小兴安岭西北部霍龙门地区花岗质杂岩锆石U--Pb年龄、岩石地球化学特征及地质意义

小兴安岭西北部的霍龙门地区位于兴蒙造山带东段,该区出露的大面积花岗质杂岩为新开岭—科洛杂岩的重要组成部分。该花岗质杂岩主要由花岗质和花岗闪长质糜棱岩等组成,其中花岗质糜棱岩的SHRIMP锆石U--Pb定年结果为310.7±6.5 Ma,表明其原岩形成于晚石炭世。该杂岩的主量元素总体显示中、高钾钙碱性准铝质--过铝质系列岩石的特点;微量元素表现出Th、Zr、Hf、Nd、Rb、K明显富集,而Ba、Sr、Nb、P、Ti明显亏损;稀土元素具有明显的轻稀土元素富集、重稀土元素相对亏损的特征,有较明显的负Eu异常,轻、重稀土元素分馏程度较强。结合区域构造演化特点及花岗质杂岩的形成环境等,综合显示该杂岩的原岩应形成于晚古生代,于三叠纪时期发生明显的变质变形作用。     

黄土高原黄土地层的对比及细分

将前人对黄土高原黄土地层划分的研究成果进行全面总结、分析,结合洛川、宝鸡、西峰3个经典剖面,利用土壤 地层学、沉积学、磁性地层学、古生物学、年代学、地球化学等研究方法对黄土高原的黄土地层进行详细对比以及进一步 细分。将早、中更新世界线调整为B/M极性倒转开始的对应层位——L9顶部。根据岩性和气候旋回周期的差异性等,将离 石黄土三分,S8/L9作为离石黄土内部划分的一条新界线,S1~L5划分为上离石黄土,S5~S8划分为中离石黄土,L9~L15划分为 下离石黄土。在分析过程中发现关键层位（S0,L1,S1,S5,L9,L15,L33） 的年龄具有差异性。     

地质非结构化数据研究战略——以JPG图件为例

从大数据时代背景出发,提出研究地质非结构化数据的战略意义。通过分析地质数据的特点,发现其大数据性。以JPG图件为例,展开国内外研究现状分析和行业应用分析。最后通过分析地质JPG图件数据的使用情况,提出地质JPG图件数据战略规划。     

华北地块南缘花山、五丈山岩体LA-ICP-MS锆石U-Pb年龄、地球化学特征及成因

花山复式岩体位于华北地块南缘,采用LA-ICP-MS技术测得复式岩体中的中细粒似斑状黑云二长花岗岩的锆石U-Pb年龄为128±1Ma,此年龄被解释为成岩年龄。该岩体及邻近的五丈山岩体中花岗岩具有高硅、富碱特征,为准铝-弱过铝质高钾钙碱性系列;在稀土和微量元素上,富集LREE、Rb、Ba、K、Sr等大离子亲石元素,亏损HREE、Zr、Hf、Ta、Nb、P、Ti等高场强元素,总体上Eu异常不明显,显示出I-A过渡型花岗岩的特征。锆石Lu-Hf同位素组成表明,花山花岗岩的ε_Hf(t)主要变化于-25.8~-19.6之间,t_DM2为2.81~2.43Ga,显示源区物质以古老的壳源物质为主,有年轻组分的参与。与岩体外围多金属成矿年龄的对比分析发现,外围金、钼矿床与花山复式岩体的年龄一致,比五丈山岩体晚20~25Ma,表明金、钼矿的形成与花山岩体在时空上联系密切,该岩体可能为成矿提供了热源。     

