全文获取类型
收费全文 | 6269篇 |
免费 | 1333篇 |
国内免费 | 1766篇 |
专业分类
测绘学 | 763篇 |
大气科学 | 893篇 |
地球物理 | 1432篇 |
地质学 | 3557篇 |
海洋学 | 1005篇 |
天文学 | 271篇 |
综合类 | 651篇 |
自然地理 | 796篇 |
出版年
2024年 | 50篇 |
2023年 | 132篇 |
2022年 | 432篇 |
2021年 | 472篇 |
2020年 | 391篇 |
2019年 | 425篇 |
2018年 | 470篇 |
2017年 | 412篇 |
2016年 | 480篇 |
2015年 | 434篇 |
2014年 | 474篇 |
2013年 | 499篇 |
2012年 | 476篇 |
2011年 | 453篇 |
2010年 | 446篇 |
2009年 | 389篇 |
2008年 | 349篇 |
2007年 | 305篇 |
2006年 | 321篇 |
2005年 | 227篇 |
2004年 | 172篇 |
2003年 | 147篇 |
2002年 | 130篇 |
2001年 | 125篇 |
2000年 | 120篇 |
1999年 | 166篇 |
1998年 | 113篇 |
1997年 | 111篇 |
1996年 | 90篇 |
1995年 | 94篇 |
1994年 | 78篇 |
1993年 | 74篇 |
1992年 | 57篇 |
1991年 | 40篇 |
1990年 | 33篇 |
1989年 | 38篇 |
1988年 | 20篇 |
1987年 | 18篇 |
1986年 | 26篇 |
1985年 | 27篇 |
1984年 | 6篇 |
1983年 | 9篇 |
1982年 | 7篇 |
1980年 | 7篇 |
1979年 | 7篇 |
1978年 | 3篇 |
1965年 | 2篇 |
1958年 | 3篇 |
1957年 | 1篇 |
1954年 | 2篇 |
排序方式: 共有9368条查询结果,搜索用时 375 毫秒
901.
Christian Wolf Alfonso Aragón-Salamanca Michael Balogh Marco Barden Eric F. Bell Meghan E. Gray Chien Y. Peng David Bacon Fabio D. Barazza Asmus Böhm John A. R. Caldwell Anna Gallazzi Boris Häußler Catherine Heymans Knud Jahnke Shardha Jogee Eelco van Kampen Kyle Lane Daniel H. McIntosh Klaus Meisenheimer Casey Papovich Sebastian F. Sánchez y Taylor Lutz Wisotzki Xianzhong Zheng 《Monthly notices of the Royal Astronomical Society》2009,393(4):1302-1323
We investigate the properties of optically passive spirals and dusty red galaxies in the A901/2 cluster complex at redshift ∼0.17 using rest-frame near-ultraviolet–optical spectral energy distributions, 24-μm infrared data and Hubble Space Telescope morphologies from the STAGES data set. The cluster sample is based on COMBO-17 redshifts with an rms precision of σ cz ≈ 2000 km s−1 . We find that 'dusty red galaxies' and 'optically passive spirals' in A901/2 are largely the same phenomenon, and that they form stars at a substantial rate, which is only four times lower than that in blue spirals at fixed mass. This star formation is more obscured than in blue galaxies and its optical signatures are weak. They appear predominantly in the stellar mass range of log M * /M⊙ =[10, 11] where they constitute over half of the star-forming galaxies in the cluster; they are thus a vital ingredient for understanding the overall picture of star formation quenching in clusters. We find that the mean specific star formation rate (SFR) of star-forming galaxies in the cluster is clearly lower than in the field, in contrast to the specific SFR properties of blue galaxies alone, which appear similar in cluster and field. Such a rich red spiral population is best explained if quenching is a slow process and morphological transformation is delayed even more. At log M * /M⊙ < 10 , such galaxies are rare, suggesting that their quenching is fast and accompanied by morphological change. We note that edge-on spirals play a minor role; despite being dust reddened they form only a small fraction of spirals independent of environment. 相似文献
902.
