全文获取类型
收费全文 | 21996篇 |
免费 | 3626篇 |
国内免费 | 4594篇 |
专业分类
测绘学 | 1779篇 |
大气科学 | 3813篇 |
地球物理 | 5724篇 |
地质学 | 11119篇 |
海洋学 | 2837篇 |
天文学 | 1164篇 |
综合类 | 1720篇 |
自然地理 | 2060篇 |
出版年
2024年 | 90篇 |
2023年 | 365篇 |
2022年 | 721篇 |
2021年 | 925篇 |
2020年 | 795篇 |
2019年 | 872篇 |
2018年 | 1287篇 |
2017年 | 1198篇 |
2016年 | 1219篇 |
2015年 | 1012篇 |
2014年 | 1120篇 |
2013年 | 1134篇 |
2012年 | 1697篇 |
2011年 | 1471篇 |
2010年 | 1243篇 |
2009年 | 1095篇 |
2008年 | 1122篇 |
2007年 | 939篇 |
2006年 | 855篇 |
2005年 | 1476篇 |
2004年 | 1410篇 |
2003年 | 1232篇 |
2002年 | 804篇 |
2001年 | 699篇 |
2000年 | 589篇 |
1999年 | 697篇 |
1998年 | 567篇 |
1997年 | 510篇 |
1996年 | 496篇 |
1995年 | 418篇 |
1994年 | 354篇 |
1993年 | 347篇 |
1992年 | 275篇 |
1991年 | 226篇 |
1990年 | 182篇 |
1989年 | 147篇 |
1988年 | 149篇 |
1987年 | 77篇 |
1986年 | 65篇 |
1985年 | 55篇 |
1984年 | 35篇 |
1983年 | 25篇 |
1982年 | 39篇 |
1981年 | 33篇 |
1980年 | 26篇 |
1979年 | 22篇 |
1978年 | 8篇 |
1976年 | 12篇 |
1975年 | 9篇 |
1958年 | 21篇 |
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
71.
Xue-Bing Wu Wen-Wen Zuo Qian Yang Wei-Min Yi Chen-Wei Yang Wen-Juan Liu Peng Jiang Xin-Wen Shu and Hong-Yan Zhou 《天文和天体物理学研究(英文版)》2012,(9):1185-1190
Quasars with redshifts greater than 4 are rare, and can be used to probe the structure and evolution of the early universe. Here we report the discovery of six new quasars with i-band magnitudes brighter than 19.5 and redshifts between 2.4 and 4.6 from spectroscopy with the Yunnan Faint Object Spectrograph and Camera (YFOSC) at the Lijiang 2.4 m telescope in February, 2012. These quasars are in the list of z > 3.6 quasar candidates selected by using our proposed J K/i Y criterion and the photometric redshift estimations from the SDSS optical and UKIDSS near-IR photometric data. Nine candidates were observed by YFOSC, and five among six new quasars were identified as z > 3.6 quasars. One of the other three objects was identified as a star and the other two were unidentified due to the lower signal-to-noise ratio of their spectra. This is the first time that z > 4 quasars have been discovered using a telescope in China. Thanks to the Chinese Telescope Access Program (TAP), the redshift of 4.6 for one of these quasars was confirmed by the Multiple Mirror Telescope (MMT) Red Channel spectroscopy. The continuum and emission line properties of these six quasars, as well as their central black hole masses and Eddington ratios, were obtained. 相似文献
72.
论耿湋诗歌在唐诗演进中的角色和影响 总被引:1,自引:0,他引:1
邓建 《广东海洋大学学报》2007,27(2):70-73
耿湋诗歌在唐诗演进过程中扮演了独特的角色,产生了不容忽视的影响。其内倾凝缩的情感取向、注重细节的表现手法、清浅平远的审美风格与盛唐诗歌之外向浓烈、疏朗大气、雄浑爽健形成鲜明对照,对急于突破前人拘囿、有心另辟蹊径的中晚唐诗人有明显的开启、示范、渗透、辐射之功。其工于五律、兼擅七律的诗歌体式表现出明显的过渡痕迹,昭示出中晚唐古风消歇、近体勃兴与五律盛极、七律崛起的历史趋势。 相似文献
73.
A method that estimates mass and stiffness matrices of shear building from modal test data is presented in this paper. The method depends on only measurable points that are less in number than the total structural degrees of freedom, and on the first two orders of structural mode measured. So it is applicable to most of the general test. Based on this method modal data of unmeasurable points are estimated, then global mass and stiffness matrices of structure are obtained by using the first two orders of modal data. Taking advantage of iteration the optimum global mass and stiffness matrices are gained. Finally, an example is studied in this paper. Its result shows that this method is reliable. © 1998 John Wiley & Sons, Ltd. 相似文献
74.
Antonio?VecchioEmail author Leonardo?Primavera Vincenzo?Carbone Luca?Sorriso-Valvo 《Solar physics》2005,229(2):359-372
We use the Proper Orthogonal Decomposition (POD) to investigate the spatiotemporal features of the solar activity. Daily observation
in the period 1949–1996 of the green coronal emission line at 530.3 nm are used as indicators of the activity behavior. We
show that few POD modes suffice in describing both the space and time main periodicities. In particular, being affected by
a strongly energetic stochastic behavior, daily data are described by five POD modes, while two POD modes are enough to describe
the butterfly diagram in monthly averaged data. Apart from the basic period T0 = 11 years, using daily data we found evidences for intercycle temporal periodicities. 相似文献
75.
76.
