石羊河流域近50 a来日照时数的时空变化特征分析

 基于石羊河流域5个气象站点1959—2008年的日照时数资料,采用气候倾向率分析、Kriging空间插值、Mann-Kendall检验、小波分析等方法对石羊河流域日照时数的变化特征进行了分析。结果表明,近50 a来,石羊河流域年日照时数呈显著增加趋势,其变化倾向率为33.9 h/10a;四季日照时数均呈增加趋势,春季增加最显著,对年日照时数的贡献率最大,冬季次之。石羊河流域日照时数空间差异显著,表现为年日照时数自南向北递增。突变分析表明,1987年为日照时数的突变年。Morlet小波分析表明,石羊河流域年日照时数存在8 a的显著周期。     

广东“18.8”季风槽极端降水事件对流尺度集合预报分析

受季风槽影响,2018年8月30—31日华南地区出现一次极端暴雨过程,单日站点累计降水量达1?056.7 mm,刷新了广东有历史纪录以来新的极值。对于此次极端降水事件,常用的业务模式包括欧洲中期天气预报中心全球模式（ECMWF）、日本气象厅谱模式（JMA）和中国气象局广东快速更新同化数值预报系统（CMA-GD）,都低估了降水强度。利用深圳市气象局业务对流尺度集合预报系统分析了此次特大暴雨过程,结果表明：对流尺度集合预报系统对本次特大暴雨过程具有比较好的预报能力,概率匹配平均最大雨量达348.7 mm·(24 h)-1,集合平均的强降水中心和观测基本一致,观测极值附近区域发生大暴雨（≥150 mm）概率最大值达到80%。选取了较“好”和较“差”集合成员预报进行对比分析,发现较“好”成员预报的强降水中心位置和观测基本一致,而较“差”成员预报的降水中心位置则偏向福建地区。较 “好”成员预报出莲花山南侧地面中尺度辐合线较长时间的维持和缓慢移动,导致强降水雨团在莲花山脉附近不断地触发和维持,同时地形的阻挡作用使得对流系统在地形附近区域持续维持,造成了罕见的特大暴雨;而较“差”成员辐合区位于莲花山以北,对流形成后向东、向北移动,最终导致强降水预报位置偏向福建地区。     

针对一次对流云降水反演大气垂直运动速度及雨滴谱

反演大气垂直速度和雨滴谱分布是研究云降水机制和云微物理信息的重要内容,对人工预报天气、干预天气都有重要意义。针对2021年8月29日安徽省内毫米波雷达探测到的一次对流云降水过程,处理毫米波雷达的功率谱数据并进行大气垂直速度和雨滴谱反演。在小粒子示踪法的基础上引入改进小粒子示踪法：选取有效云信号段中最小功率对应的谱点作为反演大气垂直速度的示踪物。首先,根据改进前后的小粒子示踪法分别从功率谱数据中反演大气垂直速度,并跟基数据反演大气速度的结果展开对比分析。进一步得到粒子在静止空气中的下落速度,根据现有粒子下落速度-粒子直径之间的经验公式计算反演粒子直径。研究表明：(1) 采用改进后的小粒子示踪法反演大气垂直速度得到的结果比小粒子示踪法得到的结果更精确,在云层内部两者误差较大;(2) 进一步得到粒子下落速度,结合探测时段的天气状况,得到的粒子速度与大气速度可很好地契合,跟对流云天气情况信息大致吻合;(3) 粒子浓度是反演雨滴谱分布时需要注意的主要参数,云在快速发展过程中,内部粒子持续朝外部扩张,云内部的粒子浓度较小,云边界的粒子浓度反而较大。     

隧道与临近地面结构动力相互作用规律数值模拟

通过建立不同场地条件下隧道-土-上部结构相互作用的模型,研究有、无上部结构存在、场地条件和地震波频谱特性对隧道-土-上部结构体系地震响应的影响.计算结果表明:(1)对于隧道等地下结构,其地震响应主要受场地条件影响,不同场地条件隧道动内力值相差巨大,设计时应引起足够重视,相比之下有、无邻近上部结构对其影响较小;(2)S波...     

