全文获取类型
收费全文 | 3573篇 |
免费 | 394篇 |
国内免费 | 832篇 |
专业分类
测绘学 | 199篇 |
大气科学 | 410篇 |
地球物理 | 1219篇 |
地质学 | 1668篇 |
海洋学 | 588篇 |
天文学 | 141篇 |
综合类 | 168篇 |
自然地理 | 406篇 |
出版年
2024年 | 18篇 |
2023年 | 44篇 |
2022年 | 54篇 |
2021年 | 72篇 |
2020年 | 48篇 |
2019年 | 62篇 |
2018年 | 79篇 |
2017年 | 37篇 |
2016年 | 78篇 |
2015年 | 59篇 |
2014年 | 93篇 |
2013年 | 97篇 |
2012年 | 141篇 |
2011年 | 201篇 |
2010年 | 95篇 |
2009年 | 111篇 |
2008年 | 190篇 |
2007年 | 185篇 |
2006年 | 203篇 |
2005年 | 199篇 |
2004年 | 174篇 |
2003年 | 145篇 |
2002年 | 131篇 |
2001年 | 122篇 |
2000年 | 162篇 |
1999年 | 120篇 |
1998年 | 107篇 |
1997年 | 114篇 |
1996年 | 109篇 |
1995年 | 104篇 |
1994年 | 124篇 |
1993年 | 153篇 |
1992年 | 95篇 |
1991年 | 155篇 |
1990年 | 111篇 |
1989年 | 102篇 |
1988年 | 91篇 |
1987年 | 86篇 |
1986年 | 44篇 |
1985年 | 70篇 |
1984年 | 60篇 |
1983年 | 59篇 |
1982年 | 37篇 |
1981年 | 31篇 |
1980年 | 44篇 |
1965年 | 11篇 |
1964年 | 14篇 |
1959年 | 17篇 |
1958年 | 17篇 |
1957年 | 18篇 |
排序方式: 共有4799条查询结果,搜索用时 15 毫秒
81.
近东西走向的天山造山带位于中亚造山带或阿尔泰构造拼贴体的最南端,是哈萨克斯坦和塔里木板块的汇聚地带,也是一个重要的铜一金等多金属成矿带[1].天山造山带是在古生代由塔里木和西伯利亚板块之间的古亚洲洋的消减闭合,塔里木、准噶尔、哈萨克斯坦等板块的俯冲-碰撞-增生所形成[2]. 相似文献
82.
磷处理粉煤灰可作农业土壤磷源 总被引:2,自引:0,他引:2
粉煤灰(简称CCP或ash)具有改良土壤,增加植物产量的功能。此外,由于它特殊的多孔结构,也可用作吸纳并承载植物养分的载体。用NaH2PO4配制成含磷0.10mol/L浓度的溶液,对采自加拿大西安大略省Sarnia地区Lambton电厂的底灰(bottomash)进行振荡浸渍处理。结果表明,振荡浸渍66h后的粉煤灰中磷含量可达784×10-6。以磷处理粉煤灰、未进行磷处理的粉煤灰和石英砂按比例混合,作为基本生长介质进行玉米种植实验,其中实验配方设计为生长介质中含磷量分别为标准含磷浓度(50×10-6)的10%、25%、50%、75%和100%。生长26、34和46d后分别与不含磷的空白配方、施加含氮-磷-钾为0-20-0标准磷肥并控制磷含量为标准浓度(50×10-6)配方进行生物产量对比。生长实验结果表明,以磷处理粉煤灰供磷的生长介质,当含磷量为标准浓度的25%至100%时,其植物生长量就比添加标准浓度磷肥的配方好。种植46d后的生物生长量统计结果显示,含磷分别为标准浓度50%、75%和100%的实验介质中,玉米杆的鲜重较施标准磷肥介质中玉米分别增长39.46%、42.73%和46.13%;玉米杆干重依次增加29.71%、13.39%和28.87%;根鲜重平均增加16.62%;根干重平均增加14.03%。上述实验结果启示,粉煤灰可以很好地吸纳承载磷养分,并持续供给植物吸收生长,如果采用吸纳磷(或其他养分)的粉煤灰改良砂质土壤将有重要意义。 相似文献
83.
地图符号是地图的语言单位,通过对地图符号的解读,可以直观的了解地图所表达的地理信息。ArcGis的符号化功能对于测绘符号的绘制是有一定局限的。而其他大部分测图软件的符号系统基本上是针对各个软件的,不同的软件都有独立的符号系统,离开了软件平台,如不打散块状符号或不添加辅助线就不能为其它软件所调用,本文中提出的ArcSymbol插件实现了在ArcGis操作环境下无需打散或添加辅助线即可方便、快速、无损的查看和打印满足地形图图式要求的图形,减少空间数据库中的数据冗余。并且ArcSymbol支持Shape、Coverage、Geodatabase格式,不需要数据的转换就能轻松地实现图形符号化,实现符号化的无损性。 相似文献
84.
矿井构造是影响煤矿安全生产的主要因素,对瓦斯突出、矿井突水有着明显的控制作用。矿井构造具有空间性和非线性等特点,使矿井构造复杂程度评价的难度较大,据此利用MapObjects的空间分析功能和非线性人工神经网络(ANN)耦合技术,对矿井构造复杂程度进行评价。根据前人的研究成果,将突水系数、底板倾角变异系数、底板标高变异系数、断层强度指数、断层密度等5项指标引入评价体系,经过空间分析统计和模型识别,建立了矿井构造复杂程度评价模型。在开滦矿区东欢矿8煤层构造复杂程度的评价中,共训练及评价了研究区的226个评价单元.评价结果表明研究区西部及西北部构造复杂,中部及东南部构造相对简单。 相似文献
85.
