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   4630篇
  免费   1508篇
  国内免费   1866篇
测绘学   450篇
大气科学   3340篇
地球物理   880篇
地质学   1840篇
海洋学   454篇
天文学   250篇
综合类   224篇
自然地理   566篇
  2024年   67篇
  2023年   189篇
  2022年   408篇
  2021年   516篇
  2020年   529篇
  2019年   589篇
  2018年   543篇
  2017年   655篇
  2016年   620篇
  2015年   606篇
  2014年   560篇
  2013年   442篇
  2012年   386篇
  2011年   310篇
  2010年   239篇
  2009年   286篇
  2008年   159篇
  2007年   194篇
  2006年   173篇
  2005年   82篇
  2004年   44篇
  2003年   70篇
  2002年   50篇
  2001年   36篇
  2000年   44篇
  1999年   82篇
  1998年   21篇
  1997年   16篇
  1996年   11篇
  1995年   12篇
  1994年   7篇
  1993年   8篇
  1992年   9篇
  1991年   7篇
  1990年   6篇
  1989年   8篇
  1988年   12篇
  1987年   3篇
  1986年   1篇
  1954年   4篇
排序方式: 共有8004条查询结果,搜索用时 156 毫秒
1.
2.
Prediction Test for the Two Extremely Strong Solar Storms in October 2003   总被引:2,自引:0,他引:2  
In late October and early November 2003, a series of space weather hazard events erupted in solar-terrestrial space. Aiming at two intense storm (shock) events on 28 and 29 October, this paper presents a Two-Step method, which combines synoptic analysis of space weather–`observing’ and quantitative prediction – ‘palpating’, and uses it to test predictions. In the first step, ‘observing’, on the basis of observations of the source surface magnetic field, interplanetary scintillation (IPS) and ACE spacecraft, we find that the propagation of the shock waves is asymmetric and northward relative to the normal direction of their solar sources due to the large-scale configuration of the coronal magnetic fields, and the Earth is located near the direction of the fastest speed and greatest energy of the shocks. Being two fast ejection shock events, the fast explosion of extremely high temperature and strong magnetic field, and background solar wind velocity as high as 600 and 1000 km s−1, are also helpful to their rapid propagation. According to the synoptic analysis, the shock travel times can be estimated as 21 and 20 h, which are close to the observational results of 19.97 and 19.63 h, respectively. In the second step, ‘palpating’, we adopt a new membership function of the fast shock events for the ISF method. The predicted results here show that for the onset time of the geomagnetic disturbance, the relative errors between the observational and the predicted results are 1.8 and 6.7%, which are consistent with the estimated results of the first step; and for the magnetic disturbance magnitude, the relative errors between the observational and the predicted results are 4.1 and 3.1%, respectively. Furthermore, the comparison among the predicted results of our Two-Step method with those of five other prevailing methods shows that the Two-Step method is advantageous in predicting such strong shock event. It can predict not only shock arrival time, but also the magnitude of magnetic disturbance. The results of the present paper tell us that understanding the physical features of shock propagation thoroughly is of great importance in improving the prediction efficiency.  相似文献   
3.
山区短波反射辐射的计算模式   总被引:2,自引:0,他引:2  
本文提出计算山区测点可接受到的来自周围山地的短波反射辐射日平均通量密度的通用计算机模式,并以大别山南段赵公岭山区为例进行了试验,结果表明,该式通用性强、精度较高。  相似文献   
4.
The sulfur isotopic composition of carbonate associated sulfate (CAS) has been used to investigate the geochemistry of ancient seawater sulfate. However, few studies have quantified the reliability of δ34S of CAS as a seawater sulfate proxy, especially with respect to later diagenetic overprinting. Pyrite, which typically has depleted δ34S values due to authigenic fractionation associated with bacterial sulfate reduction, is a common constituent of marine sedimentary rocks. The oxidation of pyrite, whether during diagenesis or sample preparation, could thus adversely influence the sulfur isotopic composition of CAS. Here, we report the results of CAS extractions using HCl and acetic acid with samples spiked with varying amounts of pyrite. The results show a very strong linear relationship between the abundance of fine-grained pyrite added to the sample and the resultant abundance and δ34S value of CAS. This data represents the first unequivocal evidence that pyrite is oxidized during the CAS extraction process. Our mixing models indicate that in samples with much less than 1 wt.% pyrite and relatively high δ34Spyrite values, the isotopic offset imparted by oxidation of pyrite should be much less than ? 4‰. A wealth of literature exists on the oxidation of pyrite by Fe3+ and we believe this mechanism drives the oxidation of pyrite during CAS extraction, during which the oxygen used to form sulfate is taken from H2O, not O2. Consequently, extracting CAS under anaerobic conditions would only slow, but not halt, the oxidation of pyrite. Future studies of CAS should attempt to quantify pyrite abundance and isotopic composition.  相似文献   
5.
