Study on multiple induced polarization parameters in groundwater exploration in Bashang poverty alleviation area of Heibei Province,China          下载免费PDF全文

LIU Zhi-yuan  TAN Ding  CHEN Zhi-bin  WEI Yun-fei  CHAI Quan  CHEN Xiao-hang 《地下水科学与工程》2020,8(3):274-280

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   

四川地区震后应急会商资料快速产出系统的设计与实现     

祁玉萍  汪小厉  林圣杰  肖本夫  何畅  廖晓峰 《震灾防御技术》2020,15(1):176-183

地震预报意见以大量资料为基础，依靠专家经验和多学科知识并通过会商讨论形成。显著地震发生后，快速、准确、有效地研判震情可为后期应急指挥和地震现场工作奠定基础。本文以Datist软件为平台，基于四川及邻区的基础资料，设计研发符合四川震情的震后会商资料快速产出系统，当四川及邻区发生中强地震时，通过该系统可在收到地震短信5分钟内以请求触发的方式快速产出应急会商资料，并以微信、PowerPoint和Word的形式将基础资料发送给分析预报人员，为后期趋势分析奠定基础。  相似文献   

2017年九寨沟M_S7.0地震对周围地区的静态应力影响          下载免费PDF全文

靳志同  万永革  刘兆才  黄骥超  李瑶  杨帆 《地球物理学报》2019,62(4):1282-1299

基于九寨沟M_S7.0地震的破裂模型及均匀弹性半空间模型，本文计算了该地震在周围主要活动断层上产生的库仑应力变化、在周围地区产生的应力场和位移场和同震库仑应力变化对余震的触发.结果表明：（1）九寨沟地震造成虎牙断裂中段库仑破裂应力有较大增加，已经超过0.01 MPa的阈值，虎牙断裂北段、塔藏断裂中段和岷江断裂北段北部的库仑破裂应力有较大降低，因此尤其要注意虎牙断裂中段的危险性.（2）水平面应力场在该地震震中东西两侧增加（拉张），张应力起主要作用.在震中南北两侧降低（压缩），压应力起主要作用.从水平主压和主张应力方向来看，均呈现出条形磁铁的磁场形态.从剖面上的应力场来看，在上盘的面膨胀区域内，大部分点的主张应力方向与地表是垂直的，在其他区域内，主张应力和主压应力均以震中为中心，向外呈辐射状.（3）从地表水平位移场来看，震中东西两侧物质朝震中位置汇聚，南北两侧物质向外流出，在震中处的最大水平位移量达43 mm.从地表垂直位移场来看，震中南北两侧出现明显的隆升，隆升最大值达56.8 mm.震中东西两侧出现明显的沉降，沉降最大值达74.5 mm.从剖面的位移场来看，九寨沟地震为左旋走滑地震，且有一定的正断成分.由分析可以推测该断层破裂在大致22~26 km的深度上就截止了.并推测下盘物质运动的动力来自震源北东东方向（四川块体）深度在6~30 km的下盘下层物质，上盘物质运动的动力来自震源北西西方向（巴颜喀拉块体）深度在0~6 km的上盘上层物质.（4）通过计算不同深度上主震对余震的触发作用可知，主震后的最大余震受到了主震的触发作用，多数其他余震也受到主震的触发作用.主震的发生促使了库仑应力增加地区余震的发生，抑制了一部分库仑应力减少地区余震的发生.  相似文献   

Study of Star/Galaxy Classification Based on the XGBoost Algorithm     

《Chinese Astronomy and Astrophysics》2019,43(4):539-548

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   

Cotton canopy reflectance under variable solar zenith angles: Implications of use in evapotranspiration models     

Christopher M. U. Neale  Maria P. Gonzalez-Dugo  Angelica Serrano-Perez  Isidro Campos  Luciano Mateos 《水文研究》2021,35(6):e14162

Evapotranspiration (ET) is an important parameter in hydrologic processes and modelling. In agricultural watersheds with competing uses of fresh water including irrigated agriculture, estimating crop evapotranspiration (ET_c) accurately is critical for improving irrigation system and basin water management. The use of remote sensing-based basal crop coefficients is becoming a common method for estimating crop evapotranspiration for multiple crops over large areas. The Normalized Difference Vegetation Index (NDVI) and the Soil Adjusted Vegetation Index (SAVI), based on reflectance in the red and near-infrared bands, are commonly used for this purpose. In this paper, we examine the effects of row crop orientation and soil background darkening due to shading and soil surface wetness on these two vegetation indices through modelling, coupled with a field experiment where canopy reflectance of a cotton crop at different solar zenith angles, was measured with a portable radiometer. The results show that the NDVI is significantly more affected than the SAVI by background shading and soil surface wetness, especially in north–south oriented rows at higher latitudes and could lead to a potential overestimation of crop evapotranspiration and irrigation water demand if used for basal crop coefficient estimation. Relationships between the analysed vegetation indices and canopy biophysical parameters such as crop height, fraction of cover and leaf area index also were developed for both indices.  相似文献   