Chen Cao Hong Wu Jian-Ling Wang Cai-Na Hao Zu-Gan Deng Xiao-Yang Xia Zhen-Long Zou National Astronomical Observatories Chinese Academy of Sciences Beijing Graduate School of Chinese Academy of Sciences Beijing College of Physical Sciences Graduate School of Chinese Academy of Sciences Beijing Department of Physics Tianjin Normal University Tianjin 《中国天文和天体物理学报》2006,6(2):197-209
We selected a sample of luminous infrared galaxies by cross-identification of the Faint Source Catalogue (FSC) and Point Source Catalogue (PSC) of the IRAS Survey with the Second Data Release of the SDSS. The size of our sample is 1267 for FSC and 427 for PSC by using the 2σ significance level cross-section. The "likelihood ratio" method is used to estimate the individual's reliability and for defining two more reliable subsamples (908 for FSC and 356 for PSC). A catalog of infrared, optical and radio data is compiled and will be used in further work. Some statistical results show that luminous infrared galaxies are quite different from ultra-luminous infrared galaxies. The AGN fractions of galaxies at different infrared luminosities and the radio-infrared correlations are consistent with the previous studies. 相似文献
77.
Sedimentary evolution of the Holocene subaqueous clinoform off the southern Shandong Peninsula in the Western South Yellow Sea 总被引:1,自引:0,他引:1
Jiandong Qiu Jian Liu Yoshiki Saito Zigeng Yang Baojing Yue Hong Wang Xianghuai Kong 《中国海洋大学学报(英文版)》2014,13(5):747-760
Based on the stratigraphic sequence formed since the last glaciation and revealed by 3000 km long high-resolution shallow seismic profiles and the core QDZ03 acquired recently off the southern Shandong Peninsula, we addressed the sedimentary characteristics of a Holocene subaqueous clinoform in this paper. Integrated analyses were made on the core QDZ03, including sedimentary facies, sediment grain sizes, clay minerals, geochemistry, micro paleontology, and AMS 14 C dating. The result indicates that there exists a Holocene subaqueous clinoform, whose bottom boundary generally lies at 15–40 m below the present sea level with its depth contours roughly parallel to the coast and getting deeper seawards. The maximum thickness of the clinoform is up to 22.5 m on the coast side, and the thickness contours generally spread in a banded way along the coastline and becomes thinner towards the sea. At the mouths of some bays along the coast, the clinoform stretches in the shape of a fan and its thickness is evidently larger than that of the surrounding sediments. This clinoform came into being in the early Holocene(about 11.2 cal kyr BP) and can be divided into the lower and upper depositional units(DU 2 and DU 1, respectively). The unit DU 2, being usually less than 3 m in thickness and formed under a low sedimentation rate, is located between the bottom boundary and the Holocene maximum flooding surface(MFS), and represents the sediment of a post-glacial transgressive systems tract; whereas the unit DU 1, the main body of the clinoform, sits on the MFS, belonging to the sediment of a highstand systems tract from middle Holocene(about 7–6 cal kyr BP) to the present. The provenance of the clinoform differs from that of the typical sediments of the Yellow River and can be considered as the results of the joint contribution from both the Yellow River and the proximal coastal sediments of the Shandong Peninsula, as evidenced by the sediment geochemistry of the core. As is controlled mainly by coactions of multiple factors such as the Holocene sea-level changes, sediment supplies and coastal dynamic conditions, the development of the clinoform is genetically related with the synchronous clinoform or subaqueous deltas around the northeastern Shandong Peninsula and in the northern South Yellow Sea in the spatial distribution and sediment provenance, as previously reported, with all of them being formed from the initial stage of the Holocene up to the present. 相似文献
78.
Little is known about the genome of Pacific white shrimp (Litopenaeus vannamei). To address this, we conducted BAC (bacterial artificial chromosome) end sequencing of L. vannamei. We selected and sequenced 7 812 BAC clones from the BAC library LvHE from the two ends of the inserts by Sanger sequencing. After trimming and quality filtering, 11 279 BAC end sequences (BESs) including 4 609 paired- ends BESs were obtained. The total length of the BESs was 4 340 753 bp, representing 0.18% of the L. vannamei haploid genome. The lengths of the BESs ranged from 100 bp to 660 bp with an average length of 385 bp. Analysis of the BESs indicated that the L. vannamei genome is AT-rich and that the primary repeats patterns were simple sequence repeats (SSRs) and low complexity sequences. Dinucleotide and hexanucleotide repeats were the most common SSR types in the BESs. The most abundant transposable element was gypsy, which may contribute to the generation of the large genome size of L. vannamei. We successfully annotated 4 519 BESs by BLAST searching, including genes involved in immunity and sex determination. Our results provide an important resource for functional gene studies, map construction and integration, and complete genome assembly for this species. 相似文献
79.
?????????????????????????ο??????????????????????????????????????????????????????????NGA?????????????????????????飬??????????????????????о?????????????????????????????????????????2012?????4.7??????????е?????????????????????????????????????PGA??????S??a??T???????б????о?????????????????????????????????????????????????????????????????????????????????????????????? 相似文献
80.
Water is a necessary element during gas hydrate formations. Therefore, by analyzing water depletion changes in media, the reaction characteristics of methane hydrate in media can be studied. In this study, two water sources supplying some liquid water which may be consumed by the methane hydrate formation reactions were designed and assembled. Using them, the full formation processes of methane hydrate was studied. Experimental results show the following: If heat released from nucleation reaction of methane hydrate is diffused rapidly, the nucleation ratios will be enhanced discernibly. While the hydrate is formed, a force is generated that sucks fresh water from the source into the vicinity of the hydrate, slowing down the cementation process and causing some hydrate grain dissociation. As a result of cementation differences, the hydrate reaction processes with different water sources present linear or quadratic equation characteristics. After a few repeated dissociation and formation processes of some hydrate grains caused by the fresh water, the gas amounts contained in hydrate will be significantly enhanced. 相似文献