The fast neutron capture process (the r-process) occurs in the neutron-rich circumstance. However its concrete physical environment is not very clear. With recent progress in observations, many extremely metal-poor halo stars have been discovered. They have two characteristics: one is the overabundance of fast neutron elements with the relative abundance consistent with that of the sun; the other is that fast neutron element contents in stars at the same metal abundance have a very large dispersion. This provides a particular way to study the origin of the r-process. Simulation was used to study the galaxy's evolution process and the resulting dispersion of fast neutron nuclide contents in stars. The model of galaxy evolution obtained in this way not only contains spontaneous star formation in the gas region, but also includes the star formation excited by the supernova explosion. It is shown from our results that the supernovae at the low mass end should be the place producing the fast neutron nuclides. In addition, it is also shown that the non-uniformity of the galaxy evolution caused by the supernova explosion is not enough to explain the observed dispersion of fast neutron element contents in halo stars. This problem should be further studied. 相似文献
903.
Chia-Nan Liu Jia-Jyun Dong Yih-Ferng Peng Hsiao-Fung Huang 《Engineering Geology》2009,104(3-4):241-253
Typhoon Herb in 1996 caused widespread debris flows in central Taiwan. The 7.3 Chi-Chi earthquake on September 21, 1999, which also took place in central Taiwan, induced many landslides in the region. These landslides turned into debris flows when Typhoon Toraji struck Taiwan in 2001. This research selects three regions which suffered a ground motion class of 5, 6, and 7 on the Richter scale during the Chi-Chi earthquake as study areas. Air photos from 1997 and 2001 of these regions are used to map the gully-type debris flows that took place after Typhoons Herb and Toraji, respectively. The gullies adjacent to the debris flow, but without a trace of debris flows, are also mapped as the non-debris flow data. The topography, hydrogeology, and rainfall factors – where debris flow occurred and in which there was no occurrence of debris flows in these gullies were retrieved from DTM, geological maps, and iso-countour maps, and of rainfall through GIS processing. These characteristic are introduced into a probabilistic neural network to build a predicting model for the probability of the occurrence of debris flows. Three series of cross analyses are conducted to compare the probability of the occurrence of debris flows of the same dataset predicted by different prediction models. The results reveal that the susceptibility of debris flows was elevated after the Chi-Chi earthquake struck. The upsurge of susceptibility was more obvious for the regions that received a higher class of ground motion. 相似文献
904.
内蒙古苏莫查干敖包萤石矿区流纹岩锆石SHRIMP定年及地质意义 总被引:5,自引:1,他引:4
内蒙古苏查(苏莫查干敖包)萤石矿区晚古生代火山沉积岩分布广泛,主要岩石类型有碳泥质板岩、结晶灰岩、凝灰岩、千枚岩、英安岩和流纹岩,其中碳泥质板岩和流纹岩为苏查特大型萤石矿床的顶和底板围岩。采用锆石SHRIMP UPb铅法分别对底板围岩中蚀变流纹岩和顶板围岩中未蚀变流纹岩样品进行了同位素年代测定,所获数据分别为276±10 Ma和271±8 Ma。蚀变和未蚀变流纹岩的形成时间均为海西晚期(早二叠世)。苏查萤石矿区早二叠世流纹岩是华北陆台与西伯利亚板块从碰撞挤压到松弛张裂转折期,酸性岩浆喷发活动的产物,其成岩物质来自壳、幔混合源。早二叠世流纹岩的出现不仅标志着苏查到西里庙地区海西期构造岩浆活动的终结,同时也为苏查特大型萤石矿床的成矿作用提供了动力、热力和物质来源。早二叠世流纹岩成岩时代的厘定不仅为阐明华北陆台北缘西段构造演化历史提供了科学依据,而且对于查明流纹岩的原岩性质和圈定新的萤石矿床找矿靶区也具有重要意义。 相似文献
905.