有机饵料常规饵料对扣蟹品质的比较研究   总被引:2,自引:0,他引:2  
从扣蟹的体重、壳长、壳宽,扣蟹体内粗蛋白、氨基酸及药物残留和重金属含量等几个方面比较了在有机养殖和常规养殖模式下扣蟹的品质。结果显示,在有机养殖模式下,扣蟹的体重增长,壳长、壳宽与常规养殖差异显著(p<0.05);体内粗蛋白含量、必需氨基酸含量中,有机养殖组为55.43%、48.07%,常规养殖组为46.55%、40.64%,常规养殖组扣蟹的氨基酸含量明显低于有机饵料养殖组;在药残和重金属含量方面,除常规养殖组的六六六检出外,其余指标均符合有机蟹卫生质量地方标准(DB32/T609.3-2003),但有机养殖组的重金属含量则远较常规养殖组低。  相似文献   
6.
摘要: 近年国际上相控阵技术在大气探测领域中的应用有了重要进展,成为雷达气象学研究的又一新热点,并可能成为今后天气雷达发展的重要方向。介绍了相控阵技术在大气探测中应用现状和研究进展,以及近年在气象应用中所获得的最新研究结果,展望了相控阵技术的应用前景,进一步讨论了开展相控阵技术研究所面临的技术挑战和未来发展的方向。为我国开展相控阵天气雷达的研制提供参考。  相似文献   
7.
近50年来中国六大流域径流年内分配变化趋势   总被引:16,自引:0,他引:16       下载免费PDF全文
基于1950年以来的全国六大流域19个重点控制水文站实测月径流量观测资料,以1980年为界,分析各站实测径流量年内分配不均匀系数、集中度以及集中期的变化;采用Mann-Kendall非参数统计检验方法,诊断了各月径流量的变化趋势。结果表明,自1980年以来,全国六大流域的月径流发生了时空变化,除海河的石匣里、响水堡站和黄河花园口站年内径流不均匀性和相对集中度较小以外,其它站的年内径流不均匀性和相对集中度较大,以松辽流域为最大;此外,南方流域各站冬春季(12~3月)的径流均呈现增加的趋势,5月份呈现减少的趋势,7月份呈现增加的趋势;北方流域各站冬春季(1~5月)径流呈现减少的趋势,以海河流域各站、松辽的铁岭、黄河利津站和淮河的吴家渡站减少趋势最为严重。  相似文献   
8.
We investigate, via a two-dimensional (nonplanar) MHD simulation, a situation wherein a bipolar magnetic field embedded in a stratified solar atmosphere (i.e., arch-filament-like structure) undergoes symmetrical shear motion at the footpoints. It was found that the vertical plasma flow velocities grow exponentially leading to a new type of global MHD-instability that could be characterized as a Dynamic Shearing Instability, with a growth rate of about 8{ovV} A a, where {ovV} A is the average Alfvén speed and a –1 is the characteristic length scale. The growth rate grows almost linearly until it reaches the same order of magnitude as the Alfvén speed. Then a nonlinear MHD instability occurs beyond this point. This simulation indicates the following physical consequences: the central loops are pinched by opposing Lorentz forces, and the outer closed loops stretch upward with the vertically-rising mass flow. This instability may apply to arch filament eruptions (AFE) and coronal mass ejections (CMEs).To illustrate the nonlinear dynamical shearing instability, a numerical example is given for three different values of the plasma beta that span several orders of magnitude. The numerical results were analyzed using a linearized asymptotic approach in which an analytical approximate solution for velocity growth is presented. Finally, this theoretical model is applied to describe the arch filament eruption as well as CMEs.  相似文献   
9.
