篇
地球物理   124141篇
地质学   258953篇
海洋学   70817篇
天文学   69625篇
综合类   24534篇
自然地理   61887篇
  2023年   5101篇
  2022年   14769篇
  2021年   18656篇
  2020年   16523篇
  2019年   18063篇
  2018年   22540篇
  2017年   21438篇
  2016年   23680篇
  2015年   20377篇
  2014年   25835篇
  2013年   36856篇
  2012年   31078篇
  2011年   34386篇
  2010年   33128篇
  2009年   35080篇
  2008年   33870篇
  2007年   32570篇
  2006年   31004篇
  2005年   25253篇
  2004年   20512篇
  2003年   16944篇
  2002年   16181篇
  2001年   14821篇
  2000年   15264篇
  1999年   12138篇
  1998年   9690篇
  1997年   8784篇
  1996年   8346篇
  1995年   8198篇
  1994年   7373篇
  1993年   5517篇
  1992年   5128篇
  1991年   4771篇
  1990年   4643篇
  1989年   4233篇
  1988年   4013篇
  1987年   4466篇
  1986年   4080篇
  1985年   4909篇
  1984年   5367篇
  1983年   4911篇
  1982年   4809篇
  1981年   4322篇
  1980年   3981篇
  1979年   3834篇
  1978年   3717篇
  1977年   3475篇
  1976年   3223篇
  1975年   3107篇
  1973年   3265篇
排序方式: 共有10000条查询结果,搜索用时 18 毫秒
991.
We used multi-component profiles to model the Hβ and [OⅢ]λλ4959,5007 lines of SDSS J143030.22-001115.1, a narrow-line Seyfert 1 galaxy (NLS1) in a sample of 150 NLS1 candidates selected from the Sloan Digital Sky Survey (SDSS), Early Data Release (EDR). After subtracting the Hβ contribution from narrow line regions (NLRs), we found that its full width half maximum (FWHM) of broad Hβ line is nearly 2900km s~(-1) , significantly larger than the customarily adopted criterion of 2000 km s~(-1) . With its weak Fe Ⅱ multiples, we believe that SDSS J143030.22-001115.1 should not be classified as a genuine NLS1. When we calculate the virial black hole masses of NLS1s, we should use the Hβ linewidth after subtracting the NLR component.  相似文献   
992.
Y.C. Minh  W.M. Irvine   《New Astronomy》2006,11(8):594-599
The large-scale structure associated with the 2′N HNCO peak in Sgr B2 [Minh, Y.C., Haikala, L., Hjalmarson, Å., Irvine, W.M., 1998. ApJ 498, 261 (Paper I)] has been investigated. A ring-like morphology of the HNCO emission has been found; this structure may be colliding with the Principal Cloud of Sgr B2. This “HNCO Ring” appears to be centered at (l,b) = (0.7°,−0.07°), with a radius of 5 pc and a total mass of 1.0 × 105 to 1.6 × 106 M. The expansion velocity of the Ring is estimated to be 30–40 km s−1, which gives an expansion time scale of 1.5 × 105 year. The morphology suggests that collision between the Ring and the Principal Cloud may be triggering the massive star formation in the Sgr B2 cloud sequentially, with the latest star formation taking place at the 2′N position. The chemistry related to HNCO is not certain yet, but if it forms mainly via reaction with the evaporated OCN from icy grain mantles, the observed enhancement of the HNCO abundance can be understood as resulting from shocks associated with the collision between the Principal Cloud and the expanding HNCO Ring.  相似文献   
993.
酶解法提取鱼油的工艺参数优化   总被引:1,自引:0,他引:1  
利用蛋白酶酶解法从黄鳍金枪鱼(Thunnus albacares)加工的下脚料——鱼头中提取鱼油。以鱼油提取率和感官特征为指标,通过正交优化实验设计,获得了胰蛋白酶提取鱼油的最佳酶解工艺参数:酶解温度45℃,酶添加量1.5%.料液质量比1:1,酶解时间4h,酶解pH8。在该条件下.鱼油的提取率为4.34%,理化指标除过氧化值外均达到SC/T3502-2000的粗鱼油二级标准。多不饱和脂肪酸总含量高达38.47%,其中DHA和EPA的含量分别为23.63%和4.84%。  相似文献   
994.
