全文获取类型
收费全文 | 24616篇 |
免费 | 3981篇 |
国内免费 | 6109篇 |
专业分类
测绘学 | 2231篇 |
大气科学 | 3799篇 |
地球物理 | 5163篇 |
地质学 | 9860篇 |
海洋学 | 5119篇 |
天文学 | 1385篇 |
综合类 | 1879篇 |
自然地理 | 5270篇 |
出版年
2024年 | 101篇 |
2023年 | 325篇 |
2022年 | 915篇 |
2021年 | 988篇 |
2020年 | 1145篇 |
2019年 | 1343篇 |
2018年 | 1055篇 |
2017年 | 1216篇 |
2016年 | 1188篇 |
2015年 | 1386篇 |
2014年 | 1507篇 |
2013年 | 1718篇 |
2012年 | 1584篇 |
2011年 | 1605篇 |
2010年 | 1325篇 |
2009年 | 1511篇 |
2008年 | 1612篇 |
2007年 | 1837篇 |
2006年 | 1772篇 |
2005年 | 1519篇 |
2004年 | 1310篇 |
2003年 | 1157篇 |
2002年 | 943篇 |
2001年 | 737篇 |
2000年 | 876篇 |
1999年 | 797篇 |
1998年 | 607篇 |
1997年 | 464篇 |
1996年 | 408篇 |
1995年 | 327篇 |
1994年 | 300篇 |
1993年 | 275篇 |
1992年 | 229篇 |
1991年 | 162篇 |
1990年 | 108篇 |
1989年 | 118篇 |
1988年 | 62篇 |
1987年 | 43篇 |
1986年 | 41篇 |
1985年 | 24篇 |
1984年 | 17篇 |
1983年 | 8篇 |
1982年 | 7篇 |
1981年 | 12篇 |
1980年 | 3篇 |
1979年 | 5篇 |
1978年 | 2篇 |
1977年 | 3篇 |
1954年 | 4篇 |
1877年 | 1篇 |
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
31.
Analysis of Zn, Cu, Pb, Co, Cr, Li, Ni, K, Al, Fe extracted by 1 mol/L HCl or 0.5 mol/LHCl/H_2O_2, showed concentrations of Zn, Cu, Pb, Co, Cr, Fe, Ni were significantly correlated with Li, Al,K, and clay. Two methods are used to indicate the background value of the non-residual phase of elementsin sediments, and are the same as the methods used to indicate the background value of totalconcentrations in sediments. The first method uses correlograms and regression equations,the second usesthe mean element concentrations normalized with grain size. Li, Al, K can be used as reference elements to determine the background value of Zn, Cu, Pb, Co,Cr, Ni, Fe, while the clay concentration's correlation with some extractable concentrations can be used tocalculate the background value of the non-residual phase of elements as a percentage of clay concentrationin the sediments. Based on this study, the concept of using the background value of the non-residualphase of elements to compare the pollution level in differ 相似文献
32.
Tidal effects on temperature front in the Yellow Sea 总被引:5,自引:0,他引:5
Temperature front (TF) is one of the important features in the Yellow Sea, which forms in spring, thrives in summer, and fades
in autumn as thermocline declines. TF intensity ⋎S
T
⋎ is defined to describe the distribution of TF. Based on the MASNUM wave-tide-circulation coupled model, temperature distribution
in the Yellow Sea was simulated with and without tidal effects. Along 36°N, distribution of TF from the simulated results
are compared with the observations, and a quantitative analysis is introduced to evaluate the tidal effects on the forming
and maintaining processes of the TF. Tidal mixing and the circulation structure adapting to it are the main causes of the
TF.
Supported by the National Basic Research Program of China (No. G1999043809) and the National Science Foundation of China (No.
49736190). 相似文献
33.
三峡重庆库区深部地球物理特征与断裂构造 总被引:1,自引:0,他引:1
为了深入研究三峡重庆库区岩石圈动力学特征及其对断裂构造活动的控制和影响.并为之提供基础资料,为三峡重庆库区地震、地质灾害的监测与防治提供基础依据,在已有地球物理资料的基础上,从综合地球物理研究角度出发,通过实测地震测线资料的再解释.采用新的处理技术方法,对本区的东西向主剖面和南北向支测线的地震测深资料进行二维射线追踪处理、Pg波成像;选用场分离技术、位移数字成像技术重新处理了重力和航磁资料,通过联合反演来建立深部二维构造剖面,对剖面所揭示的基底构造特征和地壳结构特征、主要断裂构造特征以及莫霍面的起伏特征进行了精细分析和细致研究.从地球物理平面场特征出发建立了岩石圈构造三维框架。研究结果表明,这样的研究思路准确、方法得当.结论可靠;沿该剖面,把可解译的断裂分为Ⅲ级:Ⅰ级为超岩石圈断裂;Ⅱ级为壳断裂;Ⅲ级为盖层断裂。依据地球物理特征,准确揭示了库区的断裂构造特征,达到了预期效果。 相似文献
34.
