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1.
Emplacement of small‐volume (<0·1 km3) pyroclastic flows is significantly influenced by topography. The Arico ignimbrite on Tenerife (Canary Islands) is a characteristic small‐volume pyroclastic flow deposit emplaced on high relief topography. The pyroclastic flow flowed down pre‐existing valleys on the southern slopes of the island. In proximal areas deep (up to 100 m) valleys acted as efficient conduits for the pyroclastic flow, which was mostly channelled; in this particular area the ignimbrite corresponds to a homogeneous, moderately welded deposit, consisting of flattened pumices in an abundant ashy matrix with a relatively low lithic fragment content. In intermediate zones significant changes occur in the steepness of the slope and, although still channelled, here the pyroclastic flow was influenced by hydraulic jumps. In this area, two different units can be clearly distinguished in the ignimbrite: the lower unit is composed of a lithic‐rich ground‐layer deposit that formed at the turbulent, highly concentrated head of the flow; the upper unit consists of a well welded pumice‐rich deposit that occasionally reveals a basal layer formed by shearing with the lower part. This division into two units is maintained as far as distal areas near the present‐day coastline, where the slope is very gentle or null and the ignimbrite is not channelled. The ground layer is not found in distal areas. The ignimbrite here only consists of the upper unit, which is occasionally repeated due to a surging process provoked by the lower flow speed, as the pyroclastic flow spread out of the channelled zone. A theoretical model on how topography controlled the deposition of the Arico ignimbrite is derived by interpreting the observed lithological and sedimentological variations in terms of changes in topography and bedrock morphology. This new model is of general applicability and will help to explain other deposits of similar characteristics.  相似文献   
2.
本文主要利用地震海洋学方法研究地中海直布罗陀海峡附近内孤立波的结构特征,此处内孤立波为第一模态下沉型,为中幅度和大幅度内孤立波,垂向振幅最大可达74.5 m,振幅随深度增加呈增大趋势,传播速度随振幅增大而增大,可以确定"真"最大振幅位置位于密跃层附近.由于类多普勒效应和孤立波与测量船之间存在夹角的原因,从地震剖面上得到的为视半高宽参数,需要进行校正后才能得到比较真实的半高宽参数,校正后半高宽最高可达到1721.8 m,但是校正后的半高宽与理论结果有些差距,这可能与内孤立波的发育稳定程度有关.随着内孤立波包不断向东运动,整体波宽变大,垂向速度变小.本文将地震海洋学方法拓展应用于地中海区域内孤立波分析,进一步证明了利用地震海洋学方法研究海水运动的可行性.  相似文献   
3.
李向东 《世界地质》2020,39(1):45-55
笔者从流体的角度,对近年来有关流体沉积问题的研究成果进行整理、总结、归纳和诠释。从沉积学的角度总体上可将流体分为牵引流、过渡流和重力流3大类:其中牵引流是研究的基础,可进一步分为单向流、双向流和振荡流3种基本类型以及叠置流、复合流和叠加流3种复合类型,可按照流体力学的相关方法展开研究;过渡流和重力流沉积研究的关键在于各种重力流类型之间(浊流、液化沉积物流、颗粒流和碎屑流)及其和牵引流之间的相互转化。流体的沉积机制可分为垂直降落沉积(静水)、底床阻碍沉积(牵引流)和能量减弱沉积(重力流)3大类,各种流体的交互作用最终可形成丘状(洼状)交错层理的水动力条件。通过综述可以发现,从流体角度进行沉积学研究尽管困难,但仍然可行,特别是对于复杂水动力条件下的沉积学研究具有一定的意义。  相似文献   
4.
我国铁路桥梁普遍采用少筋混凝土重力式桥墩(配筋率<0.5%),现有普通钢筋混凝土结构的延性抗震理论不适用于该类型桥墩。为了促进我国铁路重力式桥墩抗震理论的发展,详细论述了我国少筋混凝土重力式桥墩的研究现状和存在问题。首先,对少筋混凝土重力式桥墩的破坏特征及破坏机理进行了总结;其次,分析了各参数对少筋混凝土重力式桥墩抗震性能的影响;再次,对目前少筋混凝土重力式桥墩的抗震设计方法进行了汇总与分析;最后,对少筋混凝土重力式桥墩的数值分析模型进行了归纳与分析。通过对现有研究的汇总发现:目前对少筋混凝土重力式桥墩的试验研究主要以拟静力方法为主,还缺少振动台试验研究其动力状态下的破坏机理及抗震性能;少筋混凝土重力式桥墩的破坏机理及其与各影响因素之间的定量关系还不明确;已提出的少筋混凝土重力式桥墩的抗震设计方法存在塑性铰区计算不合理等问题,还需要进一步的完善。为少筋混凝土重力式桥墩抗震研究提供了方向。  相似文献   
5.