86.
Brack A 《Planetary and Space Science》1996,44(11):1435-1440
Processing of organic molecules by liquid water was probably an essential requirement towards the emergence of terrestrial primitive life. According to Oparin's hypothesis, organic building blocks required for early life were produced from simple organic molecules formed in a primitive reducing atmosphere. Geochemists favour now a less reducing atmosphere dominated by carbon dioxide. In such an atmosphere, very few building blocks are formed. Import of extraterrestrial organic molecules may represent an alternative supply. Experimental support for such an alternative scenario is examined in comets, meteorites and micrometeorites. The early histories of Mars and Earth clearly show similarities. Liquid water was once stable on the surface of Mars attesting the presence of an atmosphere capable of decelerating C-rich micro-meteorites. Therefore, primitive life may have developed on Mars, as well. Liquid water disappeared from the surface of Mars very early, about 3.8 Ga ago. The Viking missions did not find, at the surface of the Martian soil, any organic molecules or clear-cut evidence for microbial activities such as photosynthesis, respiration or nutrition. The results can be explained referring to an active photochemistry of Martian soil driven by the high influx of solar UV. These experiments do not exclude the existence of organic molecules and fossils of micro-organisms which developed on early Mars until liquid water disappeared. Mars may store below its surface some well preserved clues of a still hypothetical primitive life. 相似文献
87.
Ricard A Cernogora G Fitaire M Hochard L Kouassi N Speller C Vacher JR 《Planetary and Space Science》1995,43(1-2):41-46
The kinetic reactions in N2-xCH4(C2H2) gas discharges with x less than 1% have been studied by emission spectroscopy in the afterglow of D.C. discharges and by mass spectroscopy from radiolysis ionization using alpha particles. The pressure range is from several Torr to 100 Torr. At the end of N2 D.C. discharges at room temperature, for a residence time of about 10(-2) s, the dominant active species are the N atoms with density of 10(14)-10(15) cm-3 for N2 density of about 10(17) cm-3 (3 Torr), the N2(X,V) vibrational molecules with for example [N2(X,V = 10)] approximately 10(14) cm-3 and the electronic metastable molecules N2(A 3 sigma u +) with a density of 10(12) cm-3. In such conditions, the following kinetic reactions have been studied: N2(A) + N2(A) --> N2(C,B,V') + N2(X), N2(A) + N2(X,V>5) --> N2(X) + N2(B,V') in pure N2 post-discharges and N2(A) + CH4 --> products, C + N + M2 --> CN(B,V') + M2, N2(X,V>4) + CN --> N2(X) + CN(B,A,V'), in N2-1% CH4 post-discharges. The clustering reactions of N2-(1-5%)CH4(C2H2) gas mixtures after radiolysis ionization have been studied for the H2CN+ nN2 ions and the equilibrium constants have been determined in the temperature range T = 140-300 K. 相似文献
88.
Ahmad A 《Population geography : a journal of the Association of Population Geographers of India》1995,17(1-2):7-14
"This paper documents the current evidence of the state of the Tibetan society in India with special reference to the trends in social transformation, livelihood patterns and cultural adaptation to a geographically alien environment....Three-and-a-half decades of living in India [have] demonstrated how a culture group can survive by carving out ecological niches in ethnically segregated social space and yet adapt to a new cultural environment without losing its identity." 相似文献
89.
"Debates concerning the origins and development of the late nineteenth- to early twentieth-century declines in marital fertility and infant mortality in England and Wales have been centred largely on the material provided by answers to the ?special' questions in the 1911 census. In their published form these figures have restricted researchers to an examination of large scale geographic and social class differences in the levels and rates of decline of the two phenomena. This paper outlines research conducted on a sample of individual census returns from the 1911 census. From this data it becomes clear that for Victorian and Edwardian England ?where one lived' was rather more important than ?who one was' in determining both family building strategies and the survival of those children born." 相似文献
90.
Avanesov G Zhukov B Ziman YA Kostenko V Kuzmin A Murav'ev V Fedotov V Bonev B Mishev D Petkov D Krumov A Simeonov S Boycheva V Uzunov YU Weide GG Halmann D Pössel W Head J Murchie S Schkuratov YuG Berghänel R Danz M Mangoldt T Pihan U Smith B 《Planetary and Space Science》1991,39(1-2):281-295
From February to March 1989 the Phobos 2 spacecraft took 37 TV images of Phobos at a distance of 190-1100 km. These images complement Mariner-9 and Viking data by providing higher-resolution coverage of a large region West of the crater Stickney (40-160 degrees W) and by providing disk-resolved measurements of surface brightness at a greater range of wavelengths and additional phase angles. These images have supported updated mapping and characterization of large craters and grooves, and have provided additional observations of craters' and grooves' bright rims. Variations in surface visible/near-infrared color ratio of almost a factor of 2 have been recognized; these variations appear to be associated with the ejecta of specific large impact craters. Updated determinations of satellite mass and volume allow calculation of a more accurate value of bulk density, 1.90 +/- 0.1 g cm-3. This is significantly lower than the density of meteoritic analogs to Phobos' surface, suggesting a porous interior perhaps containing interstitial ice. 相似文献