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广平地震台地磁异常与地震关系的研究

利用加卸载响应比、日变幅逐日比、空间相关分析法,研究分析了广平台1982-2006年地磁垂直分量观测资料与河北省及邻近地区Ms≥5.0地震之间的关系,发现它们之间有较好的对应关系;同时给出了适用于广平地磁台的地震分析预报参数,为今后广平台依磁报震提供了依据.     

Formation of saddle dolomites in Upper Cambrian carbonates, western Tarim Basin (northwest China): Implications for fault-related fluid flow

The saddle dolomites occur more intensely in cores closely to fault than that in cores far away from the fault in Upper Cambrian carbonate of western Tarim basin, suggesting that formation of the saddle dolomites is likely related to fault-controlled fluid flow. They partially fill in fractures and vugs of replacement dolomite. The saddle dolomites exhibit complex internal textures, commonly consisting of core and cortex. In comparison with the matrix dolomites, the saddle dolomites show lower Sr-content and ⁸⁷Sr/⁸⁶Sr ratios, higher Fe- and Mn-content, and more negative δ¹⁸O values. Combined with high Th (100–130 °C) of primary fluid inclusions, it is suggested that the saddle dolomites precipitated from hydrothermal fluid derived from the deep evaporite-bearing Middle Cambrian strata, and the magnesium source may be due to dissolution of host dolomite during hydrothermal fluid migration. Fault activity resulted in petrographic and geochemical difference of the core and cortex of the saddle dolomites. The cores precipitated from the formation water mixed by deep brines at the early stage of fault activity, and the cortexes precipitated from the deep fluid with higher temperatures through the Middle Cambrian later. In summary, the formation of the saddle dolomites implies a hydrothermal fluid event related to fault activity, which also resulted in high porosity in Upper Cambrian carbonate in western Tarim Basin.     

大气能见度研究

回顾总结了国内外有关大气能见度的理论研究、仪器观测和数值模拟方面取得的成果;介绍大气能见度研究的基本理论、消光系数的概念及计算方法;总结了几种白天大气能见度探测仪的使用原理及优缺点;介绍测量夜间大气能见度和数字摄像法探测大气能见度的方法;并着重介绍4种计算与雾有关的大气能见度的经验公式,基于2004年4月11日黄海海雾个例的RAMS模式数值模拟结果,采用4种方法分别计算了大气能见度的分布并进行了比较。总结出大气能见度研究中存在的问题和今后研究的主要方向,并针对其中仍然存在的问题提出一些建议。     

准噶尔盆地西北缘扇体形成演化与扇体油气藏勘探

准噶尔盆地西北缘广泛发育二叠纪-侏罗纪冲积扇、水下扇、扇三角洲等砾质粗碎屑沉积,其形成演化严格受不同时期活动的同生断裂控制.二叠纪以乌尔禾组扇体最为发育,呈由盆缘向盆地方向逐渐增强的前展式推覆冲断及渐进式扇体迁移响应模式.三叠纪-侏罗纪以百口泉组、克拉玛依组扇体最为发育,呈由盆内向盆缘方向逐渐减弱的退覆式冲断活动及后退式扇体迁移响应模式.已知扇体油气藏主要富集于水下扇扇根及扇中、扇三角洲平原及前缘4个亚相带,及二叠系佳木河组、乌尔禾组、三叠系百口泉组、克拉玛依组、侏罗系八道湾组、头屯河组6个层位.二叠-三叠纪扇体含油层多、规模大、储量丰度高,侏罗纪扇体反之.受断裂、不整合、岩相岩性、物性4种因素控制,扇体主要形成断块、地层不整合及构造岩性油气藏.断阶带及扇根-扇中相带主要发育构造(断块)油藏,为扇体与断层相配置的垂向运聚成藏模式;斜坡区及扇中-扇缘相带主要发育岩性油藏,为扇体与不整合相配置的侧向运聚成藏模式.西北缘扇体成藏条件好,探明程度总体较低,剩余资源潜力大,进而指出了七大有利勘探区块和方向.     