记述了四川盆地西南部晚侏罗世上沙溪庙组顶部的中国盗龙型肉食龙类化石材料,并依此建立一新属新种——犍为乐山龙 (Leshansaurus qianweiensis gen. et sp. nov.)。它以上枕骨中嵴呈尖峰状,额骨最大长度与最大宽度之比约2.86,基蝶骨之基翼骨突细长,环椎间椎体马蹄形,背椎横突相当细长,背椎和荐椎神经棘非常薄,荐椎椎体具有明显的腹嵴,肠骨内侧髋臼缘存在一明显的嵴等特征区别于其他肉食龙类。犍为乐山龙是目前所知四川盆地产出层位最高的肉食龙材料,它的发现扩大了肉食龙类的时代分布和地理分布,对探讨肉食龙的演化具有比较重要的意义。 相似文献
906.
Hong Lu Tengshui Chen Kliti Grice Paul Greenwood Ping’an Peng Guoying Sheng 《Organic Geochemistry》2009,40(8):902-911
An unusual series of C22–C27 monounsaturated sterenes and C24–C30 tetracyclic terpanes (17,21-secohopanes) were detected in relatively high concentrations in an immature evaporitic marl sediment of the Jinxian Sag, Bohai Bay Basin, North China. The site of unsaturation in these novel sterenes is assigned tentatively to the D ring on the basis of mass spectral interpretation, which also distinguishes them from reported unsaturated sterenes. Other hydrocarbon biomarker or stable isotope characteristics are indicative of microbial (e.g. methyl hopanes), phytoplankton or higher plant (depleted δ13C values of isoprenoids and hopanes) inputs and an anoxic carbonate depositional environment (hexacyclic hopanes; tetracyclic terpanes). The hydrocarbon composition showed no obvious biodegradation and the relatively high concentration of unsaturated terpenoids (e.g. gammacerene) and low values of other established maturity parameters (Ts/Tm = 0.23; Ro = 0.44%; Tmax = 417 °C), are consistent with sediments of low maturity. The novel, low molecular weight sterenes and the tetracyclic terpanes may be early diagenetic products of microbial sources in a carbonate environment. 相似文献
907.
钛磁铁矿的制备及其异相Fenton反应催化性能 总被引:2,自引:0,他引:2
在水相中合成了钛磁铁矿(Fe3-xTixO4),并用XRD、MSssbauer、TG-DSC和SEM等手段对合成的Fe3-xTixO4进行了表征。结果表明,合成的Fe3-xTixO4为立方晶系尖晶石结构,样品中的钛离子都已经进入其晶格中;钛掺杂有抑制钛磁铁矿进一步向钛磁赤铁矿转化和稳定尖晶石结构的作用。此外,以亚甲基蓝降解为探针反应,考察了钛磁铁矿异相Fenton反应的催化性能。实验表明,钛含量较高的钛磁铁矿是一种性能优越的异相Fenton反应催化剂。 相似文献
908.
随着深度学习的发展,遥感影像处理技术也从传统机器学习算法向深度学习转变,然而,用于遥感图像的训练数据集却十分稀少,且数据标注困难。本文将GIS技术与图像标注技术相结合,基于Flask Web框架设计一个可用于海量遥感数据的标注系统。该系统可用于海量遥感数据的数据框标注、数据类别标注,以及目标关键点标注,同时能将标注数据导出为深度学习训练最常用的COCO数据集和VOC2007两种格式。 相似文献
909.
随着对地立体观测体系的建立,遥感大数据不断累积。传统基于文件、景/幅式的影像组织方式,时空基准不够统一,集中式存储不利于大规模并行分析。对地观测大数据分析仍缺乏一套统一的数据模型与基础设施理论。近年来,数据立方体的研究为对地观测领域大数据分析基础设施提供了前景。基于统一的分析就绪型多维数据模型和集成对地观测数据分析功能,可构建一个基于数据立方的对地观测大数据分析基础设施。因此,本文提出了一个面向大规模分析的多源对地观测时空立方体,相较于现有的数据立方体方法,强调多源数据的统一组织、基于云计算的立方体处理模式以及基于人工智能优化的立方体计算。研究有助于构建时空大数据分析的新框架,同时建立与商业智能领域的数据立方体关联,为时空大数据建立统一的时空组织模型,支持大范围、长时序的快速大规模对地观测数据分析。本文在性能上与开源数据立方做了对比,结果证明提出的多源对地观测时空立方体在处理性能上具有明显优势。 相似文献
910.