渗流场与应力场耦合分析在地质科学中的应用

论述了渗流场与应力场耦合分析的基本原理及其在石油勘探、成矿预测及斜坡稳定性评价中应用的理论基础和技术路线。     

表面多次波衰减技术在渤海海峡应用效果

浅水地震勘探对于了解近海底地质构造具有重要意义,目前已被广泛用于油气开发、近岸工程等领域。表面多次波的存在干扰了有效波信息,影响了资料品质,造成解释假象,如何有效地压制多次波,已成为浅水地震勘探中的关键问题。表面多次波衰减方法(SRME)是一种去除海面相关多次波效果较好的技术方法,但是,一般认为SRME技术并不适合于浅水区域。分析了SRME去除多次波的基本原理,并将其应用于海洋高分辨率浅水区域多次波的去除。实际处理效果表明,使用SRME技术处理后的叠加剖面多次波去除效果明显,剖面基底清楚,断面清晰。通过对SRME技术应用于浅水区域的探讨,证实了SRME技术在海洋高分辨率地震勘探浅水区域应用效果较好。     

逻辑回归模型在边坡稳定性分析中的应用

采用逻辑回归模型和确定性系数CF建立概率模型,使用收集到的22个边坡实例,将重度、内聚力、坡角、坡高、内摩擦角和孔隙压力比六个影响因子作为自变量,边坡状态作为因变量,应用SPSS取不同的滑坡概率P与不滑坡概率1-P的比值的自然对数Z进行回归分析。将获得的滑坡概率拟合模型反馈到样本参数上,对比其误差,选取Z=±10时的函数模型对另外8组边坡进行验证,证明预测模型的合理性。     

闽中南罕见冬季锋前暴雨个例特征分析

利用福建省逐小时加密自动站资料、风廓线、S波段双偏振雷达与雨滴谱等新型探测资料以及NCEP逐6 h的1°×1°大气再分析资料,分析了2017年2月21—22日福建中南部一次预报失败的冬季暴雨过程。结果表明:(1)此次暴雨过程类似于锋前暖区暴雨,自2000年以来仅此一例,十分罕见,是在低空急流偏强并长时间维持的背景下产生的,并未受到南支槽和冷空气的影响。(2)闽中大到暴雨带和闽南暴雨区的对流系统相互独立,有多个对流系统影响闽中地区,仅两个对流系统影响闽南地区。降水有较明显对流特征,属暖云弱对流降水,容易导致预报员对雨强估计不足。(3)此次冬季暴雨过程的水汽主要来自南海地区,低层水汽条件与汛期暴雨相当,但整层水汽条件较汛期略差;低空急流对暖湿气流的输送使暴雨区趋于不稳定,但对流不稳定度较汛期弱。(4)高空辐散低层辐合的配置为冬季暴雨带来了有利的动力抬升条件,但暴雨区涡旋性不强,无明显正涡度柱。其中,闽中大到暴雨主要与条件性对称不稳定有关,是在湿斜压作用下倾斜上升运动中产生,而闽南暴雨区既存在对流不稳定,也存在条件性对称不稳定。     

桑沟湾沉积碳库年汇入速率的长期变化及其区域性差异

对取自桑沟湾北西南三根柱样近200 a碳来源及埋藏通量的解析,分析了湾内不同站位各形态碳的差异性,进而对全湾碳埋藏进行了估算。湾内环流、贝藻养殖等造成湾内不同区域碳埋藏的差异;桑沟湾总碳（TC）平均量1.79%,有机碳（TOC）平均量0.54%,无机碳（TIC）平均量1.25%,TOC含量相对较小,为海陆混合来源,以陆源有机碳（C_t）为主,大规模人工养殖后,海源有机碳（C_a）有明显增加的趋势。桑沟湾碳埋藏通量平均为228.9 g/（m2·a）,以无机碳为主要埋藏形式（约占70%）,高的沉积速率及生物残骸沉降使桑沟湾养殖区碳的来源及埋藏区别于其他陆架海域。     

走滑拉分断块对沉积的控制作用——准噶尔盆地东部侏罗系中下统沉积主控因素新认识

通过在南缘露头剖面相构型识别,北部地震剖面解释的沉积体侧向迁移特征,建立了走滑拉分构筑的可容空间变化型式。此沉积对构造的响应模式,不仅可以很好的解释拼合砂体的分布,古流向偏转等问题,而且对于预测盆内沉积体走向也是一个很有用的工具。     

Tracking Galaxy Evolution Through Low-Frequency Radio Continuum Observations using SKA and Citizen-Science Research using Multi-Wavelength Data

