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   8299篇
  免费   1362篇
  国内免费   2850篇
测绘学   235篇
大气科学   355篇
地球物理   1944篇
地质学   7311篇
海洋学   1442篇
天文学   317篇
综合类   392篇
自然地理   515篇
  2024年   75篇
  2023年   166篇
  2022年   247篇
  2021年   305篇
  2020年   307篇
  2019年   394篇
  2018年   318篇
  2017年   354篇
  2016年   394篇
  2015年   419篇
  2014年   499篇
  2013年   510篇
  2012年   487篇
  2011年   541篇
  2010年   448篇
  2009年   578篇
  2008年   605篇
  2007年   638篇
  2006年   671篇
  2005年   507篇
  2004年   503篇
  2003年   429篇
  2002年   372篇
  2001年   364篇
  2000年   366篇
  1999年   320篇
  1998年   293篇
  1997年   241篇
  1996年   200篇
  1995年   178篇
  1994年   175篇
  1993年   128篇
  1992年   115篇
  1991年   63篇
  1990年   71篇
  1989年   43篇
  1988年   49篇
  1987年   39篇
  1986年   13篇
  1985年   25篇
  1984年   16篇
  1983年   10篇
  1982年   13篇
  1981年   6篇
  1980年   3篇
  1978年   4篇
  1977年   1篇
  1976年   1篇
  1972年   1篇
  1954年   5篇
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
21.
本文系统地研究了鄂尔多斯盆地南部延长组凝灰岩元素和同位素地球化学特征。结果表明:凝灰岩主量元素具有高K、高Al、Si中等至高、低Na的特征; REE总体特征为轻稀土富集、重稀土亏损,∑REE在4857~40212 μg/g 之间变化,Eu呈现出负异常,在034~082内变化,δCe范围在080~208之间; 微量元素中U含量在312~144 μg/g 之间,Ba、U、Th、Hf和Ce呈明显正异常,Nb、P、Ti和Rb呈现负异常。详细的分析表明:U的富集和一些微量元素如Ta、Dy、Lu等相关,Th与∑REE存在明显的正相关性,这些变化可能和盆地中铀矿的富集有关; 凝灰岩的硫同位素总体呈现深源特征。根据以上的研究对凝灰岩的形成原因及形成环境进行了探讨。鄂尔多斯盆地南部延长组凝灰岩来源于秦岭造山带火山作用,其中的铀元素富集是由于砂岩型铀矿中铀向凝灰岩迁移而被还原所致。本研究对盆地砂岩型铀矿的铀运移和富集机理认识具有一定指导意义。  相似文献   
22.
Recent advances in railway-induced ground vibrations showed that the track/soil interaction plays an important role in the low frequency range. This paper contributes to the numerical analysis of train/track/foundation dynamics by presenting the accuracy of a coupled lumped mass (CLM) model devoted to the railway foundations and to the track/soil coupling. Following a summary of the background and the advantages of the CLM model, the coupling strategy is quantified through two application cases. Firstly, the dynamic track deflection is calculated for different railway lines considering various degrees of complexities of foundations. Then, the foundation responses are compared depending on whether detailed coupling is introduced or not. The benefit of the proposed model is emphasized by presenting free-field ground vibration responses generated by a tram and a high-speed train, obtained by a revisited two-step prediction model developed by the authors.  相似文献   
23.