Depositional processes on oceanic island shelves – Evidence from storm‐generated Neogene deposits from the mid‐North Atlantic

Oceanic islands – such as the Azores in the mid‐North Atlantic – are periodically exposed to large storms that often remobilize and transport marine sediments along coastlines, and into deeper environments. Such disruptive events create deposits – denominated tempestites – whose characteristics reflect the highly dynamic environment in which they were formed. Tempestites from oceanic islands, however, are seldom described in the literature and little is known about storm‐related sediment dynamics affecting oceanic island shelves. Therefore, the geological record of tempestite deposits at oceanic islands can provide invaluable information on the processes of sediment remobilization, transport and deposition taking place on insular shelves during and after major storms. In Santa Maria Island (Azores), a sequence of Neogene tempestite deposits was incorporated in the island edifice by the ongoing volcanic activity (thus preserved) and later exposed through uplift and erosion. Because it was overlain by a contemporary coastal lava delta, the water depth at the time of deposition could be inferred, constituting an excellent case‐study to gain insight on the still enigmatic processes of insular shelf deposition. Sedimentological, palaeontological, petrographic and palaeo‐water depth information allowed the reconstruction of the depositional environment of these sediments. The sequence typifies the characteristics of a tempestite (or successive tempestites) formed at ca 50 m depth, in a steep, energetic open insular shelf, and with evidence for massive sediment remobilization from the nearshore to the middle or outer shelf. The authors claim that cross‐shelf transport induced by storm events is the main process of sediment deposition acting on steep and narrow shelves subjected to high‐energetic environments, such as the insular shelves of open‐sea volcanic islands.     

新疆准噶尔北缘托斯巴斯套铁铜金矿床矽卡岩和磁铁矿矿物学特征及其地质意义

托斯巴斯套铁铜金矿床赋存于中泥盆统北塔山组火山岩与闪长(玢)岩的接触带中,矿体呈脉状、透镜状,矿体及其周围发育大量矽卡岩.本文分别利用电子探针、电感耦合等离子体质谱法(ICP-MS),对托斯巴斯套铁铜金矿附近的石榴子石、辉石、绿帘石的化学组分及磁铁矿的主量及微量元素开展研究.结果表明:矽卡岩矿物中石榴子石端员组分以钙铝榴石一钙铁榴石系列为主,辉石端员组分以透辉石为主,绿帘石化学成分富铁富钙,这些特点表明矿区矽卡岩具有钙矽卡岩特征.矽卡岩是由岩浆热液流体交代北塔山组基性火山岩而形成的,磁铁矿的形成与矽卡岩的退化变质作用有关.在石英-硫化物-碳酸盐阶段形成铜和金矿化.     

恰什坎萨伊沟玄武岩年代学、地球化学特征及其对北阿尔金洋盆闭合过程的制约

北阿尔金恰什坎萨伊沟红柳泉以南早古生代蛇绿岩剖面发育两段玄武岩岩片.北段玄武岩锆石LA-ICP-MS U-Pb定年与前人对南段玄武岩定年结果(晚奥陶世)相近,表明该玄武岩形成于中—晚奥陶世;样品TR050-10-1锆石热干扰年龄为421～412 Ma、395～388 Ma和283～228Ma,TR050-13-1锆石热干扰年龄为442～434Ma、415Ma和241～221Ma.地球化学特征显示北段玄武岩和南段玄武岩的岩浆演化过程中均以单斜辉石结晶分异为主,仅表现极轻微地壳物质混染;二者均来自尖晶石二辉橄榄岩地幔源区,前者源区为原始尖晶石二辉橄榄岩相,后者源区为原始—亏损尖晶石二辉橄榄岩过渡相,前者的部分熔融程度更高.微量元素、稀土元素及构造判别图解指示其为形成于聚合背景下的E-MORB型拉斑玄武岩,具弧后盆地性质.结合区域资料,提出北阿尔金早古生代洋盆4阶段闭合模式:①早期俯冲阶段(∈2～O1),②晚期俯冲阶段(O1～O3),③俯冲-碰撞转换阶段(O3～S2),④后碰撞造山阶段(S3～D2).     

