培养德识双馨的国家栋梁之才：《普通地质学》课程教学有感

《普通地质学》是引领新生进入地学殿堂、了解地球科学知识的一门专业启蒙课,也是新形势下地学通识教育中的一门基础理论课。其内容涉及地质学全部基础知识中的最必要部分,具有衔接和统领地学各门专业基础知识的特点。根据多年教学体会,笔者认为在精英教育与通才教育并举的新形势下,必须心系学生,与时俱进,转变教育理念,优化集课堂、实验、野外教学为一体的教学体系,推进教学内容的改革与建设,摈弃不适应时代发展与国家需求的教育模式,采用现代化的教学方法和教育技术;对学生开展基础理论传授、专业基础技能训练、创新科研培育的系统教育,拓宽学生的专业知识面,激发学生专业兴趣和创造性思维。在传授科学知识的同时,目标明确地开展思政教育,引导学生认清学问与道德的关系,建立德识双馨的价值取向,提高基础地质课程教学质量和学生的综合素质,促进教学改革,为国家培养五育兼备的优秀人才。     

重庆市实物地质资料管理工作中的难点与对策探讨

实物地质资料管理是自然资源主管部门和馆藏机构的一项法定工作职责。由于历史原因,重庆市自变为直辖市以来实物地质资料管理工作相对滞后,近年来实物地质资料筛选工作的分级开展,实物地质资料的种类和数量呈增长趋势,粗放式分散保管在地勘单位和野外工作现场的方式已不再适应新形势,亟需规范管理。本文主要论述了重庆市实物地质资料管理现状,阐述了在实物地质资料管理工作中急需解决的难点,提出了加强实物地质资料馆藏机构建设、理顺实物地质资料管理体系、落实实物地质资料管理专项资金以及编制重庆市实物地质资料收藏规划等相关对策,为推进重庆市实物地质资料管理工作提供参考。     

甘肃白银厂铜多金属矿田地球化学场特征及信息提取

甘肃白银厂铜多金属硫化物矿田位于北祁连造山带东段,近年来面临严重的资源枯竭危险。通过对区内的构造地球化学测量数据进行多元统计、指数累加等方法的分析,进一步探讨了矿田内地球化学场分布特征,提取更多的找矿预测地球化学信息;研究发现矿田内主要的成矿元素分布受岩性及构造的双重控制,具有明显的北西向成带、北东向成串的特征,矿田中部和外围具有不同的地球化学异常场特征。构造地球化学测量的主要指示元素为 Cu、Pb、Zn、Au、Ag、As、Sb、Hg、K、W等。根据地球化学场分布特征分析认为拉牌沟地区赋矿酸性火山岩向北侧伏,其深部具有一定的找矿前景。基于特征因子得分推断出矿田内具有北东向、北北东向、北东东向、北西向4组规模较大的断裂构造21条,最晚期形成的北西向次级断裂F15-F21是主要的控矿构造。已知的古火山喷口位于W-Au-Mn-Fe-Ti-V-Ba-K-S因子得分小于-0.7的负异常中心内,据此厘定出11个中心喷发口和5个火山喷发中心,已知的矿床位于火山喷发中心内或各火山中心喷发口的结合部。本研究为该矿田开展找矿预测工作提供了有利的地球化学找矿信息。     

TeV γ-ray fluxes from the long campaigns on Mrk 421 as constraints on the emission of TeV–PeV neutrinos and UHECRs

Long TeV γ-ray campaigns have been carried out to study the spectrum, variability and duty cycle of the BL Lac object Markarian 421. These campaigns have given some evidence of the presence of protons in the jet: (i) Its spectral energy distribution which shows two main peaks; one at low energies (∼1 keV) and the other at high energies (hundreds of GeV), has been described by using synchrotron proton blazar model. (ii) The study of the variability at GeV γ-rays and X-rays has indicated no significant correlation. (iii) TeV γ-ray detections without activity in X-rays, called “orphan flares” have been observed in this object.Recently, The Telescope Array Collaboration reported the arrival of 72 ultra-high-energy cosmic rays with some of them possibly related to the direction of Markarian 421. The IceCube Collaboration reported the detection of 37 extraterrestrial neutrinos in the TeV–PeV energy range collected during three consecutive years. In particular, no neutrino track events were associated with this source. In this paper, we consider the proton–photon interactions to correlate the TeV γ-ray fluxes reported by long campaigns with the neutrino and ultra-high-energy cosmic ray observations around this blazar. Considering the results reported by The IceCube and Telescope Array Collaborations, we found that only from ∼25% to 70% of TeV fluxes described with a power law function with exponential cutoff can come from the proton–photon interactions.     