基于地学信息图谱的河道、海岸线演变对黄河三角洲景观格局影响研究

本文利用1988、1998、2009和2016年四期遥感影像,运用GIS技术,将地学信息图谱的图形思维与景观生态学的定量思维相结合,以距今不同时期的亚三角洲和滨海湿地为研究区,从景观结构和景观演替两个方面探究黄河三角洲河道、海岸线演变对景观格局的影响。结果表明:(1)距今不同时间的河道对黄河三角洲景观结构的影响程度不同,距今时间越长的亚三角洲研究区内耕地占总面积的比例越大且耕地是亚三角洲研究区中的第一优势景观类型。在1855—1889亚三角洲研究区内,除耕地和建筑用地外,其他各类景观占总面积的比例都较小且随时间变化不明显;在1929—1934亚三角洲研究区内,盐田、养殖池占总面积的比例从2009年到2016年增加了近40%,涨幅明显;在1964—1976亚三角洲研究区内,各类景观占总面积的比例趋于平均;在2017至今的亚三角洲研究区内,耕地和光滩占总面积的比例较高,达到24%左右。(2)距今不同时间的海岸线对黄河三角洲景观结构的影响程度也不同,在1855滨海湿地研究区内,耕地占总面积比例为60%左右,而海域占总面积比例接近于0,极差较大;在1934和1974滨海湿地研究区内,光滩、柽柳、碱蓬群落、芦苇、白茅群落占总面积比例随时间变化几乎呈逐渐下降趋势,而建筑用地和盐田、养殖池则呈逐渐上升趋势;2009滨海湿地研究区,河流、人工水域占总面积比例在2009年和2016年均达到32%以上。(3)根据景观类型重心变化特征,分析河道、海岸线演变对景观演替的影响程度,将不同时期亚三角洲和滨海湿地研究区景观演替分为如下几类:亚三角洲人类活动主导型、废弃河道主导型、行水河道主导型、滨海湿地人类活动主导型、废弃海岸主导型、新海岸主导型。     

基于Mann-Kendall方法的胶东半岛海岸带归一化植被指数趋势分析

利用1998—2008年SPOT/VEGETATION逐旬共372期归一化植被指数时间序列影像数据,引入Mann-Kendall非参数趋势检验方法,分析了胶东半岛最近10 a来的归一化植被指数变化趋势。结果表明,最近10 a来,胶东半岛归一化植被指数变化趋势以衰减区域居主导地位,其中有明显衰减变化趋势的区域占半岛总面积的19.3%,有明显增强变化趋势的区域仅占半岛总面积的2.8%。归一化植被指数衰减区域在空间上沿海岸线呈环状分布,从沿海岸到远离海岸,归一化植被指数增强趋势逐渐明显,衰减最明显的区域大部分位于半岛沿海30 km以内,植被增强趋势最明显区域位于半岛中部山地及沿海防护林地区。人类活动及其空间分布是归一化植被指数变化的主要因素,其中沿海城市化、工业化和海岸湿地开发利用程度的提高导致归一化植被指数衰减,而山地植被保护和海岸防护林建设导致归一化植被指数增强。     

琼州海峡海底电缆路由工程地质特征

根据地球物理、声学探测、海底取样及实验室测试等实测资料详细分析,发现琼州海峡具有独特的自然条件以及复杂的工程地质特征。海底地形地貌非常复杂,存在沙波、沙堤沙丘、冲刷槽、冲刷脊和丘状突起、陡坡、滑坡、珊瑚礁、浅埋岩石、软弱地层等潜在的地质灾害因素,尤其在琼州海峡中央深槽区,坡度很大,分布着多种潜在的地质灾害,是海底光缆的危险区,应引起重视。     

Early Cretaceous Metasomatized Lithospheric Mantle beneath the Central Jiangnan Orogen in South China: Geochemical and Sr-Nd Isotope Evidence from the Tuanshanbei Dolerite

It is well established that Cretaceous magmatism in the South China Block (SCB) is related to the Paleo-Pacific subduction. However, the starting time and the associated deep crust-mantle processes are still debatable. Mafic dike swarms carry important information on the deep earth (including mantle) geodynamics and geochemical evolution. In the Jiangnan Orogen (South China), there is no information on whether the Mesozoic magmatic activities in this region are also directly related to the Pacific subduction or not. In this study, we present detailed zircon U-Pb geochronological, whole-rock element and Sr-Nd isotope data for Early Cretaceous Tuanshanbei dolerite dikes, and provide new constraints on the condition of the lithospheric mantle and mantle dynamics of the SCB during that time. LA-ICP-MS zircon U-Pb dating suggests that this dolerite erupted in the Early Cretaceous (~145 Ma). All samples have alkaline geochemical affinities with K2O + Na2O = 3.11–4.04 wt%, K2O/Na2O = 0.50–0.72, and Mg# = 62.24–65.13. They are enriched in LILE but depleted in HFSE with higher initial 87Sr/86Sr ratio (0.706896–0.714743) and lower εNd(t) (?2.61 to ?1.67). They have high Nb/U, Nb/La, La/Sm and Rb/Sr, and low La/Nb, La/Ta, Ce/Pb, Ba/Rb, Tb/Yb and Gd/Yb ratios. Such geochemical signatures suggest that the fractional crystallization is obvious but crustal contamination play a negligible role during magmatic evolution. Tuanshanbei dolerite were most likely derived from low-degree (2%–5%) partial melting of a phlogopite-bearing mantle material consisted of ~85% spinel peridotite and ~15% garnet peridotite previously metasomatized by asthenosphere-derived fluids/melts with minor subduction-derived fluids/melts. Slab-rollback generally lead to the upwelling of the hot asthenosphere. The upwelling of asthenosphere consuming the lithospheric mantle by thermo-mechanical-chemical erosion. The lithospheric mantle may have partially melted due to the heating by the upwelling asthenosphere and lithospheric extension. It is inferred that the Tuanshanbei dolerite might be associated with the initial slab rollback and corresponding lithospheric extension occurred potentially at ca. 145 Ma.