OLE技术的开发方式能够将成熟地理信息系统软件的强大功能和面向对象开发语言有机结合起来,但在海量数据管理上还存在一些问题。本文以泰宁基础地理信息系统(TNGIS)的开发为例,重点介绍了基于OLE技术的回叫机制、MapInfo对象、实现MapInfo与应用程序通讯所用的类、窗体类及其使用方法。以此为基础,笔者提出了以大型分布式数据库MYSQL为平台,采用图形与属性分离的方式对海量空间数据进行管理的方法,以解决系统运行速度缓慢的问题,达到优化数据访问方法的目的。  相似文献   
995.
基于蚁群算法的城市可持续发展综合评价   总被引:1,自引:0,他引:1  
在可持续发展体系分类的基础上,应用蚁群算法对可持续发展各分类指数公式和综合指数公式进行优化,建立可持续发展评价模型。将该模型应用于乌鲁木齐市可持续发展水平评价,评价结果与现状分析一敛。结果表明该模型简单适用、有良好的通用性。  相似文献   
996.
997.
To derive a matched filter for detecting a weak target signal in a hyperspectral image, an estimate of the band-to-band covariance of the target-free background scene is required. We investigate the effects of including some of the target signal in the background scene. Although the covariance is contaminated by the presence of a target signal (there is increased variance in the direction of the target signature), we find that the matched filter is not necessarily affected. In fact, if the variation in plume strength is strictly uncorrelated with the variation in background spectra, the matched filter and its signal-to-clutter ratio (SCR) performance will not be impaired. While there is little a priori reason to expect significant correlation between the plume and the background, there usually is some residual correlation, and this correlation leads to a suppressing effect that limits the SCR obtainable even for strong plumes. These effects are described and quantified analytically, and the crucial role of this correlation is illustrated with some numerical examples using simulated plumes superimposed on real hyperspectral imagery. In one example, we observe an order-of-magnitude loss in SCR for a matched filter based on the contaminated covariance.  相似文献   
998.

As well known, the methods of remote sensing and Bowen Ratio for retrieving surface flux are based on energy balance closure; however, in most cases, surface energy observed in experiment is lack of closure. There are two main causes for this: one is from the errors of the observation devices and the differences of their observational scale; the other lies in the effect of horizontal advection on the surface flux measurement. Therefore, it is very important to estimate the effects of horizontal advection quantitatively. Based on the local advection theory and the surface experiment, a model has been proposed for correcting the effect of horizontal advection on surface flux measurement, in which the relationship between the fetch of the measurement and pixel size for remote sensed data was considered. By means of numerical simulations, the sensitivities of the main parameters in the model and the scaling problems of horizontal advection were analyzed. At last, by using the observational data acquired in agricultural field with relatively homogeneous surface, the model was validated.

  相似文献   
999.
1000.
This research paper analyses the grain-size characteristics of the Quaternary deposits at Xingshan near Siping, Jilin province in China by employing graphic measures to study the grain size distribution and its mode of transport and deposition. The Quaternary deposits at Xingshan lie unconformable on Cretaceous rocks made of siltstone, mudstone and sandstone. The average grain size is between 8.06 to 8.55Φ (0.002 6 ~0.003 7 mm). The Quaternary deposits at Xingshan mainly compose of very fine silt to clay. The compositions of the grade are clay 63% and silt 37%. The clay size components are weathered debris transported and deposited by flowing water from the SE highlands or hills to the low lying NW Xingshan plains whereas the silty components accumulated by aoelian process. The Quaternary deposits at Xingshan accumulated in the middle and late Pleistocene interglacial periods from (459.12~39.03) ka to (88.92~7.56) ka. The standard deviation ranged from 0.96 to 1.36Φ, indicating that the sediments are moderately to poorly sorted, Coefficient of skewness ranged from 0.16~0.31 with an average skewness of 0.218, (Positively skewed towards fine). Kurtosis values (0.84~1.05) from the grain size distribution and visual inspection of the frequency curves indicate platykurtic to mesokurtic curves and unimodal to bimodal grain-size distribution. The type of deposit formation is sand dune and the source is at a distal from its provenance.  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