Current theories of F-layer storms are discussed using numerical simulations with the Upper Atmosphere Model, a global self-consistent, time dependent numerical model of the thermosphere-ionosphere-plasmasphere-magnetosphere system including electrodynamical coupling effects. A case study of a moderate geomagnetic storm at low solar activity during the northern winter solstice exemplifies the complex storm phenomena. The study focuses on positive ionospheric storm effects in relation to thermospheric disturbances in general and thermospheric composition changes in particular. It investigates the dynamical effects of both neutral meridional winds and electric fields caused by the disturbance dynamo effect. The penetration of short-time electric fields of magnetospheric origin during storm intensification phases is shown for the first time in this model study. Comparisons of the calculated thermospheric composition changes with satellite observations of AE-C and ESRO-4 during storm time show a good agreement. The empirical MSISE90 model, however, is less consistent with the simulations. It does not show the equatorward propagation of the disturbances and predicts that they have a gentler latitudinal gradient. Both theoretical and experimental data reveal that although the ratio of [O]/[N2] at high latitudes decreases significantly during the magnetic storm compared with the quiet time level, at mid to low latitudes it does not increase (at fixed altitudes) above the quiet reference level. Meanwhile, the ionospheric storm is positive there. We conclude that the positive phase of the ionospheric storm is mainly due to uplifting of ionospheric F2-region plasma at mid latitudes and its equatorward movement at low latitudes along geomagnetic field lines caused by large-scale neutral wind circulation and the passage of travelling atmospheric disturbances (TADs). The calculated zonal electric field disturbances also help to create the positive ionospheric disturbances both at middle and low latitudes. Minor contributions arise from the general density enhancement of all constituents during geomagnetic storms, which favours ion production processes above ion losses at fixed height under day-light conditions.  相似文献   
24.
沈位刚  赵涛  戴峰  王塞玉 《工程地质学报》2016,24(s1):1047-1053
落石是山区公路边坡常见的地质灾害。落石撞击破碎是落石灾害中常见的现象,落石破碎致使运动轨迹改变往往会增大落石的危害性,但其通常未被考虑到落石的防护设计中。因此,落石破碎机理的研究对落石防护措施设计有重要的指导意义。本文运用离散元方法(离散元开源软件Esys-Particle)模拟落石铅直撞击地面的过程。在模型中,落石由大量的颗粒组成,并且相邻的颗粒由可断裂的黏结材料黏接;地面由一层固定的颗粒组成,从而模拟地面的摩擦、弹性变形性质。模型模拟出落石反弹、破碎和粉碎等过程,分析黏结材料的杨氏模量、颗粒间凝聚力和内摩擦角对落石撞击地面过程的影响,得出落石撞击过程中破坏率和动能的变化过程。研究发现:当杨氏模量和凝聚力的比值较小时,落石将会发生反弹;当杨氏模量和凝聚力的比值增大到一定程度时,落石将会破碎成不同大小的块体;当杨氏模量和凝聚力的比值超过一定限度时,落石将会破碎成非常细小的块体;内摩擦角的变化对撞击过程影响非常小。  相似文献   
25.
英峰岭剖面红土的粘土矿物和化学特征与成土环境关系   总被引:14,自引:4,他引:14  
徐义芳  朱照宇 《地球化学》1999,28(3):281-288
地球化学与粘土矿物学研究表明,广东雷州半岛英峰岭多期红土是拉弱武岩红土化初级阶段的产物,由剖面底层至顶层,红土成熟度依次递增。各层红土中主要粘土矿物含量和粘土的Fe2O3含量,以及工土和粘土的氧化,淋溶,富铁铝等化学特征系数与红土埋深之间呈波动起伏的关系。  相似文献   
26.
为了进一步完善Q460钢材在抗震设计规范中相关限值的要求,本文利用有限元软件ABAQUS,以轴压比、翼缘宽厚比、腹板高厚比和壁板宽厚比为变量,建立了共48根“工”字型框架柱和“箱”型框架柱,分析了其抗震性能。结果表明:翼缘宽厚比对框架柱的能量耗散系数影响较小;能量耗散系数随轴压比、腹板高厚比(“工”字型)和壁板宽厚比(“箱”型)增大而明显减小;框架柱的极限承载力随轴压比的减小及壁板宽厚比和翼缘宽厚比的增大而逐渐增大,当腹板高厚比接近规范限值时,承载力下降趋势明显增大。与采用Q235钢材的框架柱相比,Q460钢材框架柱的延性较小,仅为2左右;当采用Q460钢材时,“工”字型框架柱的极限位移角限值建议取为0.03,“箱”型框架柱的极限位移角限值建议取为0.032。规范中对翼缘宽厚比限值的规定偏于保守,其值最大可取至9。无论是“工”字型框架柱还是“箱”型框架柱,其腹板高厚比均不宜过大。Q460钢材框架柱的刚度退化率随轴压比的增大而增强,且翼缘宽厚比越大,腹板高厚比越小,柱的初始刚度越大,刚度退化程度越明显。  相似文献   
27.