We present a brief review of progress in the understanding of general spiral and elliptical galaxies, through merger, star formation and AGN activities. With reference to case studies performed with the GMRT, we highlight the unique aspects of studying galaxies in the radio wavelengths where powerful quasars and bright radio galaxies are traditionally the dominating subjects. Though AGN or quasar activity is extremely energetic, it is extremely short-lived. This justify focussing on transitional galaxies to find relic-evidences of the immediate past AGN-feedback which decide the future course of evolution of a galaxy. Relic radio lobes can be best detected in low frequency observations with the GMRT, LOFAR and in future SKA. The age of these relic radio plasma can be as old as a few hundred Myr. There is a huge gap between this and what is found in optical bands. The very first relic-evidences of a past quasar activity (Hanny’s Voorwerp) was discovered in 2007 by a Galaxy Zoo citizen-scientist, a school teacher, in the optical bands. This relic is around a few tens of thousand years old. More discoveries needed to match these time-scales with star formation time-scales in AGN host galaxies to better understand black hole galaxy co-evolution process via feedback-driven quenching of star formation. It is now well-accepted that discovery and characterization of such faint fuzzy relic features can be more efficiently done by human eye than a machine. Radio interferometry images are more complicated than optical and need the citizen-scientists to be trained. RAD@home, the only Indian citizen-science research project in astronomy, analysing TIFR GMRT Sky Survey (TGSS) 150 MHz data and observing from the Giant Meterwave Radio Telescope (GMRT), was launched in April 2013. Unique, zero-infrastructure zero-funded design of RAD@home as a collaboratory of 69 trained e-astronomers is briefly described. Some of the new-found objects like episodic radio galaxies, radio-jet and companion galaxy interaction, radio galaxy bent by motion of the intra-filament medium in a Mpc-scale galaxy filament etc. are briefly presented as demonstration of its potential. Citizen-science has not only opened up a new way for astronomy research but also possibly the only promising way to extract maximum science out of the Big Data in the SKA-era. This possibly can convert the Big Data problem into a prospect. Citizen-science can contribute to the knowledge creation in never-seen-before speed and in approach. As it is based on internet, it can provide an equal opportunity of academic-growth to people even in the under-developed regions where we always need to put our optical and radio telescopes. This can liberate the research-activity of city-based research-institutes out of the four brick walls and alleviate various socio-economic and geo-political constraints on growth of citizens educated in undergraduate-level science but located in remote areas.     

河南栾川火神庙钼矿床辉钼矿Re-Os同位素年龄及其地质意义

火神庙矽卡岩型钼矿床是东秦岭钼矿带栾川矿集区近些年查明的一个中型钼矿床,钼矿体主要赋存于火神庙复式岩体与新元古界蓟县系三川组大理岩接触带的矽卡岩中。为厘定火神庙钼矿床的成矿时代、成矿物质来源及与南泥湖—三道庄、上房沟钼矿床的关系,采用ICP-MS辉钼矿Re-Os同位素定年法对6件辉钼矿样品进行成矿年龄测定,获得的模式年龄为146.1Ma±2.0Ma~148.1Ma±2.1Ma,年龄加权平均值为147.01Ma±0.95Ma,等时线年龄为145.7Ma±3.9Ma,表明火神庙钼矿床形成于晚侏罗世。辉钼矿样品的Re含量为39×10-6~65.4×10-6,显示成矿物质来源于壳幔混源。火神庙钼矿床与南泥湖—三道庄、上房沟钼矿床均为栾川矿集区晚侏罗世第二次岩浆活动的产物,它的发现为在栾川矿集区西部寻找矿产资源提供了依据。     

重庆涪陵页岩气勘查开发区环境地质调查进展

紧密结合国家非常规能源勘探开发的重大战略,聚焦重庆涪陵页岩气勘查开发区环境地质调查工作,总结了研究区岩溶发育特征与分布规律,评价了涪陵页岩气开发区区域水资源量和地下水质量。在此基础上,收集分析国内外资料,梳理了页岩气勘查开发所引发的6类环境(地质)问题及勘查、钻井、压裂、开采、闭井等5个阶段需关注的地质环境问题或风险等,其中涪陵页岩气勘查开发区主要诱发水土污染、地质灾害和大气污染等环境(地质)问题; 基本识别了2种地下水污染模式、3种污染类型及可能的地下水污染风险途径; 初步确定了涪陵页岩气勘查开发区污染指示性特征因子,并形成了页岩气勘查开发区地质环境影响评价指标体系,可指导页岩气勘查开发的环境地质调查。该研究为页岩气国家新型清洁能源的绿色开发和开发区生态文明建设提供支撑。