三维地震勘探在构造复杂区的应用

三维地震勘探通过炮点与检波点的灵活组合,适合于复杂地表条件下地震勘探,从原理上也更加符合地质体的三维空间特性,有利于构造复杂的研究与探测.本文介绍的查庄煤矿就是利用三维地震勘探方法成功解决复杂构造问题的典型实例之一.     

气测录井技术的进展及气测资料新用途的探讨

过去,由于气测录井技术的限制,气测数据被认为是不可靠的,其应用的范围也因此受到了制约。现在,随着气测获取及分析技术所取得的进步,可以得到更为准确的气测数据。为了能充分利用气测资料,通过分析气测数据不同比值的深度曲线图,利用曲线的形态及趋势可以划分岩性界面、划分油气水界面、判断地层流体的渐变、推测盖层的封堵效率、预测石油是否遭受了生物降解以及对不同层位的油源进行初步分析。     

Assessing physical vulnerability for multi-hazards using an indicator-based methodology

Globally, many built-up areas are threatened by multiple hazards which pose significant threat to humans, buildings and infrastructure. However, the analysis of the physical vulnerability towards multiple hazards is a field that still receives little attention although vulnerability analysis and assessment can contribute significantly to risk reduction efforts. Indicator-based vulnerability approaches are flexible and can be adjusted to the different hazards as well as to specific user needs. In this paper, an indicator-based vulnerability approach, the PTVA (Papathoma Tsunami Vulnerability Assessment), was further developed to be applicable in a multi-hazard context. The resulting multi-hazard version of the PTVA consists of four steps: the identification of the study area and relevant hazards as well as the acquisition of hazard information, the determination of vulnerability indicators and collection of data, the weighting of factors and vulnerability assessment and finally, the consideration of hazard interactions. After the introduction of the newly developed methodology a pilot application is carried out in the Faucon municipality located in the Barcelonnette basin, Southern French Alps. In this case study the vulnerability of buildings to debris flows, shallow landslides and river flooding for emergency planning and for general risk reduction purposes is assessed. The implementation of the methodology leads to reasonable results indicating the vulnerable buildings and supporting the priority setting of different end-users according to their objectives. The constraints of the presented methodology are: a) the fact that the method is not hazard-intensity specific, thus, vulnerability is measured in a rather qualitative and relative way and b) the high amount of data required for its performance. However, the advantage is that it is a flexible method which can be applied for the vulnerability analysis in a multi-hazard context but also it can be adjusted to the user-specific needs to support decision-making.     

玉林市“6·21”大暴雨成因分析

利用常规的天气图、物理量场及数值预报等资料,对2010年6月21日玉林市出现的大暴雨天气进行分析,结果表明：（1）高空波动、中低层切变线、西南暖湿气流和地面弱冷空气是影响此次强降水过程的主要天气系统;（2）对于单站预报,在掌握大气环流形势背景的同时,综合分析各物理量场尤其是本站的重要物理量各层垂直分布,对预报有很好的指示意义。     

济南市一次持续大雾过程分析

利用常规气象观测资料对2007年12月20-23日济南市一次持续大雾天气过程的大尺度天气背景、地面气压场、温度对数压力图以及单站气象要素进行了分析,结果表明:雾是在稳定的大气层结下出现的天气现象,根据大气稳定层结的状况及变化,可以判断大雾天气的有无及生消时间;近地面逆温和低空逆温同时存在,表明大气层结非常稳定,近地面逆温有利于近地面层水汽积累,低空逆温使近地面层水汽不易扩散而聚集,有利于近地面层维持潮湿,持续几天出现大雾;连续几天大气层结都处于稳定状态,地面风力很小,这些都限制了近地面层的水汽向外耗散,底层相对湿度较大,为大雾的形成提供了充沛的水汽条件.     

The Origin of the Element Eu in Extremely Metal-poor Halo Stars

The fast neutron capture process (the r-process) occurs in the neutron-rich circumstance. However its concrete physical environment is not very clear. With recent progress in observations, many extremely metal-poor halo stars have been discovered. They have two characteristics: one is the overabundance of fast neutron elements with the relative abundance consistent with that of the sun; the other is that fast neutron element contents in stars at the same metal abundance have a very large dispersion. This provides a particular way to study the origin of the r-process. Simulation was used to study the galaxy's evolution process and the resulting dispersion of fast neutron nuclide contents in stars. The model of galaxy evolution obtained in this way not only contains spontaneous star formation in the gas region, but also includes the star formation excited by the supernova explosion. It is shown from our results that the supernovae at the low mass end should be the place producing the fast neutron nuclides. In addition, it is also shown that the non-uniformity of the galaxy evolution caused by the supernova explosion is not enough to explain the observed dispersion of fast neutron element contents in halo stars. This problem should be further studied.