海水声速剖面基函数的重构性能分析

海水声速剖面通常使用经验正交函数（Empirical Orthogonal Function,EOF）进行稀疏表示,然而基函数会受到数据完备性和数据测量时间的制约,其代表性误差会导致声速剖面重构精度受限。为了提高声速剖面的重构精度,本文利用模糊C均值聚类对BOA_Argo历史数据集进行聚类分析,探讨不同聚类空间的训练集数据对实测声速剖面重构精度的影响。研究表明,声速剖面具有明显的时空聚集特性,聚类后的历史声速剖面集生成的基函数和平均声速剖面具有最优的重构性能。本文研究结果有助于为历史声速剖面训练集的选取提供实际指导意义,进而提高声速剖面重构精度乃至反演精度。     

层次分析法在新疆卡姆斯特煤矿区煤炭资源评价中的应用

卡姆斯特煤矿区煤炭资源储量丰富,但煤田地质工作程度低,勘探开发滞后,已不能适应阿勒泰地区经济发展对矿产开发的需求。为缓解阿勒泰地区煤炭紧缺状况,依据勘探程度、构造复杂程度、煤层露头线及煤层1 000m深部界线等因素圈定三巴斯陶、塔哈拉巴斯塔乌、喀拉萨依等3个含煤远景区作为煤炭资源评价单元,将资源条件、开采技术条件、开发条件和开发效益等影响煤炭资源评价的要素细化为29个评价参数,运用层次分析法（AHP）建立煤炭资源评价模型,构建对比矩阵,确定评价参数权值总排序。根据各评价对象的调查成果,结合专家意见给出各参数隶属度权值,利用乘积法得出评价对象的综合评价隶属度：三巴斯陶为0.627 5,塔哈拉巴斯塔乌为0.700 5,喀拉萨依为0.682 7。根据该结果,认为塔哈拉巴斯塔乌含煤远景区煤炭资源综合条件较好,可作为下一步勘查工作的首选区。     

流体 花岗岩 金矿

流体地质研究是当代地学研究中的重要前沿课题，已成为发展地质科学、建立新的知识体系的一个主要支柱和知识生长点。本文阐述了当今国内外流体的研究现状、发展水平、流体的涵义、性质、研究方法和研究重点及其与板块构造、变质作用、岩浆作用、成矿作用、成矿作用的重要意义。流体地质为地质科学提出了许多新的研究机会和挑战。该文在简要评述当今花岗岩研究现状的基础上，对花岗岩与金矿的关系进行了深入的讨论，指出了不同成因类型的花岗岩与金矿有着完全不同的关系。人们所说的花岗岩与金矿关系多数情况下应考虑是流体作用的结果。最后指出加强流体地质研究对提高河南地质与金矿的研究水平具有十分重要的实际意义和理论意义。     

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中国地震预报论坛2023年度学术交流大会在四川康定召开

中国地震学会地震预报专业委员会和四川省地震局于2023年8月15—19日在四川省康定市联合举办了中国地震预报论坛2023年度学术交流大会,来自全国地震行业内、外8所大学、4个中科院直属科研院所与23个地震行业直属科研院所及省市级分支机构共35个单位的100余名代表参加了此次会议。学术交流设置了12个专题;会前征集到论文96篇,会期交流报告78个,其中口头报告23个,张贴展板55个;23个口头报告中,大会特邀报告6个;从55个张贴报告中,评选出优秀报告6个,最佳设计创意报告1个。为了配合活断层野外识别的科普培训,本次大会将原计划以 “制约地震三要素的因素与地震三要素预报的瓶颈问题” 为主题的大会圆桌讨论改成了 “鲜水河断裂带高震级危险性分析” 的专题培训讲座,讲座之后再适时举行了 “如何强化高危险区的临震监测与临震跟踪预报能力” 的专题讨论。对2022年泸定6.8级地震的交流讨论提出了新的科学问题。大会不仅重视学术交流,还兼顾了科学传播的普及,利用当地的科普资源,因地制宜地组织了为期一天的鲜水河断裂带活动特征的野外识别科普培训。地震预报论坛学术交流大会全体与会代表参加了此次野外实训活动,活动中邀请了著名的鲜水河断裂带活动特征研究专家现场授课,增强了地震预报与地震地质领域的跨学科交流,强化了学术交流的效果。

     

Analysis of city centrality based on entropy weight TOPSIS and population mobility: A case study of cities in the Yangtze River Economic Belt

