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341.
2021年2月13日23点07分(当地时间)日本福岛县海域发生了7.3级地震,这是2011年以来东日本大地震记录到的较大余震。距离震源较近的强震动观测点记录到约1.5 g的最大加速度。对离震源较近的几个城市及乡村,包括郡山市、福岛市和仙台市以内的地方进行了建筑物的震害调查。调查中发现:日本常用的木结构民宅在地震中仅发生了屋顶的瓦片掉落和剥离等轻微破坏,并没有发生严重的破坏。另外,在郡山市和福岛市有几栋高层钢筋混凝土结构的房屋有较严重的损坏。2021年福岛地震这一现象可能与地震动的短周期特性(小于1s)以及建筑物的高次振型有关。  相似文献   
342.
张振斌  王宏伟 《中国地震》2021,37(4):908-915
以新疆强震动台网获取的伽师6.4级地震的42组126条原始加速度记录为依据,对强震动记录时程、幅值、频谱三方面进行分析。结果表明,此次地震获取的最大加速度峰值为633.3cm/s2,仪器地震烈度为Ⅸ度;在震中距200km以内两水平向与垂直向加速度峰值比在1~3之间,速度峰值比在0~4之间。分析此次地震三分向加速度峰值衰减关系,0~50km范围内地震峰值加速度观测值在分区地震动衰减关系(Yu13)长轴预测值误差范围之内,高于南天山西段土层衰减关系(Zhang)预测值;水平向加速度反应谱卓越周期主要集中在0~0.5s,垂直向集中在0~0.2s。65XKR台水平向反应谱高于Ⅷ度罕遇地震设计反应谱,峰值卓越周期为0.48s;垂直向反应谱高于Ⅷ度罕遇地震设计反应谱,峰值位于高频段。  相似文献   
343.
Unlike most tropical Pacific islands, which lie along island arcs or hotspot chains, the Loyalty Islands between New Caledonia and Vanuatu owe their existence and morphology to the uplift of pre-existing atolls on the flexural forebulge of the New Hebrides Trench. The configuration and topography of each island is a function of distance from the crest of the uplifted forebulge. Both Maré and Lifou are fully emergent paleoatolls upon which ancient barrier reefs form highstanding annular ridges that enclose interior plateaus representing paleolagoon floors, whereas the partially emergent Ouvea paleoatoll rim flanks a drowned remnant lagoon. Emergent paleoshoreline features exposed by island uplift include paleoreef flats constructed as ancient fringing reefs built to past low tide levels and emergent tidal notches incised at past high tide levels. Present paleoshoreline elevations record uplift rates of the islands since last-interglacial and mid-Holocene highstands in global and regional sea levels, respectively, and paleoreef stratigraphy reflects net Quaternary island emergence. The empirical uplift rates vary in harmony with theoretical uplift rates inferred from the different positions of the islands in transit across the trench forebulge at the trench subduction rate. The Loyalty Islands provide a case study of island environments controlled primarily by neotectonics.  相似文献   
344.
远场类谐和地震动与近断层脉冲型地震动是两种不同类型的长周期地震动,确定其能量的时频分布特性对理解长周期地震动作用下长周期结构的反应特点及揭示结构破坏机理具有重要意义.各选10条远场类谐和地震动、近断层脉冲型地震动与普通地震动,利用Hilbert-Huang变换,提取出各地震动的3-D Hilbert幅值谱、边际谱、Hilbert能量谱与瞬时能量曲线,在此基础上提出累积能量谱、强频段、能量时间分布系数等概念,定义了多个指标对比分析三类地震动的长周期特性、宽频带特性和脉冲特性.结果表明:与普通地震动相比,远场类谐和地震动与近断层脉冲型地震动的能量主要集中于较低的频段,长周期特性明显,且远场类谐和地震动的能量集中频段低于近断层脉冲型地震动;远场类谐和地震动的强频段宽度小于其他两类地震动,且能量在强频段内的分布比其他两类地震动均匀;与其他两类地震动相比,远场类谐和地震动的脉冲特性不明显;三类地震动的卓越频率与能量时间分布系数均存在明显的分布规律,可以作为地震动的能量表征参数.  相似文献   
345.
