首页 | 本学科首页   官方微博 | 高级检索  
文章检索
  按 检索   检索词:      
出版年份:   被引次数:   他引次数: 提示:输入*表示无穷大
  收费全文   1077篇
  免费   186篇
  国内免费   141篇
测绘学   5篇
大气科学   19篇
地球物理   209篇
地质学   873篇
海洋学   101篇
天文学   57篇
综合类   24篇
自然地理   116篇
  2024年   1篇
  2023年   8篇
  2022年   27篇
  2021年   41篇
  2020年   22篇
  2019年   45篇
  2018年   38篇
  2017年   18篇
  2016年   33篇
  2015年   34篇
  2014年   51篇
  2013年   87篇
  2012年   89篇
  2011年   62篇
  2010年   46篇
  2009年   67篇
  2008年   69篇
  2007年   63篇
  2006年   71篇
  2005年   53篇
  2004年   52篇
  2003年   43篇
  2002年   32篇
  2001年   36篇
  2000年   78篇
  1999年   27篇
  1998年   30篇
  1997年   22篇
  1996年   14篇
  1995年   27篇
  1994年   23篇
  1993年   22篇
  1992年   11篇
  1991年   21篇
  1990年   10篇
  1989年   7篇
  1988年   6篇
  1987年   7篇
  1986年   4篇
  1984年   1篇
  1983年   1篇
  1981年   1篇
  1971年   1篇
  1875年   2篇
  1872年   1篇
排序方式: 共有1404条查询结果,搜索用时 31 毫秒
1.
The uv-faceting imaging is one of the widely used large field of view imaging technologies, and will be adopted for the data processing of the low-frequency array in the first stage of the Square Kilometre Array (SKA1). Due to the scale of the raw data of SKA1 is unprecedentedly large, the efficiency of data processing directly using the original uv-faceting imaging will be very low. Therefore, a uv-faceting imaging algorithm based on the MPI (Message Passing Interface)+OpenMP (Open Multi-Processing) and a uv-faceting imaging algorithm based on the MPI+CUDA (Compute Unified Device Architecture) are proposed. The most time-consuming data reading and gridding in the algorithm are optimized in parallel. The verification results show that the results of the proposed two algorithms are basically consistent with that obtained by the current mainstream data processing software CASA (Common Astronomy Software Applications), which indicates that the proposed two algorithms are basically correct. Further analysis of the accuracy and total running time shows that the MPI+CUDA method is better than the MPI+OpenMP method in both the correctness rate and running speed. The performance test results show that the proposed algorithms are effective and have certain extensibility.  相似文献   
2.
商志文  李建芬  姜兴钰  李琰  王宏 《地质学报》2020,94(8):2433-2445
大凌河河口地区LZK06孔40m以浅岩心的沉积学、古生物学和年代学等综合研究以及该地区LZK02- 04钻孔资料,揭示了研究区中更新世晚期以来经历了两次海侵- 海退旋回,依次形成了中更新世晚期湖相/河流相 SymbolnB@ 晚更新世海相- 湖相/河流相 SymbolnB@ 全新世海相- 河流相地层。全新世早中期由于物源供给很少,研究区处于长达约10ka的饥饿滞留相沉积环境,平均沉积速率仅约0. 02~0. 05cm/a。全新世晚期约1500a cal BP以来,由于人类活动导致水土流失,河流输砂量增加,研究区开始了快速加积过程,平均沉积速率约0. 9~1. 2cm/a,下辽河平原被快速充填,开始成陆。与全球海面变化时空分布特征的对比,推断辽东湾的第II海相层发育于MIS 5- MIS 3早期,第I海相层发育于MIS 1阶段高海面时期。晚更新世以来频繁的海面升降是辽东湾泥质海岸带地层和环境演化的主要控制因素。  相似文献   
3.
AST3-2 (the second Antarctic Survey Telescope) is located in Antarctic Dome A, the loftiest ice dome on the Antarctic Plateau. It produces a huge amount of observational data which require a more efficient data reduction program to be developed. Also the data transmission in Antarctica is much difficult, thus it is necessary to perform data reduction and detect variable and transient sources remotely and automatically in Antarctica, but this attempt is restricted by the unsatisfactory performance of the low power consumption computer in Antarctica. For realizing this purpose, to develop a new method based on the existing image subtraction method and random forest algorithm, taking the AST3-2 2016 dataset as the test sample, becomes an alternative choice. This method performs image subtraction on the dataset, then applies the principle component analysis to extract the features of residual images. Random forest is used as a machine learning classifier, and in the test a recall rate of 97% is resulted for the positive sample. Our work has verified the feasibility and accuracy of this method, and finally found out a batch of candidates for variable stars in the AST3-2 2016 dataset.  相似文献   
4.