The study examines a water exploration and poverty alleviation project in Guyuan county. The study analyzes correlations between aquifers and multiple induced polarization (IP) parameters, including resistivity, polarizability, deviation, half decay time, water-bearing factors, and Kc, a new parameter refined in this study. Based on the study, the well was placed accurately, and its maximum water inflow reached 30 m3/h. Kc value highlights the rate of change at early stages of IP secondary field. Kc value served as a quick indicator in this groundwater prospecting and is validated in practice. Progress has been made in finding new parameters in exploring water with IP method. Thanks to the project, local people have access to water and poverty alleviation has scored some achievements.  相似文献   
6.
利用东北地区近几年流动重力观测数据,分析前郭5.8级震群周边重力点值的时序变化特征,并基于重力段差变化对东北地区整体和局部重力变化引入能够反映异常显著性程度的指标量G和C值,最后对前郭5.8级震群前的重力场动态变化作三维密度反演。结果表明:1)前郭5.8级震群发震构造两侧的局部重力变化具有较明显的差异性,其变化趋势可作为识别构造活化或解耦运动的标志;2)显著性指标量G和C值能够为地震重力前兆的定量描述提供新思路;3)震前重力变化的反演结果显示地震发生在质量运移的过渡区域,垂向反演结果对本次地震的震源深度有一定的揭示意义。  相似文献   
7.
选取唐山地区2008~2018年震相数据,利用单台多震和达法和多台多震和达法分别计算波速比,结合研究区内的地震活动对波速比的变化特征进行研究。结果显示,多台多震和达法得到的波速比结果较为稳定,而单台多震和达法得到的结果变化幅度大,显示更多细节;唐山地区ML≥4.5地震发生前单台波速比存在不同程度的异常,异常台站的方位与地震具有一定的对应性。  相似文献   
8.
为保证海上风电升压电站建设的经济合理与安全可靠,合理确定海上风电升压电站平台高程十分必要。文中从波浪与潮位的遭遇组合、最大波高取值与现行相关标准的比较、最大波峰高度计算的合理性等方面,全面分析了确定海上风电升压站平台高程各组成项取值标准的合理性,研究认为现行标准明显偏高。建议海上升压站平台底部高程按"100年一遇极端高水位+重现期50年波列累积频率1%的最大波峰高度+安全超高"确定。结合工程实例计算分析,按本文建议可使海上升压站平台高程明显降低,从而节省工程造价,还可减轻升压站工程对周边风机的遮蔽影响,以达到多发电量的效果。  相似文献   
9.
Machine learning has achieved great success in many areas today. The lifting algorithm has a strong ability to adapt to various scenarios with a high accuracy, and has played a great role in many fields. But in astronomy, the application of lifting algorithms is still rare. In response to the low classification accuracy of the dark star/galaxy source set in the Sloan Digital Sky Survey (SDSS), a new research result of machine learning, eXtreme Gradient Boosting (XGBoost), has been introduced. The complete photometric data set is obtained from the SDSS-DR7, and divided into a bright source set and a dark source set according to the star magnitude. Firstly, the ten-fold cross-validation method is used for the bright source set and the dark source set respectively, and the XGBoost algorithm is used to establish the star/galaxy classification model. Then, the grid search and other methods are used to adjust the XGBoost parameters. Finally, based on the galaxy classification accuracy and other indicators, the classification results are analyzed, by comparing with the models of function tree (FT), Adaptive boosting (Adaboost), Random Forest (RF), Gradient Boosting Decision Tree (GBDT), Stacked Denoising AutoEncoders (SDAE), and Deep Belief Nets (DBN). The experimental results show that, the XGBoost improves the classification accuracy of galaxies in the dark source classification by nearly 10% as compared to the function tree algorithm, and improves the classification accuracy of sources with the darkest magnitudes in the dark source set by nearly 5% as compared to the function tree algorithm. Compared with other traditional machine learning algorithms and deep neural networks, the XGBoost also has different degrees of improvement.  相似文献   
10.
There is a growing practical interest in the ability to increase the sea states at which marine operations can be safely undertaken by exploiting the quiescent periods that are well known to exist under a wide range of sea conditions. While the actual prediction of quiescent periods at sea for the control of operations is a deterministic process, the long term planning of future maritime tasks that rely on these quiescent periods is a statistical process involving the anticipated quiescence properties of the forecasted sea conditions in the geographical region of interest. It is in principle possible to obtain such data in tabular form either large scale simulation or from field data. However, such simulations are computationally intensive and libraries of appropriate field data are not common. Thus, it is clearly attractive to develop techniques that exploit standard wave spectral models for describing the quiescence statistics directly from such spectra. The present study focuses upon such techniques and is a first step towards the production of a computationally low-cost quiescence prediction tool and compares its efficacy against simulations. Two significant properties emerge for a large class of wave spectral models that encompasses the ubiquitous Neumann and Pierson Moskowitz or Bretschneider forms. Firstly, the auto-correlation function of the wave profile that are required to produce the quiescence property can be obtained analytically in terms of standard special functions. This considerably reduces the computational cost making desktop computer-based planning tools a reality. Secondly, for each class of these parametric spectra, the probability of a given number of consecutive wave heights (normalised to the significant wave heights) less than some critical value is in fact independent of absolute wave height. Thus, for a broad class of practically interesting wave spectra all that is required to obtain the statistical distribution of the quiescent periods is simple rescaling.  相似文献   
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