Dynamic characteristics of structures — viz. natural frequencies, damping ratios, and mode shapes — are central to earthquake‐resistant design. These values identified from field measurements are useful for model validation and health‐monitoring. Most system identification methods require input excitations motions to be measured and the structural response; however, the true input motions are seldom recordable. For example, when soil–structure interaction effects are non‐negligible, neither the free‐field motions nor the recorded responses of the foundations may be assumed as ‘input’. Even in the absence of soil–structure interaction, in many instances, the foundation responses are not recorded (or are recorded with a low signal‐to‐noise ratio). Unfortunately, existing output‐only methods are limited to free vibration data, or weak stationary ambient excitations. However, it is well‐known that the dynamic characteristics of most civil structures are amplitude‐dependent; thus, parameters identified from low‐amplitude responses do not match well with those from strong excitations, which arguably are more pertinent to seismic design. In this study, we present a new identification method through which a structure's dynamic characteristics can be extracted using only seismic response (output) signals. In this method, first, the response signals’ spatial time‐frequency distributions are used for blindly identifying the classical mode shapes and the modal coordinate signals. Second, cross‐relations among the modal coordinates are employed to determine the system's natural frequencies and damping ratios on the premise of linear behavior for the system. We use simulated (but realistic) data to verify the method, and also apply it to a real‐life data set to demonstrate its utility. Copyright © 2012 John Wiley & Sons, Ltd.  相似文献   
346.
As the forward directivity and fling effect characteristics of the near-fault ground motions, seismic response of structures in the near field of a rupturing fault can be significantly different from those observed in the far field. The unique characteristics of the near-fault ground motions can cause considerable damage during an earthquake. This paper presents results of a study aimed at evaluating the near-fault and far-fault ground motion effects on nonlinear dynamic response and seismic damage of concrete gravity dams including dam-reservoir-foundation interaction. For this purpose, 10 as-recorded earthquake records which display ground motions with an apparent velocity pulse are selected to represent the near-fault ground motion characteristics. The earthquake ground motions recorded at the same site from other events that the epicenter far away from the site are employed as the far-fault ground motions. The Koyna gravity dam, which is selected as a numerical application, is subjected to a set of as-recorded near-fault and far-fault strong ground motion records. The Concrete Damaged Plasticity (CDP) model including the strain hardening or softening behavior is employed in nonlinear analysis. Nonlinear dynamic response and seismic damage analyses of the selected concrete dam subjected to both near-fault and far-fault ground motions are performed. Both local and global damage indices are established as the response parameters. The results obtained from the analyses of the dam subjected to each fault effect are compared with each other. It is seen from the analysis results that the near-fault ground motions, which have significant influence on the dynamic response of dam–reservoir–foundation systems, have the potential to cause more severe damage to the dam body than far-fault ground motions.  相似文献   
347.
西沙海域内潮与近惯性内波的相互作用   总被引:4,自引:1,他引:3       下载免费PDF全文
通过使用西沙海域锚定潜标的测流数据,分析了距浣熊台风路径100 km处海流受浣熊台风影响前后的动能谱、旋转谱和流剪切谱,从而阐明近惯性波,以及近惯性波与全日内潮波的相互作用机制.台风浣熊之后所引起的近惯性波主要在上250 m较强,其能量是普通风场所引起的40倍.近惯性波的能量向下传播至450 m左右,与此同时,强的近惯性流的剪切驱动着惯性波与全日内潮波之间的相互作用,从而产生强的近惯性波与全日内波的耦合波(f+D1).此三波耦合机制为Davies的波波相互作用理论提供了观测依据,同时,近惯性内波与全日内潮波之间的非线性相互作用,揭示了南海近惯性波能量耗散的一种机制.  相似文献   
348.
349.
A parametric study of wave loads on trimaran ships traveling in waves   总被引:3,自引:0,他引:3  
In this paper, we present a spectral analysis based on wave loads to select suitable side-hull arrangements for a trimaran ship traveling in waves. Neglecting the steady flow effect, the three-dimensional source-distribution method, using a pulsating source potential incorporating the panel method, is adopted to solve the corresponding hydrodynamic coefficients. The significant values for wave loads, including shear forces, bending moments, and torsion moments at different locations on the main hull and connected deck with respect to different staggers and clearances, are derived by the spectral analysis. Several ship speeds and wave headings are also considered for comparison. This study offers more information for selecting the side-hull arrangement from the viewpoint of wave loads on trimaran ships, which may be regarded as helpful references for seakeeping design of these types of ships.  相似文献   
350.
The line profiles of Hα in a limb flare on 1998 November 11 appear to be unusually broadened. It is considered that macro-turbulence (or macroscopic mass motions) may be one of the main causes. We use an inversion technique to extract the probability distribution of the line-of-sight velocity in the flare. There exist some differences between the velocity distributions deduced from Hα and from CaⅡ λ8542, which may be because the two lines depend differently on the temperature and velocity. Since the loop density is high, we obtain a rather short cooling time (several tens of seconds) from the hot X-ray loops to the cool loops visible in Hα. Possible origins of the large scale motions are discussed.  相似文献   
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