全文获取类型
收费全文 | 67302篇 |
免费 | 17267篇 |
国内免费 | 20864篇 |
专业分类
测绘学 | 10645篇 |
大气科学 | 9513篇 |
地球物理 | 12583篇 |
地质学 | 43242篇 |
海洋学 | 12296篇 |
天文学 | 2428篇 |
综合类 | 5425篇 |
自然地理 | 9301篇 |
出版年
2024年 | 294篇 |
2023年 | 1420篇 |
2022年 | 3862篇 |
2021年 | 4671篇 |
2020年 | 3941篇 |
2019年 | 4216篇 |
2018年 | 4385篇 |
2017年 | 4171篇 |
2016年 | 4074篇 |
2015年 | 4517篇 |
2014年 | 4600篇 |
2013年 | 5561篇 |
2012年 | 5969篇 |
2011年 | 6088篇 |
2010年 | 5954篇 |
2009年 | 5491篇 |
2008年 | 5618篇 |
2007年 | 5368篇 |
2006年 | 5062篇 |
2005年 | 4075篇 |
2004年 | 3136篇 |
2003年 | 2257篇 |
2002年 | 2300篇 |
2001年 | 2105篇 |
2000年 | 1723篇 |
1999年 | 968篇 |
1998年 | 485篇 |
1997年 | 416篇 |
1996年 | 341篇 |
1995年 | 313篇 |
1994年 | 277篇 |
1993年 | 225篇 |
1992年 | 220篇 |
1991年 | 134篇 |
1990年 | 145篇 |
1989年 | 124篇 |
1988年 | 86篇 |
1987年 | 82篇 |
1986年 | 83篇 |
1985年 | 67篇 |
1984年 | 71篇 |
1983年 | 59篇 |
1982年 | 53篇 |
1981年 | 35篇 |
1980年 | 26篇 |
1979年 | 52篇 |
1978年 | 27篇 |
1977年 | 25篇 |
1975年 | 27篇 |
1954年 | 34篇 |
排序方式: 共有10000条查询结果,搜索用时 31 毫秒
1.
In this work,we studied the variable stars in the open cluster NGC 1912 based on the photometric observations and Gaia DR2 data.More than 3600 CCD frames in B,V,R filters were reduced,and we obtained the light curves that span about 63 hours.By analyzing these light curves,we detected 24 variable stars,including 16 periodic variable stars,seven eclipsing binaries and one star whose type is unclear.Among these 24 variable stars,11 are newly discovered,which are classified as sixγDoradus stars,oneδScuti star,three detached binaries and one contact binary.We also confirmed 13 previously known variable stars.Based on cluster members identified by Cantat-Gaudin et al.(2018),we inferred cluster memberships for these detected variable stars.Using Gaia DR2 data,we plotted a new color-magnitude diagram for NGC1912,and showed the nature of variable cluster members in kinematical properties and heliocentric distance.Among the 24 variable stars,seven variables are probable cluster members,which show homogeneity in kinematic characters and space position with the established cluster members.Four of the seven variable cluster members are the previously discovered stars,consisting of twoγDor stars and twoδSct stars.The remaining three variable cluster members,which are allγDor stars,are firstly detected in this work.The main physical parameters of these variable cluster members estimated from the color-magnitude diagram are log(age/yr)=8.75,[Fe/H]=-0.1,m-M=10.03 mag,and E(B-V)=0.307. 相似文献
2.
Large dams and reservoirs alter not only the natural flow regimes of streams and rivers but also their flooding cycles and flood magnitudes. Although the effect of dams and reservoirs has been reported for some vulnerable locations, the understanding of the inner-basin variation with respect to the effects remains limited. In this study, we analyse the Three Gorges Dam (TGD) built on the Changjiang mainstream (Yangtze River) to investigate the dam effect variations in the system of interconnected water bodies located downstream. We investigated the effect of flow alterations along the downstream river network using discharge time series at different gauging stations. The river–lake interactions (referring to the interactions between the Changjiang mainstream and its tributary lakes i.e. the Dongting and Poyang lakes) and their roles in modifying the TGD effect intensity were also investigated in the large-scale river–lake system. The results show that the water storage of the tributary lakes decreased after the activation of the TGD. Severe droughts occurred in the lakes, weakening their ability to recharge the Changjiang mainstream. As a consequence, the effect of the TGD on the Changjiang flow increase during the dry season diminished quickly downstream of the dam, whereas its impact on the flow decrease during the wet season gradually exacerbated along the mainstream, especially at sites located downstream of the lake outlets. Therefore, when assessing dam-induced hydrological changes, special attention should be paid to the changes in the storage of tributary lakes and the associated effects in the mainstream. This is of high importance for managing the water resource trade-offs between different water bodies in dam-affected riverine systems. 相似文献
3.