川东北地区三叠系飞仙关组白云化流体的Ca/Mg比定量估算

作为川东北地区三叠系飞仙关组天然气气藏最重要储集岩的粒屑白云岩和结晶白云岩的成因始终是沉积和石油地质学家高度关注的研究热点之一.在总结川东北地区三叠系飞仙关组不同类型白云岩形成温度的基础上,通过已有的白云化流体Ca/Mg值和温度之间关系式获得了川东北地区三叠系飞仙关组白云化流体的Ca/Mg值的主要分布范围.结果表明:不同类型白云岩对应的白云化流体具有不同的Ca/Mg值,同时证实了三叠纪海水或与之有关的海源流体、三叠纪海水与大气淡水混合流体的Ca/Mg值都符合在40～130℃区间、甚至更高温度下白云化(白云石沉淀)作用的要求,微晶白云岩和具原始结构的粒屑白云岩可能与地表—近地表的低温、小Ca/Mg值混合流体中相对快速的白云石沉淀作用有关,并形成了相对细的他形白云石;结晶白云岩(包括结构类似的过渡岩石类型、白云石胶结物)可能与埋藏的高温、大Ca/Mg值三叠纪海水或与之有关的海源流体中相对缓慢的白云石沉淀作用有关,并形成了相对粗的自形白云石.白云化流体的Ca/Mg值估算,可望为川东北地区三叠系飞仙关组优质储层白云岩的成因研究提供一些有价值的基础资料.     

新疆北山地区两个含铜镍镁铁—超镁铁质岩体铂族元素地球化学研究

对北山地区坡一和罗东含铜镍的镁铁-超镁铁质岩体铂族元素研究表明,两个岩体的铂族元素(PGE)总量较低,PPGE较IPGE富集,原始地幔标准化模式呈正斜率,均较原始地幔亏损,具Ir和Rh的弱负异常。较低的Pd/Ir比值表明岩石主要受岩浆作用控制,后期热液作用影响不明显。两个岩体的原生岩浆均为MgO 含量较高的PGE不亏损的拉斑玄武质岩浆,较高的Cu/Pd、Ti/Pd比值表明岩浆在演化过程中发生了硫化物的熔离。罗东岩体早期矿物相（橄榄石、铬铁矿）的分离结晶作用对岩浆中的硫达到饱和具有重要的贡献,而坡一岩体该作用对硫化物熔离的贡献不明显。坡一和罗东岩体的R值表明两岩体均具有达到中型Ni矿床的潜力。     

Contribution of mantle components within juvenile lower-crust to collisional zone porphyry Cu systems in Tibet

Most porphyry Cu–Mo–Au deposits are found in magmatic arcs worldwide, and are associated with hydrous, high-fO₂, calc-alkaline magmas, derived from a mantle wedge that was metasomatized by the fluids from a subducted oceanic slab. Recently, such deposits have been documented as occurring widely in collisional settings, where they are associated with potassic magmas generated during the collisional process, but the genesis of the fertile magmas and the mechanism of metallic enrichment remain controversial. Here we present new geochemical and Sr–Nd–Hf isotopic data from the post-collisional fertile and barren porphyries of the Miocene Gangdese porphyry belt in the Tibetan orogen, an orogen formed by the collision of India and Asia in the early Cenozoic. Both types of porphyry are characterized by high K₂O contents, and have geochemical affinities with adakite, but the fertile magmas were most likely derived from the melting of a thickened juvenile mafic lower-crust, formed by the underplating of earlier asthenospheric melts at the base of crust, whereas the derivation of the barren magmas involved variable amounts of old lower-crust in Tibet. The melting of sulfide-bearing phases in the juvenile mantle components of the Tibetan lower-crust probably provided Cu, Au, and S to the fertile magmas. The breakdown of amphibole during melting at the source released the fluids necessary for the formation of the porphyry Cu deposits in Tibet. The thickened crust (up to 70–80 km), due to collision, is thought to be responsible for a decrease in the fO₂ of the fertile magmas during their ascent to the upper crust, thus preventing the generation of more porphyry Cu–Au and epithermal Au deposits in this collisional zone.