嫩江断裂带是松辽盆地的西边界断裂,但受第四系强覆盖等研究条件的限制,前人对该断裂第四纪构造活动的研究较少。本文针对该断裂带北段开展了野外地质调查,并综合大地电磁测深和纵波速度结构等结果,初步研究了嫩江断裂带北段的第四纪活动特征。调查发现,该断裂北段主要发育地貌陡坎、基岩滑坡、地层揉皱变形、近垂直擦痕、基岩崩塌与线性断塞塘等特征。探槽古地震研究揭示断裂带北段在(80.9±4.6)—(62.9±2.3)ka BP曾发生1次古地震事件,运动方式为正断,垂直位移量约1.5m,震级约为MS 7.1—7.3,断裂在晚更新世曾发生过强烈活动。研究结果有助于认识了解该断裂和松辽盆地的第四纪构造变形过程,并为评价该断裂及邻区的地震活动潜势提供参考。  相似文献   
5.
宁夏红寺堡盆地萨拉乌苏组地层时代重新厘定及意义   总被引:1,自引:1,他引:0  
以沉积旋回划分为基础,采用光释光和碳十四测年技术手段,将宁夏红寺堡盆地上更新统地层时代进行了重新划分与厘定。研究结果将红寺堡盆地原定为萨拉乌苏组的湖相沉积解体为上下两套,下部湖相沉积即为传统意义上的萨拉乌苏组,上部湖相沉积结合区域地层对比结果将其重新划归为水洞沟组,总体上反映了晚更新世青藏高原东北缘发育的两期重要的古大湖事件。在深海大洋氧同位素曲线上这两期古大湖事件分别相当于MIS3与MIS5段,代表了区域上两期温暖湿润的气候环境,也与该时期全球古气候环境的变迁基本一致。同时,在这两期古大湖发育期间,存在一期重要的构造隆升事件,表现为两套地层之间存在明显的区域不整合接触,可能是青藏高原晚更新世强烈隆升的响应。因此,针对青藏高原东北缘上更新统萨拉乌苏组湖相沉积层开展系统的年代学研究,对其地层时代进行重新划分与厘定,对于研究晚更新世古大湖形成与演化、古气候变迁以及青藏高原的隆升提供了重要的地质背景资料。  相似文献   
6.
Two photometric follow-up transit (primary eclipse) observations on WASP-43 b and four observations on TrES-3 b are performed using the Xuyi Near-Earth Object Survey Telescope. After differential photometry and light curve analysis, the physical parameters of the two systems are obtained and are in good match with the literature. Combining with transit data from a lot of literature, the residuals (O ? C) of transit observations of both systems are fitted with the linear and quadratic functions. With the linear fitting, the periods and transit timing variations (TTVs) of the planets are obtained, and no obvious periodic TTV signal is found in both systems after an analysis. The maximum mass of a perturbing planet located at the 1:2 mean motion resonance (MMR) for WASP-43 b and TrES-3 b is estimated to be 1.826 and 1.504 Earth mass, respectively. By quadratic fitting, it is confirmed that WASP-43 b may have a long-term TTV which means an orbital decay. The decay rate is shown to be P? = (?0.005248 ± 0.001714) s·yr?1, and compared with the previous results. Based on this, the lower limit of the stellar tidal quality parameter of WASP-43 is calculated to be Q*1.5×105, and the remaining lifetimes of the planets are presented for the different Q* values of the two systems, correspondingly.  相似文献   
7.
This paper discusses the results of the investigation of Pleistocene sediments at the Royal Oak Portal (ROP) site on the new Crossrail scheme near Paddington Station, London. The site was sampled and recorded in May 2011 by archaeologists from Oxford Archaeology commissioned by Crossrail Ltd. The investigation revealed a sedimentary sequence associated with cool climate waterlain deposition towards the edge of the River Westbourne floodplain. During excavation an assemblage of around 100 identifiable large mammal bones was recovered, dating to the Late Pleistocene. The major concentration of bones, from bison and reindeer, was located and excavated from a shallow sequence of sediments. Analysis of the bones indicates that they represent a natural death assemblage, scavenged and subsequently disarticulated, transported by water, exposed and further dispersed and broken by trampling. The site is of regional and national importance because the assemblage derives from a well-constrained geological context, with associated dating evidence suggesting accumulation during the later parts of Marine Isotope Stage (MIS) 5 and continuing within MIS 4. The site is also of significance because it is one of a growing number of recently discovered sites away from the main fluvial archive for the British Middle and Upper Pleistocene. These sites have the potential to add significantly to our understanding of parts of the Pleistocene record that remain difficult to document through the investigation of the more active systems associated with major rivers such as the Thames, Severn or Trent.  相似文献   
8.