北秦岭柳叶河盆地石炭系—二叠系含砾砂岩碎屑锆石LA-ICP-MS U-Pb年龄及其地质意义

通过北秦岭黑河地区柳叶河盆地碎屑锆石年龄研究,探讨盆地沉积物年龄结构,并进一步推断其物源及与秦岭造山带的盆山耦合过程。采自柳叶河盆地石炭系—二叠系含砾砂岩样品中的82颗碎屑锆石年龄可分为6组:260~542Ma、800~1100Ma、1320~1560Ma、1640~2250Ma、2300~2660Ma和2720~2870Ma。其中260~542Ma年龄段所占测点比例最大,占锆石总数的31%,其次为1640~2250Ma、2300~2660Ma和800~1100Ma年龄段。最老年龄值为2834±40Ma,最年轻者为264±5Ma。从碎屑锆石年龄结构对比及石炭纪地层交错层理推断,柳叶河盆地石炭系—二叠系物源区主要为当时的北秦岭山地。此外,碎屑锆石年龄结构对比表明,鄂尔多斯盆地南部与柳叶河原始盆地有相同的年龄谱特征,意味着它们具有同一物源区。北秦岭山地是在加里东造山作用后期影响下迅速隆升而形成的。其后,随着南侧勉略洋的打开,华北地台相对沉降及沿商丹带的走滑断陷使柳叶河盆地出现,仍旧处于隆升状态的北秦岭山地开始作为该盆地及其北侧鄂尔多斯盆地南部的主要物源区。     

柴北缘尕秀雅平东和红柳沟北镁铁-超镁铁质岩体锆石U-Pb年龄及其找矿意义

位于柴达木地块北缘构造带内欧龙布鲁克微陆块东缘的2个镁铁-超镁铁质岩体——含Cu-Ni的尕秀雅平东岩体和含Ti-Fe的红柳沟北岩体,前者的LA-ICP-MS锆石U-Pb年龄为408.0±1.5Ma,属早泥盆世;后者的SHRIMP锆石U-Pb年龄为418.3±2.8Ma,属晚志留世。区域地质资料研究表明,东昆仑地区、柴北缘在晚志留世—晚泥盆世处于后造山伸展阶段,尕秀雅平东岩体和红柳沟北岩体正是拉张环境下幔源岩浆活动的产物。在东昆仑地区、柴北缘发现的铜镍矿床和铜镍矿点(除夏日哈木有争议外)基本都形成于晚志留世—晚泥盆世。结合区域成矿年代学研究,认为晚志留世—晚泥盆世期间,东昆仑造山带和祁连造山带之间的柴达木地块、欧龙布鲁克微陆块,以及位于这两大造山带内部的微型古陆块区,是形成岩浆铜镍硫化物矿床和钛铁氧化物矿床的有利环境。     

Quantifying the variability and allocation patterns of aboveground carbon stocks across plantation forest types,structural attributes and age in sub-tropical coastal region of KwaZulu Natal,South Africa using remote sensing

Quantifying the variability and allocation patterns of aboveground carbon stocks across plantation forests is central in deriving accurate and reliable knowledge and understanding of the extent to which these species contribute to the global carbon cycle and towards minimizing climate change effects. The principal objective of this study was to quantify the variability and allocation patterns of aboveground carbon stocks across Pinus and Eucalyptus plantation forests, tree-structural attributes (i.e. stems, barks, branches and leaves) and age groups, using models developed based on remotely sensed data. The results of this study demonstrate that aboveground carbon stocks significantly (α = 0.05) vary across different plantation forest species types, structural attributes and age. Pinus taeda and Eucalyptus grandis species contained aboveground carbon stocks above 110 t C ha⁻¹, and Eucalyptus dunii had 20 t C ha⁻¹. Across plantation forest tree structural attributes, stems contained the highest aboveground carbon stocks, when compared to barks, branches and leaves. Aboveground carbon stock estimates also varied significantly (α = 0.05) with stand age. Mature plantation forest species (i.e. between 7 and 20 years) contained the highest aboveground carbon stock estimates of approximately 120 t C ha⁻¹, when compared to younger species (i.e. between 3 and 6 years), which had approximately 20 t C ha⁻¹. The map of aboveground carbon stocks showed distinct spatial patterns across the entire study area. The findings of this study are important for understanding the contribution of different plantation forest species, structural attributes and age in the global carbon cycle and possible climate change moderation measures. Also, this study demonstrates that data on vital tree structural attributes, previously difficult to obtain, can now be easily derived from cheap and readily-available satellite data for inventorying carbon stocks variability.     

