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   144篇
  免费   22篇
  国内免费   31篇
测绘学   1篇
地球物理   22篇
地质学   157篇
海洋学   2篇
天文学   7篇
综合类   3篇
自然地理   5篇
  2023年   1篇
  2022年   5篇
  2021年   5篇
  2020年   4篇
  2019年   3篇
  2018年   2篇
  2017年   5篇
  2016年   13篇
  2015年   7篇
  2014年   7篇
  2013年   5篇
  2012年   5篇
  2011年   7篇
  2010年   8篇
  2009年   8篇
  2008年   5篇
  2007年   5篇
  2006年   7篇
  2005年   4篇
  2004年   6篇
  2003年   4篇
  2002年   2篇
  2001年   11篇
  2000年   17篇
  1999年   7篇
  1998年   3篇
  1997年   1篇
  1996年   1篇
  1995年   17篇
  1994年   12篇
  1993年   1篇
  1992年   4篇
  1990年   3篇
  1984年   1篇
  1983年   1篇
排序方式: 共有197条查询结果,搜索用时 484 毫秒
181.
YQ0902孔位于浙江南部瓯江三角洲南侧温瑞平原上。沉积相、粒度分析以及AMS 14C测年数据表明,硬土层之下为海洋氧同位素3阶段(MIS 3)形成的潟湖相沉积,据此推测MIS 3高海平面至少达到现今海平面之下30m左右(未经构造升降和沉积物压实作用等影响的校正,下同)。硬土层的成土过程发生于MIS 2,其母质部分为MIS 3的潟湖沉积,部分为河漫滩沉积。硬土层之上是一套形成于全新世的海侵—海退旋回,与长江三角洲南翼前缘的沉积相组合类似。研究钻孔初始海泛面约形成于9 cal ka BP,推算当时的海平面约低于现今海平面25 m。中全新世最大海侵前后,东亚季风较强,通过径流或沿岸流输入本区的沉积物较充足,沉积速率较大。随着海平面相对稳定或略有下降,东亚季风减弱,可容空间减小,中晚全新世(5~2 cal ka BP)沉积速率较低。高分辨率的XRF岩心扫描获得的元素相对含量是古环境与古气候研究的重要指标,其中Cl/Ti、Fe/Ti值可分别作为海相性(与海洋联通程度)与东亚季风强弱的替代指标。  相似文献   
182.
Computer aided multi-parameter signal correlation is used to develop a common high-precision age model for eight gravity cores from the subtropical and subantarctic South Atlantic. Since correlations between all pairs of multi-parameter sequences are used, and correlation errors between core pairs (A, B) and (B, C) are controlled by comparison with (A, C), the resulting age model is called a stratigraphic network. Precise inter-core correlation is achieved using high-resolution records of magnetic susceptibility κ, wet bulk density ρ and X-ray fluorescence scans of elemental composition. Additional δ18O records are available for two cores. The data indicate nearly undisturbed sediment series and the absence of significant hiatuses or turbidites. After establishing a high-precision common depth scale by synchronously correlating four densely measured parameters (Fe, Ca, κ, ρ), the final age model is obtained by simultaneously fitting the aligned δ18O and κ records of the stratigraphic network to orbitally tuned oxygen isotope [J. Imbrie, J. D. Hays, D. G. Martinson, A. McIntyre, A. C. Mix, J. J. Morley, N. G. Pisias, W. L. Prell, N. J. Shackleton, The orbital theory of Pleistocene climate: support from a revised chronology of the marine δ18O record, in: A. Berger, J. Imbrie, J. Hays, G. Kukla, B. Saltzman (Eds.), Milankovitch and Climate: Understanding the Response to Orbital Forcing, Reidel Publishing, Dordrecht, 1984, pp. 269-305; D. Martinson, N. Pisias, J. Hays, J. Imbrie, T. C. Moore Jr., N. Shackleton, Age dating and the orbital theory of the Ice Ages: development of a high-resolution 0 to 300.000-Year chronostratigraphy, Quat. Res. 27 (1987) 1-29.] or susceptibility stacks [T. von Dobeneck, F.Schmieder, Using rock magnetic proxy records for orbital tuning and extended time series analyses into the super-and sub-Milankovitch Bands, in: G. Fischer, G. Wefer (Eds.), Use of proxies in paleoceanography: Examples from the South Atlantic, Springer-Verlag, Berlin (1999), pp. 601-633.]. Besides the detection and elimination of errors in single records, the stratigraphic network approach allows to check the intrinsic consistency of the final result by comparing it to the outcome of more restricted alignment procedures. The final South Atlantic stratigraphic network covers the last 400 kyr south and the last 1200 kyr north of the Subtropical Front (STF) and provides a highly precise age model across the STF representing extremely different sedimentary regimes. This allows to detect temporal shifts of the STF by mapping δMn / Fe. It turns out that the apparent STF movements by about 200 km are not directly related to marine oxygen isotope stages.  相似文献   
183.