《Chemical Geology》2006,225(1-2):137-155
Carbon stable isotopes from carbonate minerals (mainly dolomite) from six wells from the Lower Triassic Sherwood Sandstones of the Corrib Gas Field, Slyne Basin, west of Ireland, allow stratigraphic correlation. The results also provide information on palaeoenvironmental change during the deposition of these continental redbed sedimentary rocks. The Triassic reservoir rocks have been buried to > 4000 m and heated to > 165 °C and now contain methane-rich gas. Although the oxygen isotopic signal has been at least partially reset during burial and heating, a primary carbon isotopic signal appears to have survived diagenesis. The carbon isotope ratio varies from − 3.2‰ to + 2.1‰. All six wells show similar stratigraphic changes when all the carbon isotope data are plotted relative to a major playa horizon. δ13C increases from about − 3‰ at the base of the Sherwood to about + 2‰ 170 m above the base. δ13C then decreases to about − 2‰ for the next 70 m and remains steady for the following 50 m. The top 20 m of the Sherwood contains carbonate with a δ13C values decreasing to about − 3‰. The occurrence of a stratigraphically-correlatable carbon isotope pattern implies that the primary evolution signal has been preserved. The change in δ13C correlates with indicators of aridity and biological stress such that the highest δ13C values are in sedimentary rocks deposited in a playa lake (arid times); these rocks contain the greatest quantity of dolomite cement. Conversely, the lowest δ13C values correspond to sedimentary rocks deposited from well-developed rivers (relatively humid times) from the lowest quantity of dolomite cement. The same carbon isotope evolution has been found in another well in the Slyne basin and in Belgium, suggesting that the palaeoenvironmental isotope signal in the Triassic sedimentary rocks of the Corrib Field may have a regional significance.  相似文献   
10.
《Sedimentary Geology》2006,183(1-2):15-30
Carbonate concretions in the Miocene sedimentary rocks of the Yeonil Group in the Pohang Basin (Korea) were investigated in terms of stable oxygen and carbon isotope composition to delineate the origin and associated diagenetic environment for their formation. Carbonate concretions are widely distributed in all the sedimentary rocks in the Pohang Basin, showing that the calcitic concretions are preserved within the mass-flow deposits and the dolomitic ones mostly in the hemipelagic siliceous rocks (diatomites). Concretions can be classified into four different types, on the basis of the stable isotopic signatures, each of which represents its own geochemical range.Type I concretions are calcitic and are composed of micrite to microspar. They occur in the conglomerates and sandstones which were deposited by mass flows (debris flow to turbidity current). It shows relatively lower δ18O (− 14.0 to − 9.3‰) and δ13C (− 19.6 to − 8.4‰) values. These concretions grew in a sulfate reducing zone under the influence of residual ambient seawater which had been significantly modified by volcanogenic sediments. Type II concretions are also calcitic, composed mostly of micrite with minor microspar and found in the sandstones. These concretions are characterized by relatively high δ18O (+ 1.8 to + 2.4‰) and variable δ13C (− 17.3 to − 0.4‰) values. These isotopic signatures reflect that Type II concretions formed from just beneath the sediment/water interface down to the sulfate reducing zone through the early stage of methanogenesis. Type III concretions are also calcitic, and composed largely of micrite with a minor contribution of microspar. They are observed in hemipelagic mudrocks which were deposited under the influence of mass flows. They are characterized by intermediate to high δ18O (− 4.6 to + 1.6‰) and high δ13C (− 1.3 to + 8.8‰) values. These concretions grew in a methanogenic zone by residual ambient seawater and/or seawater slightly modified by reaction with volcanogenic sediments. Type IV concretions are dolomite with calcite inclusion, and occur in hemipelagic siliceous rocks. These concretions are mostly composed of micrite and characterized by variable δ18O (− 9.1 to + 0.7‰) and high δ13C (+ 3.1 to + 17.9‰) values, suggesting formation in the methanogenic zone, although the residual ambient seawater is slightly modified by volcanogenic sediments.The same type of the concretions is widely distributed throughout the basin and always shows its own distinctive stable isotopic signature. This means that the formation of the given type depends upon the lithology and composition of host sediments that are closely related to the depositional process of the fan-delta systems regardless of their localities. Further, the different types of concretions are also found at the different, but closely spaced stratigraphic levels in the same locality, displaying the distinctive diagenetic conditions for each type. Such preservation of the unique diagenetic signatures in individual type of concretion suggests that the concretions formed in a completely closed diagenetic system. Therefore, caution should be made to simplify and generalize the diagenetic condition for the formation of any concretions in a large sedimentary basin.  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