于洪军 《地质与勘探》2011,47(4):615-623
在前人对玲珑金矿矿体浅部的研究基础之上,通过对矿体深部黄铁矿的热电性测试与分析,得出:西山矿区380m—90m中段,黄铁矿导型以P—N型(空穴型-电子型导电)为主;东山矿区50m—850m标高范围内,黄铁矿导型以P—N或N—P(电子型-空穴型导电)混合型为主。东、西山矿区的P型出现率在垂向上呈高-低-高的韵律式脉冲变化...  相似文献   
28.
We present a mathematical model of local, steady groundwater flow near a vertical barrier wall. Flow features represented in the model include an impermeable arc-shaped barrier wall and multiple wells; distant boundary conditions are not included explicitly, but their effects on the local flow field are modelled by specifying a uniform flow at infinity and a constant areal recharge within a local domain. We develop an explicit closed-form solution to the boundary-value problem using the analytic element method. The solution is an extension of a harmonic solution presented by Anderson and Mesa [Anderson EI, Mesa E. The effects of vertical barrier walls on the hydraulic control of contaminated groundwater. Adv Water Resourc 2006;29(1):89–98] which does not include the effects of recharge. We demonstrate that the general solution with recharge consists of the harmonic solution superposed on a special case of the harmonic solution along with two elementary one-dimensional flow solutions. The results are used to investigate the effects of areal recharge on the capture zone envelopes of the pumping wells and on the reduction in discharge that can be achieved by including a barrier wall in a pump and treat design. We find that the benefits of including an open barrier wall in a design, measured as a reduction in the pumping rate required to contain a plume, increase for higher recharge rates. Dimensionless plots of capture zone envelopes are presented for a practical well and barrier wall configuration.  相似文献   
29.
We present a set of rotational lightcurve measurements of the small main belt Asteroid 3169 Ostro. Our observations reveal an unambiguous, double-peaked rotational lightcurve with a peak-to-peak variation up to 1.2±0.05 mag and a synodic period of 6.509±0.001 h. From the large flux variation and the overall shape of the lightcurves, we suggest that 3169 Ostro could be a tightly bound binary or a contact binary, similar to the Trojan Asteroid 624 Hektor. A shape model of this system is proposed on the assumption that 3169 Ostro is a Roche binary described by a pair of homogeneous elongated bodies, with a size ratio of 0.87, in hydrostatic equilibrium and in circular synchronous motion around each other. The direction of the spin axis is determined modulo 180° by its J2000 ecliptic coordinates λ0=50±10°, β0=±54±5°. The binary interpretation and the pole solution adequately fit the earlier photometric observations made in 1986 and 1988. However, additional supporting lightcurves are highly desirable especially in the next mutual events occurrence of 2008 and 2009 in order to remove the pole ambiguity and to confirm unambiguously the binary nature of 3169 Ostro.  相似文献   
30.
本文对冀北—辽西地区早白垩世沉积盆地富有机质沉积岩进行了初步有机地球化学分析研究。结果显示,冀北—辽西沉积盆沉积有机质特征在时间和空间上存在很大差异,代表白垩系早期沉积的滦平盆地大北沟组有机质丰度低,这不仅显示其所代表的沉积相带不利于有机质的聚集,也反映了当时生物不够繁盛;大店子组时期沉积相带发生了变化,有机质类型随着发生了变化,丰度有所增高,但总体上显示环境条件不利于生物的发育和繁盛。到了桥头组和义县组沉积岩有机质丰度大幅升高,表明生物界非常繁盛,古气候环境有利于有机质的大量生成和堆积,总体上反映了温湿的气候条件;但同时也存在较为频繁或交替性寒冷气候波动,具体的古气候环境状态尚需进一步深入研究。  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