太原盆地及周边地区双差层析成像   总被引：2，自引：0，他引：2       下载免费PDF全文

王长在  吴建平  杨婷  王未来  范莉苹  房立华 《地球物理学报》2018,61(3):963-974

山西断陷带位于鄂尔多斯与华北地块交汇处，是我国著名的历史强震活动带之一，尤其是断陷盆地中部区域，6级以上地震频发.本研究旨在揭示忻定盆地中南部、太原盆地及临汾盆地中北部交汇处的深部结构特征，分析盆地的形成和演化，探讨该区域孕震环境.利用山西地震台网观测数据以及固定地震台站融合流动台站得到的地震数据，共7455个地震事件，采用双差层析成像方法，反演得到了太原盆地及周边地区的三维P波速度结构及精定位结果.层析成像结果显示，忻定盆地、太原盆地的中上地壳为明显的低速异常，被高速的石岭关隆起隔开，深部结构特征相对简单.太原盆地、临汾盆地及灵石隆起之间的深部结构特征较为复杂，反映了两个盆地演化过程的复杂性.穿过忻定盆地的速度剖面显示，在中地壳存在明显的低速异常体，且大部分地震都发生在该低速体上方；穿过太原盆地北部的剖面显示，该区域在20~25 km深度范围内有较密集的地震分布，并勾画出交城断裂呈犁形的断层特征；穿过太原盆地中部的剖面显示，太原盆地自西向东沉积层逐渐减薄；穿过临汾盆地的剖面揭示，汾东断裂在浅部倾角较陡，随深度增加倾角逐渐变小，倾向向东.  相似文献   

联合概率法在合并相邻台网地震目录中的应用:以2014年鲁甸序列为例          下载免费PDF全文

龙锋  蒋长胜  祁玉萍  刘自凤  傅莺 《地球物理学报》2018,61(7):2815-2827

中国目前实行的区域地震台网独立运行机制，使得在相邻不同台网的交界地区可能存在多个版本的地震目录和震相观测报告，影响了地震活动性分析与研究.为此，本文提出了一种基于联合概率的方法，可标明两个或多个相邻台网目录中相同的事件，合并它们的震相数据开展重新定位，并重构不同台网交界地区的统一地震目录.该方法的思路与分析步骤是：首先，计算获得不同台网之间具有最小发震时刻差异的两两地震的时空强差异分布，查找并剔除独立地震，计算事件合并的联合概率；其次，基于联合概率分析合并不同台网的地震目录和震相观测报告，对合并事件进行重新定位和定位误差分析，并基于G-R关系检验重构目录的完整性.本文以2014年鲁甸地震序列为例的初步应用结果显示，震相合并之后的地震定位精度相比之前单个台网的结果，特别是相比四川台网的目录，定位精度提高非常显著，合并后的目录与之前相对完整的云南目录接近，但相比由两个台网目录简单拼凑而成的目录更加准确.此外，研究还发现在目录合并过程中，对于4级以上的中强震，应选择M_S而不是以M_L震级标度；震相合并后被复用台站记录的到时信息可用于检测不同台网间的震相拾取是否存在系统偏差.本文提出的方法使得在相邻不同台网的过渡区形成一个统一且尽可能准确可靠的地震目录成为可能.  相似文献   

Moment Magnitude and Its Calculation     

Chen Yuntai  Liu Ruifeng 《中国地震研究》2018,32(4):447-455

In this paper, we give a brief introduction to the proposal and development history of the earthquake magnitude concept. Moment magnitude M_W is the best physical quantity for measuring earthquakes. Compared with other magnitude scales used traditionally, moment magnitude is not saturated for all earthquakes, regardless of big and small earthquakes, deep and shallow earthquakes, far field and near field seismic data, geodetic and geological data, moment magnitude can be measured, and can be connected with well-known magnitude scales such as surface wave magnitude M_S. Moment magnitude is a uniform magnitude scale, which is suitable for statistics with wide magnitude range. Moment magnitude is the preferred magnitude selected by the International Seismological community, and it is preferred by the departments responsible for publishing seismic information to the public.Moment magnitude is a uniform magnitude scale, which is suitable for statistics with wide magnitude range. Moment magnitude is a preferred magnitude for international seismology, it is preferred by the agency responsible for providing information about earthquakes to the public. We provide all formulas used in the calculation of moment magnitude, and the calculation steps in detail. We also analyzed some problems and rules to solve these problems by using different formulas and numerical value calculation steps.  相似文献   

Characteristics and Analysis of the Seismic Damage from the M_S7.0 Jiuzhaigou Earthquake in the Area between Songpan and Jiuzhaigou     

Yan Zhaolun  Peng Xiaobo  Li Shuguang  Hong Haichun 《中国地震研究》2018,32(2):173-188

This paper expounds the features of the buildings and analyzes the seismic disaster characteristics of the Jiuzhaigou M_S7. 0 earthquake in the area between Songpan and Jiuzhaigou. New buildings (especially the frame structure) had good anti-seismic performance,but brick-wood structures and brick-concrete structures sustained large amounts of damage in the earthquake. By computing the seismic damage index,we found that the seismic damage index of the frame structure was far less than that of civil structures and brick-wood structures. The seismic damage index of frame structures were all zero in the Ⅵ area,and increased rapidly with the increase of intensity,but the increasing range was reduced. We also discussed how to evaluate the intensity in areas where there was a lack of buildings or there was only one structure type,which can be referenced in future field work.  相似文献   

Relation of Velocity Distribution and Mass for DA White Dwarfstwo     

Xiao-bo Gong  Li-fang Li 《Chinese Astronomy and Astrophysics》2018,42(2):202-212

White dwarfs are the evolutionary endpoint of the low-and-medium mass stars. In the studies of white dwarfs, the mass of white dwarf is an important physical parameter. In this paper, we give an analysis about the velocity distribution of DA white dwarfs in the Sloan Digital Sky Survey (SDSS), and hope to find the relation between mass and velocity distribution of white dwarfs. We get the radial velocity and tangential velocity of every DA white dwarf according to their proper motion and spectral shift. Through analyzing the velocity distribution of DA white dwarfs, we find that the small-mass white dwarfs, which are produced from the single-star evolution channel, have a relatively large velocity dispersion.  相似文献