在具有相同储集砂体和相似断层输导情况下,牛庄洼陷沙三中亚段砂岩体油藏长期存在以下难以解释的现象:1)现今砂岩孔隙度分布与油气分布不一致,高孔隙砂岩不含油而低孔隙砂岩含油;2)相同物性砂岩有的含油而有的不含油,含油砂体现今物性接近,但含油级别却存在很大差异。本文从古孔隙度恢复方面分析了牛庄洼陷西部地区沙三中砂岩储层在成藏期的储集条件,并探讨了成藏期储层临界孔隙度。研究发现:1)虽然现今储层物性下限很低,部分砂岩已经致密化,但成藏期的古孔隙度分布在18%~25%范围内,远大于成藏期临界孔隙度13.9%。但由于埋藏过程的差异导致砂岩储层后期减孔幅度不同,因而现今储层物性不能反映成藏期储层物性,成藏期孔隙度高并不能代表现今孔隙度高;2)成藏期高孔隙度带与现今油气分布范围高度一致,表明在相似断层输导条件下,由于储层物性级差优势形成油气优势运移通道,导致高孔隙度带砂体含油,因此,沙三中亚段岩性油藏富集在成藏期高孔隙带中,成藏期砂岩古孔隙度是油气成藏的重要控制因素,而现今砂岩储层高孔隙带在成藏期并不一定高。牛庄洼陷西部地区沙三中亚段储层中具有高古孔隙度的砂岩仍有较大勘探潜力。  相似文献   
9.
Geological maps of South Carolina, covering > 6800 km2, confirm the existence of eight preserved Pleistocene shorelines above current sea level: Marietta (+ 42.6 m), Wicomico (+ 27.4 m), Penholoway (+ 21.3 m), Ladson (+ 17.4 m), Ten Mile Hill (+ 10.7 m), Pamlico (+ 6.7 m), Princess Anne (+ 5.2 m), and Silver Bluff (+ 3 m). Current geochronologic data suggest that these eight shorelines correlate with Marine Oxygen Isotope Stages (MIS) as follows: Marietta—older than MIS 77; Wicomico—MIS 55–45; Penholoway—MIS 19 or 17; Ladson—MIS 11; Ten Mile Hill—MIS 7; Pamlico—MIS 5; Princess Anne—MIS 5; and Silver Bluff—MIS 5 or 3. Except for the MIS 5e Pamlico, and possibly the MIS 11 Ladson, the South Carolina elevations are higher than predicted by isotope proxy-based reconstructions. The < 4 m of total relief from the Pamlico to the Silver Bluff shoreline in South Carolina, for which other reconstructions suggest an expected relief of ~ 80 m, illustrates the lack of match. Our results suggest that processes affecting either post-depositional changes in shoreline elevations or the creation of proxy sea-level estimates must be considered before using paleo sea-level position on continental margins.  相似文献   
10.
In situ Pleistocene reefs form a gently sloping nearshore terrace around the island of Oahu. TIMS Th–U ages of in situ corals indicate that most of the terrace is composed of reefal limestones correlating to Marine Oxygen Isotope Stage 7 (MIS 7, ~ 190–245 ka). The position of the in situ MIS 7 reef complex indicates that it formed during periods when local sea level was ~ 9 to 20 m below present sea level. Its extensiveness and geomorphic prominence as well as a paucity of emergent in situ MIS 7 reef-framework deposits on Oahu suggest that much of MIS 7 was characterized by regional sea levels below present. Later accretion along the seaward front of the terrace occurred during the latter part of MIS 5 (i.e., MIS 5a–5d, ~ 76–113 ka). The position of the late MIS 5 reefal limestones is consistent with formation during a period when local sea level was below present. The extensiveness of the submerged Pleistocene reefs around Oahu compared to the relative dearth of Holocene accretion is due to the fact that Pleistocene reefs had both more time and more accommodation space available for accretion than their Holocene counterparts.  相似文献   
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号