胶西北地区北截金矿闪长玢岩锆石SHRIMP年龄及其地质意义

山东省招远市北截金矿是胶西北地区发现较早的金矿之一,主要赋存于严格受NEE向断裂控制的黄铁绢英岩化蚀变带内,是典型的破碎带蚀变岩型金矿。本文通过对矿区内切穿矿体的闪长玢岩、郭家岭序列下属北截岩体的地质背景和SHRIMP锆石U-Pb年代学研究,得出闪长玢岩形成年龄为117±2Ma,北截岩体形成年龄为129±1Ma,限定北截金矿成矿年龄在117~129Ma之间,属早白垩世。锆石样品中测得Ar_3、Z、J_3等多个期次的继承锆石年龄,表明北截岩体和闪长玢岩形成过程具有多重继承演化性。根据同源岩浆的成岩成矿时间差及岩体与金矿的空间位置,判断郭家岭序列与金矿关系更为密切。讨论了胶东金矿的成矿期次和构造环境,认为其形成于俯冲造山带的弧后伸展环境,其形成与演化受中生代以来中国东部岩石圈大规模减薄、地幔上涌或陆缘裂谷的影响,最终成因可能与地幔柱有关。     

华北克拉通五台群LA-ICP-MS锆石U-Pb年龄和Hf同位素特征

通过对五台群石咀亚群金刚库组4个典型样品的LA-ICP-MS锆石U-Pb年龄和Hf同位素研究,对五台群的形成时代及华北克拉通新太古代—古元古代期间的地壳演化进行了探讨。锆石U-Pb同位素测定结果表明,侵入金刚库组中的片麻状花岗岩锆石的U-Pb年龄为2548Ma,因此五台群的上限年龄约为2.5Ga;金刚库组黑云母石英片岩和片麻状石英闪长岩的原岩锆石U-Pb年龄分别为2663Ma和2636Ma,因此五台群的下限年龄约为2.7Ga。五台群的地质年龄为2.5~2.7Ga,属于新太古代。锆石Hf同位素研究结果表明,黑云母石英片岩和片麻状石英闪长岩的二阶段Hf模式年龄(tDM2)均为2.8Ga左右,指示2.8Ga左右是五台山区乃至整个华北克拉通地壳生长的重要时期;片麻状花岗岩tDM2平均为2.57Ga,与锆石结晶年龄非常接近,表明2.5Ga左右也是华北克拉通地壳的主要增生期。地壳的增长是幕式的,2.8Ga和2.5Ga都是华北克拉通地壳生长时期。     

NGC 1624 (OCl 403, Cr 53) – A very young open cluster

We present the first CCD photometric UBVRI observations of the not-so-well-studied open cluster NGC 1624 (OCl 403, Cr 53; α₂₀₀₀ = 04 h 40 m 36 s; δ₂₀₀₀ = + 50^˚ 27^′ 42″ Trumpler class = I 2 p N). This cluster was observed on 01 February 2004 with the 2 m Himalayan Chandra Telescope at Hanle using a LN2 cooled 2k × 2k CCD. The cluster presents differential reddening with E(B-V) values ranging from 0.70 to 0.90 mag, which could be attributed to the presence of the HII region wherein the cluster is embedded. It is found to be at a distance of 6.025 ± 0.5 kpc and the age of this cluster is estimated to be ∼3.98 × 10⁶ years. In view of these parameters, it can be considered as a young enough cluster located in the direction of the Perseus constellation with the galactic coordinates of l = 155^˚.35 and b = + 02 ^˚.58. Thus it could also be used as a suitable candidate for tracing the Outer Perseus spiral arm of our Galaxy. The initial mass function slope is derived as 1.65 ± 0.25 by applying the corrections for field star contamination and data incompleteness. This is in good agreement with the Salpeter value within the limits of errors.