These mature analytical techniques do not show any change in publication level from the previous two years and AAS remains dominant in terms of the number of publications. The last two years have seen fewer technical improvements than in the previous review period. Some interesting papers dealing with uncertainty and quality assurance in INAA were published during 2006–2007. It is suggested that photon activation should be reconsidered because the source of electron accelerators has recently improved. A technique to preconcentrate Se for INAA determination has also been proposed. In the case of AAS, papers on analyte preconcentration continue to be more abundant than those relating to instrumental modification. Sample preparation for AAS is also active and ultrasound‐assisted leaching shows some promising applications. There were an unusual number of reviews concerned with AAS and those important to geological samples are cited here. A technique to preconcentrate Cr in water is presented and a new device to determine As and Se is showing some potential uses. Confocal X‐ray mapping continues to show interesting developments. One group developed a technique to perform XRF inside an oyster and an interesting application of μ‐XRF mapping of sediments is presented. Determination of platinum‐group elements (at μg g1 concentrations) can be carried out very quickly with an improved XRF technique.  相似文献   
184.
Geochemical reference materials (RMs) for microbeam techniques are typically characterised by averages and dispersion statistics (e.g., standard deviation, variance) that are calculated for a number of measurements (beam shots). It is proposed that the mapping of RMs will add spatial information that better characterises the grouping and magnitudes of the heterogeneities and provides the information necessary to define a minimum analytical mass. A simple mathematical solution is proposed, which can be easily computed and understood. The analogous notions to sill and range from geostatistics are applied to the minimum analytical mass versus the relative standard deviation. To assess grouping and magnitudes of the heterogeneities, a ‘proximity number’ is computed for each average value ± ‘n’ standard deviations (magnitude). Different chemical anomalies have been simulated to demonstrate the behaviour of the proximity number. To further test the proposed spatial geochemistry concept, sulfide‐ and oxide‐bearing RMs have been selected because many are crippled with nugget effect. They have been mapped with a micro‐XRF apparatus, and results are presented for CHR‐Bkg, CHR‐Pt+, MASS‐1, MASS‐3, WMS‐1 and WMS‐1a. MASS‐1 and MASS‐3 are the most suitable RMs for microbeam techniques. Spatial geochemistry offers a new approach to better characterise reference materials.  相似文献   
185.
利用常规宝石学测试、X射线荧光光谱仪(XRF)、激光诱导离解光谱仪(LIBS)、电子探针(EPMA)对近来在珠宝市场上的铅玻璃充填碧玺样品进行测试与分析,旨在探讨其鉴定特征。结果表明,该铅玻璃充填样品的充填特征不明显,与传统的有机物充填处理方法不同;X射线荧光光谱和激光诱导离解光谱的测试结果显示,该铅玻璃充填碧玺样品具有明显的Pb峰。铅玻璃充填碧玺样品中充填物的电子探针二次电子像及背散射电子像特征,可作为碧玺样品是否经过了铅玻璃充填的诊断性依据,其充填物的化学成分主要为Si和Pb,呈不规则斑块状分布于裂隙中。  相似文献   
186.