巡天观测与高能物理、黑洞天文等领域均有密切的联系.基于星系-超新星二分类问题,研究光谱数据预处理,结合余弦相似度改善PCA(Principal Component Analysis)光谱分解特征提取方法,用SDSS(the Sloan Digital Sky Survey)、WISeREP(the Weizmann Interactive Supernova data REPository)组成的5620条光谱数据集训练支持向量机,可以得到0.498%泛化误差的识别模型和新样本分类概率.使用Neyman-Pearson决策方法建立NPSVM(Neyman-Pearson Support Vector Machine)模型可进一步降低超新星的漏判率. 相似文献
4.
基于采自冲绳海槽中部的CS2站柱状沉积物黏土矿物和AMS14C年代分析,探讨了末次冰消期以来冲绳海槽中部黏土矿物的物质来源及其环境指示意义。结果显示,CS2站黏土矿物以伊利石为主,其次为绿泥石,高岭石和蒙脱石含量较少。根据黏土矿物分布趋势变化,CS2站柱状沉积物可划分为3个阶段:阶段(I 19~12 ka BP)和阶段Ⅱ (12~8 ka BP)期间沉积物主要来源于长江,台湾和黄河物质也有一定影响,其物质来源主要受海平面升降的控制;阶段Ⅲ(8~0 ka BP)主要来源于长江和台湾,黄河贡献有限,主要受黑潮演化的影响。CS2站(蒙脱石+高岭石) (/伊利石+绿泥石)比值可以作为东亚季风演化的矿物学指标,指标变化显示出东亚冬季风强度相对夏季风的强度在16.4~14.8 ka BP和12.8~11.6 ka BP期间有两次显著的加强,指示当时气候相对寒冷干燥,结果可以与格陵兰冰心δ18O和三宝洞δ18O记录等很好对比。 相似文献
5.
随着我国煤炭资源去产能整合煤矿的增多,复采工作面临空窄煤柱采动失稳问题日益凸显,已严重制约矿井安全高效生产。为此,针对辛安煤矿复采1402工作面辅运巷道5号钻场临空窄煤柱稳定性控制的工程难题,运用数值模拟与理论分析相结合的方法,探究5号钻场临空窄煤柱稳定性采掘扰动响应特征,提出5号钻场临空窄煤柱动态注浆加固技术方案并开展现场应用和效果检验。研究结果表明:1402工作面辅运巷道掘进对5号钻场临空窄煤柱稳定性影响较小;在1402工作面回采期间,距5号钻场18~6 m范围,临空窄煤柱集中垂直应力由非对称马鞍形分布逐渐过渡为拱形分布;距5号钻场6 m时,临空窄煤柱承载叠加垂直应力超过煤体强度,塑性区完全贯通,极易破坏失稳;现场采用MP364型注浆材料及专用注浆设备对5号钻场临空窄煤柱前后5 m区域进行加固,动态注浆始终超前工作面10 m,通过深孔窥视和气体监测手段验证临空窄煤柱良好的封堵固化效果,保障了工作面安全回采,为我国整合矿井类似条件下煤柱稳定性控制提供借鉴和参考。移动阅读 相似文献
7.
以线性粘滞阻尼器加固剪切型规则框架结构为研究对象,基于能量原理提出附加阻尼系数正比于层间位移平方的分配方式。以六层和十二层钢筋混凝土框架为例,以确保结构在中震时保持弹性状态为设计目标,分别采用附加阻尼系数正比于层间位移平方的分配方式以及现有的分配方式,对结构进行消能减震设计。计算结果表明:有控结构均满足中震不坏的要求,层间位移角限值均未超过1/550,减震效果良好;附加阻尼系数正比于层间位移平方的分配方式得出的总阻尼系数最小,为最经济的设计结果。 相似文献
8.