Based on statistical data and population flow data for 2016,and using entropy weight TOPSIS and the obstacle degree model,the centrality of cities in the Yangtze River Economic Belt(YREB)together with the factors influencing centrality were measured.In addition,data for the population flow were used to analyze the relationships between cities and to verify centrality.The results showed that:(1)The pattern of centrality conforms closely to the pole-axis theory and the central geography theory.Two axes,corresponding to the Yangtze River and the Shanghai-Kunming railway line,interconnect cities of different classes.On the whole,the downstream cities have higher centrality,well-defined gradients and better development of city infrastructure compared with cities in the middle and upper reaches.(2)The economic scale and size of the population play a fundamental role in the centrality of cities,and other factors reflect differences due to different city classes.For most of the coastal cities or the capital cities in the central and western regions,factors that require long-term development such as industrial facilities,consumption,research and education provide the main competitive advantages.For cities that are lagging behind in development,transportation facilities,construction of infrastructure and fixed asset investment have become the main methods to achieve development and enhance competitiveness.(3)The mobility of city populations has a significant correlation with the centrality score,the correlation coefficients for the relationships between population mobility and centrality are all greater than 0.86(P<0.01).The population flow is mainly between high-class cities,or high-class and low-class cities,reflecting the high centrality and huge radiating effects of high-class cities.Furthermore,the cities in the YREB are closely linked to Guangdong and Beijing,reflecting the dominant economic status of Guangdong with its geographical proximity to the YREB and Beijing's enormous influence as the national political and cultural center,respectively.     

京津冀及周边一般性降水与短时强降水特征对比

京津冀及周边地区为我国北方强降水的多发区域。基于1966—2021年87个国家级气象站逐小时降水资料对比分析暖季5—9月一般性降水和短时强降水的空间分布及年际变化,并基于1980—2021年298个气象站分析日变化等特征。结果表明：京津冀及周边地区的渤海西侧平原区域存在短时强降水强度极端性显著区域。渤海西侧平原以外区域两类降水平均小时降水量、强度和降水时次百分比均呈增长趋势,但短时强降水的增幅更高,而渤海西侧平原区域趋势则均不明显。渤海西侧平原区域和渤海西侧平原以外区域的一般性降水平均小时降水量和降水时次百分比日变化幅度显著弱于短时强降水;7—9月渤海西侧平原区域降水夜发性更明显,且相比另一区域半峰持续时间多出约2 h。2005年后渤海西侧平原区域和渤海西侧平原以外区域短时强降水平均小时降水量和降水时次百分比下午时段均明显减弱,但午夜后至清晨明显增加。     

湖北省潮汐形变观测异常及干扰识别

对2003—2013年湖北省数字化定点形变潮汐观测中的突跳、阶变、震颤等异常的分析发现,气象因素对形变潮汐观测的影响复杂:1)不同气压场控制影响形变观测的异常形态不同,但响应频率一致;2)台风对形变观测的秒值和分钟值数据在1～4秒和2～4分钟较高频段均有响应;3)台址条件不同,降雨对形变观测产生的畸变影响不同。影响范围一般在0～全日波频段且存在较大的噪声;4)短时大气温度变化对形变观测有一定影响,会使曲线发生抖动或暂态波动,在64～128分钟和128～256分钟较低频段上有响应。水库冲沙、水库蓄水、土石开挖等环境荷载变化对分钟值观测曲线产生明显阶跃、抖动型实时畸变。人员进洞、施工、仪器标定检修等人为活动对观测曲线的影响可直接识别。     

The evolution of the z distribution of normal neutron stars in the Galaxy

Under the two initial 1‐D one parameter velocity distribution forms (one is normal, the other is exponential), the z direction scale height evolution of normal neutron stars in the Galaxy is studied by numerical simulation. We do statistics for the cases at different time segments, also do statistics for the cumulative cases made of each time segment. The results show in the cumulative cases the evolution curves of the scale heights are smoother than in the each time segment, i.e., the cumulation improve the signal‐to‐noise ratio. Certainly the evolution cases are different at different Galactic disk locations, which also have very large difference from the average cases in the whole disk. In the initial stages of z evolution of normal neutron stars, after the beginning transient states, the cumulative scale heights increase linearly with time, and the cumulative scale height increasing rates have linear relationship with the initial velocity distribution parameters, which have larger fluctuation in the vicinity of the Sun than in the whole disk. We utilize the linear relationship of the cumulative scale height increasing rates vs. the initial velocity distribution parameters in the vicinity of the Sun to make comparison with the observation near the Sun. The results show if there is no magnetic decay, then the deserved initial velocity parameters are obvious lower than the present well known results from some authors; whereas if introducing magnetic decay, for the 1‐D normal case we can make consistence among concerning results using magnetic decay time values which are supported by some authors, while for the 1‐D exponential case the results show the lackness of young pulsar samples in the larger z in the vicinity of the Sun (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

马鞍山的古冰川地貌

马鞍山是四川盆地西南边缘第一高山。此山存在第四纪冰川地貌。它是我国东部一处典型的古冰川地貌，时代属末次冰期与新冰期。