安徽张八岭构造带石英脉型金矿成矿流体来源研究   总被引:6,自引:1,他引:6  
对安徽张八岭构造带石英脉型金矿石英流体包裹体温度、成分和氢、氧同位素进行了研究,对成矿流体来源进行了探讨。研究表明,区内石英脉型金矿具有两类成矿流体,一类为中生代大气降水与经历水/岩交换的演化岩浆水的混合;另一类为中生代大气降水与原始岩浆水的混合。  相似文献   
187.
X射线荧光方法在矿区环境地球化学研究中的应用   总被引:1,自引:0,他引:1  
采用白行研制的高灵敏度能量色散X射线荧光分析仪分析了攀枝花矿区水系沉积物中微量元素的浓度,并根据分析结果研究了矿区元素分布的地球化学特征,本项研究的主要目的是探讨X射线荧光分析技术在矿区环境地球化学研究中的可行性,探索矿区环境地球化学研究的方法技术.结果表明,XRF方法可以有效分析沉积物中元素的含量,进而进行环境地球化学研究.  相似文献   
188.
x射线荧光光谱无标半定量分析稀土元素方法的改进   总被引:5,自引:1,他引:5       下载免费PDF全文
在Philips公司提供的x射线荧光光谱基本参数法半定量分析的SemIQ软件基础上引入重稀土元素的分析,用光谱纯的稀土氧化物与四硼酸锂熔融制备标样,重新建立一套半定量分析方法,使原软件不能分析的Dy、Ho、Er元素也可进行半定量分析,并提高了Eu、Gd、Tb、Tm、Yb、Lu元素分析的准确度。应用该方法进行了大量稀土样品的半定量分析,并与原软件方法对照,结果明显改善。  相似文献   
189.
六棱山北麓断裂新活动特征   总被引:6,自引:1,他引:6  
段瑞涛  方仲景 《地震地质》1995,17(3):207-213
通过对六棱山北麓活动断裂的几何结构、分段活动特征及段落边界等方面的地质地貌调查与研究,认为该活动断裂可分为4段,除东段在早更新世有过活动外,其他3段均为晚更新世晚期~全新世活动段,段落长度10~39km。该断裂在晚中生代表现为逆冲性质,至新生代随区域构造应力场的变化而转变为倾滑正断层。各段落上垂直位移量分布呈包络线状,而且各段平均滑动速率不同,西大东小,显示断裂新活动强度自西向东变弱  相似文献   
190.
This paper reviews research on coprolites from India, providing the first evidence of microcoprolites from the early Miocene (Aquitanian) Khari Nadi Formation sedimentary succession, exposed about 1.5 km northeast of the village of Kotada, Kachchh (Kutch) District, Gujarat State, western India. Morphometric and size comparisons (in a statistical framework) with known coprolites from the Mesozoic-Cenozoic successions of India (including those recorded herein) and globally suggest that fishes were the likely producers of the Kotada coprolites. Scanning electron microscopy confirms the presence of fish dental remains within the coprolites, while both Scanning Electron Microscopy (SEM) and Energy Dispersive X-ray Spectroscopy (EDS) reveal the phosphatic nature of the microscopic coprolite specimens (recorded herein) hinting that the producer(s) were predominantly carnivorous (ichthyophagous) in their diet. Furthermore, X-Ray Fluorescence (XRF) analysis of the host and associated lithologies allows us to deduce that the Kotada coprolites were deposited in a shallow marine environment, with possible aerial exposure of the host lithology occurring at some point after deposition. To the best of our knowledge, the present report is the first record of microscopic fish coprolites from India, as well as being the first from the Aquitanian of India and the oldest Neogene record from India.  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