9.
Groundwater exploitation has been regarded as the main reason for land subsidence in China and thus receives considerable attention from the government and the academic community.Recently,building loads have been identified as another important factor of land subsidence,but researches in this sector have lagged.The effect of a single building load on land subsidence was neglected in many cases owing to the narrow scope and the limited depth of the additional stress in stratum.However,due to the superposition of stresses between buildings,the additional stress of cluster loads is greater than that of a single building load under the same condition,so that the land subsidence caused by cluster loads cannot be neglected.Taking Shamen village in the north of Zhengzhou,China,as an example,a finite-difference model based on the Biot consolidation theory to calculate the land subsidence caused by cluster loads was established in this paper.Cluster loads present the characteristics of large-area loads,and the land subsidence caused by cluster loads can have multiple primary consolidation processes due to the stress superposition of different buildings was shown by the simulation results.Pore water migration distances are longer when the cluster loads with high plot ratio are imposed,so that consolidation takes longer time.The higher the plot ratio is,the deeper the effective deformation is,and thus the greater the land subsidence is.A higher plot ratio also increases the contribution that the deeper stratigraphic layers make to land subsidence.Contrary to the calculated results of land subsidence caused by cluster loads and groundwater recession,the percentage of settlement caused by cluster loads in the total settlement was 49.43%and 55.06%at two simulated monitoring points,respectively.These data suggest that the cluster loads can be one of the main causes of land subsidence. 相似文献
10.
老金厂金矿床是北山成矿南带最具代表性的中低温岩浆热液型金矿床之一,其规模为中型。依据脉体穿插、矿物共生组合和矿石结构构造等特征,将矿床矿化作用过程划分为石英-黄铁矿阶段(Ⅰ)、石英-含砷黄铁矿-毒砂阶段(Ⅱ)、石英-黄铁矿-多金属硫化物阶段(Ⅲ)和石英-方解石阶段(Ⅳ)。利用电子探针研究了不同成矿阶段载金矿物的元素组成及其分布规律。Ⅰ阶段:黄铁矿以粗粒自形立方体为主,粒度为0.50~1.50 mm,贫As、Au;毒砂含量极少,呈细粒他形。Ⅱ阶段:含砷黄铁矿周围常有大量毒砂产出,含砷黄铁矿多为立方体、五角十二面体,粒度为0.30~1.00 mm,富As、Au;该阶段矿化最为强烈,毒砂主要形成于此时期,多呈棱柱状、柱状、放射状集合体,显示富S亏As特征。Ⅲ阶段:多以黄铁矿-黄铜矿-闪锌矿共生组合脉的形式产出,黄铁矿多呈长条状,以富S、Cu、Zn、Au和贫Fe、As为特征。Ⅳ阶段:矿化作用极弱,毒砂、黄铁矿含量极少,为细粒他形。原位硫同位素组成显示:Ⅰ阶段黄铁矿δ34SV-CDT值为-3.8‰~-2.9‰,均值为-3.3‰;Ⅱ阶段黄铁矿和毒砂δ34SV-CDT值为-4.7‰~2.6‰,均值为-3.3‰;Ⅲ阶段黄铁矿和闪锌矿δ34SV-CDT值主要分布于-1.9‰~1.0‰之间,均值为0.1‰。此3个阶段硫同位素组成反映了成矿期硫主要来源于幔源岩浆,混入了部分地层硫。综合前人研究成果,认为成矿早期至晚期,成矿流体总体上由富S贫As向富As贫S演化。Ⅰ阶段体系处于中性稳定的环境,硫源充足;Ⅱ阶段为贫S富As的高氧逸度环境,由于大气降水对地层的淋滤渗透,混入富As流体,Au可能与As结合形成Au-As络合物,在成矿有利部位富集沉淀;Ⅲ阶段成矿元素种类丰富,体系为富S贫As的弱还原环境,Au很可能与HS-、S-形成络合物进入黄铁矿晶格。 相似文献