The coma morphology and short-term evolution was investigated of three non-periodic comets in retrograde orbits, C/2001 Q4 (NEAT), C/2002 T7 (LINEAR), and C/2003 K4 (LINEAR). All three comets display distinct coma features, which were very different from one comet to the next and remained rather constant in shape during the observational period. A single, broad feature perpendicular to the sun-tail direction dominated the coma of C/2003 K4 in all used filters (B,V,R,I), whereas the coma of Comet C/2002 T7 exhibited different features in blue and red filters. C/2001 Q4 showed rather complex coma morphology with clear short-term variability in coma brightness. Therefore, these non-periodic comets neither show a featureless coma nor any similarities of the features detected. The overall distribution of coma material was investigated from the shape of radial coma profiles averaged around the comet nucleus. For C/2001 Q4 and C/2002 T7, the slopes fitted to the linear part of these profiles are flatter in the blue than in the red, which can be explained by the presence of coma gas. For C/2003 K4 no such difference is indicated in the May observations (r = 2.3 AU), while in July (r = 1.7 AU) the profiles in the B-filter are flatter than in V, R, and I, hence gas contamination was relevant at least in the B filter. The R and I filter images were used to determine approximate Afρ values of each comet as a function of time. 相似文献
35.
ASCA observations of the two Type Ⅱ AGNs,NGC7314 and NGC 7582,show clear variations in the broad X-ray band(0.4-10keV)on short timescales-10^4s.Spectral analysis indicates that they bot have an absorbed hard X-ray component and an unabsorbed soft“excess” component.To clarify the origin of the latter,we made a cross-correlation analysis of the two components.The results show that,for NGC7314,the soft X-ray variability is proportional to that of the hard X-ray component.This indicates that the active nucleus of NGC 7314 must be partially covered and so the soft emission is a “leaking” of the variable hard component.For NGC 7582,there is no detectable variability in the soft component, although there is a definite one in the hard component.This indicates that the variable nucleus of NGC 7582 must be fully blocked by absorbing matter,and the soft emission is most likely the scattered component predicted by the AGN unified model. 相似文献
36.
37.
38.
应用显微光度术、显微傅立叶红外光谱(Micro-FT.IR)和飞行时间二次离子质谱(TOF-SIMS)等原位微分析技术并结合均一温度测量对胜利油气区下第三系沙河街组沙三段中有机包裹体进行了研究。区分出两类有机包裹体,即原生有机包裹体和次生有机包裹体。结果表明两类有机包裹体特征不同,二者物质组成、有机质成分及化学结构、热演化程度等差别也较大。结合地质分析表明原生有机包裹体是沙三段烃源岩生成烃类运移产物,具“自生自储”特点,而次生有机包裹体是沙四段烃源岩生成的烃类二次运移的产物。沙三段是沙河街组油气运移和聚集的主要层位,因而是寻找油气资源的主要目标层。研究表明,有机包裹体是研究油气生成、运移、聚集和演化等成藏系统最有效的手段之一,在油气勘探中有重要的应用意义。 相似文献
39.
We carried out a series of linear stability analyses of the radial and low-degree non-radial p modes for stellar models with initial masses of . The stellar models were computed by using convective overshoot distance , 0.25 and 0.40 H P . Our numerical results show that the β Cephei instability strip forms a horn-shaped region pointing upwards near the main sequence on the Hertzsprung–Russell diagram (HRD). The lower part of the instability strip for the radial modes join the zero-age main-sequence (ZAMS) at , while the top of the instability strip extends up to . The instability strip for the non-radial modes is even wider. The overall instability strip is dominated by the radial and non-radial fundamental modes. The first overtone (the radial-order index is also pulsationally unstable. We have shown that the β Cephei stability is almost independent of the overshoot parameter d over used for the stellar models, while it depends critically on the metal abundance. With decreasing metal abundance, the instability region shrinks and eventually disappears for . 相似文献
40.
卫星激光测距的新进展 总被引:6,自引:0,他引:6
扼要综述了近几年国际上卫星激光测距的进展,介绍了国内激光测距网的现状,展望了未来卫星激光测距的发展。 相似文献