Regional Variability in Occurrence and Distribution of Polymetallic Nodules in the Central Indian Basin

Regional scale morphological studies on different-sized polymetallic nodules from the Central Indian Basin show that only 2–5 cm sized nodules have highest occurrence per station (92–94% along latitudes; 88–94% along longitudes). A nodule size shows an inverse relationship with the nodule distribution, grade, and abundance. Interestingly, only 3–4 and 4–5 cm sized nodules have highest grade, abundance, and distribution percentages along longitudes in P₁, first generation mine site and relinquished area, which further implies that the nodule mining along the longitude would be beneficial. Different-sized nodule groups suggest their formation under variable environmental conditions that existed in the Central Indian Basin. The coexistence of different-sized nodules suggests different environmental conditions existed in the Central Indian Basin.     

Episodic crustal growth in the Tanzania Craton: evidence from Nd isotope compositions

The analysis of available Nd isotope data from the Tanzania Craton places important constraints on the crust-mantle separation ages, and events marking juvenile crustal addition and crustal recycling. Nd model ages date the oldest crust extraction to 3.16 Ga in the Tanzania Craton, although a rock record of such antiquity is yet to be found there. The most significant period of juvenile crustal addition as well as crustal recycling is 2.7–2.6 Ga. The Nd isotopes of mafic samples show that chemical heterogeneity existed in the mantle beneath the Tanzania Craton, with some samples originating from significantly depleted mantle, and most samples originating from the mixture of primitive mantle and depleted mantle. The Nd isotope section reveals significant differences in Nd isotopes between the north craton and central craton; compared to the north craton, the central craton yields a Nd model age that is approximately 100 Ma older, and its ε_Nd(t) values are more negative, indicating that the two parts of the craton have different mantle source regions. Different types of granitoids are distributed in the Tanzania Craton, such as high-K and low-Al granite, calc-alkaline granite, peraluminous granite and transitional types of tonalite-trondhjemite-granodiorites (TTGs). Most of the granitoids formed later than the mafic rocks in syn-collision and post-collision events.     

Zircon SHRIMP U-Pb dating of the Neogene coral reefs,Xisha Islands,South China Sea: implications for tectonic evolution

The Xisha Block is a minor one in the South China Sea and an important tectonic unit in the northwestern part of the region. Zircon SHRIMP U-Pb ages for three volcanic intrusive core samples from Xike-1, an exploratory well penetrating the bioherms of the Xisha Islands. The core samples are from the Miocene reef carbonate bedrock and are recognized as dark-gray biotite-hornblende gabbro, gray fine-grained biotite diorite, and gray fine-grained granite, respectively. Zircon cathodoluminescence (CL) images and trace Th, U and Pb compositions of the zircons show that these rocks are of volcanic intrusive origin. Zircon SHRIMP U-Pb dating yielded six groups of ages, ranging from 2451-1857 Ma to early Cretaceous, which indicate that the formation and evolution of the Xisha Block was affected by the evolution and closure of Neotethys Ocean, probably within its eastern extension into South China Sea. Both old, deep-sourced material, including fragments from Rodina supercontinent, and recent mantle-derived magma products contributed to the emergence and formation of the Xisha block. The SHRIMP U-Pb results also proved that this process differed from that of the Kontum massif, the Hainan Block, and the South China Block, but is similar to that of the Nansha and Zhongsha blocks. The process was associated with the effects of Yanshanian magmatism induced by subduction mechanisms of the Paleo-Pacific Plate or the reworking of the multiple magmatisms since the Early to mid-Yanshanian, possibly jointly experienced by the Xisha-Zhongsha-Nansha Block.     

华夏陆块钠质高镁玄武岩地球化学特征及地质意义

赣州盆地位于钦杭(钦州—杭州)结合带南侧华夏陆块西部,由晚白垩世早期红色碎屑沉积岩系组成,其底部夹有一套玄武岩,全岩Si O_2含量为46.50%~48.13%,具有钠质高镁特征(Mg O=15.47%~18.24%,Mg~#=74~77,K_2O/Na_2O=0.22~0.39)。稀土元素配分型式表现出轻稀土富集右倾,没有明显的Eu异常的特点,表明岩浆没有明显的斜长石分离结晶作用;微量元素上富集大离子亲石元素,高场强元素特别是Ta、Nb、Ti亏损不明显,Cr、Ni的含量分别为235×10~(-6)~617×10~(-6)、157×10~(-6)~493×10~(-6),与原生岩浆的Cr、Ni含量接近,Ba/Nb值(13.51~23.18)和La/Nb值(0.82~1.03)表明源区有富集地幔组分;Sr—Nd—Pb—O同位素显示出源区性质具有EMⅡ型富集地幔特征。岩石学和地球化学特征表明,玄武岩具有原生岩浆性质,是富集地幔部分熔融的产物。同时为中生代华夏陆块EMⅡ型岩石圈地幔提供了准确的证据。由赣州盆地晚白垩世构造背景和构造环境判别图解可知,本区玄武岩形成于板内拉张环境,可能与古太平洋俯冲条件的转变有关。     

伊宁地块早石炭世球泡流纹岩的发现及地球化学特征

伊宁地块西段中部阿腾套山一带发现的球泡流纹岩,多数产于早石炭世海相无球泡流纹岩夹层中,整体呈层状、互层状,球泡通气孔顺层平行于流纹构造定向分布,推断是海相极浅水环境下的产物,因而具有精细指相意义。该球泡流纹岩与同期A型花岗岩类共生,属碱性岩类,SiO_2含量为69.18%~77.69%,K_2O大于4%,Al_2O_3为11.32%~16.24%,Ga/Al×10~4=2.1~7.8,∑REE=85.22×10~(-6)~348.8×10~(-6),(La/Yb)_N=6.7~14.8,相对富集轻稀土,δEu具明显负异常,稀土配分及大离子元素蛛网图均与A型花岗岩类地球化学特征总体相同。ε_(Hf)(t)均大于0(+12.5~+15.5),两阶段锆石Hf模式年龄大于锆石U-Pb年龄,表明源区可能为早古生代新生地壳物质部分熔融演化而来。A型球泡流纹岩与同期A型花岗岩类均形成于拉张构造环境,是区内早石炭世大哈拉军山组中迄今唯一发现的显示拉张构造环境的珍贵实例。为揭示和探讨伊宁地块总体处于汇聚大背景下的局部拉张环境,以及东窄西宽之楔形构造形态提供了可能。     

山西长治盆地中更新世气候转型期环境变化特征

中更新世气候转型(MPT)是第四纪环境变化的一个重要时期,该时期气候模式、气候周期等均发生了明显变化,然而不同区域对中更新世气候转型的响应特征存在明显差异.本研究选取了长治盆地XZK4钻孔中更新世转型前后(1.8～0.1 Ma)共207个样品,通过古地磁定年,运用粒度端元分析和孢粉分析,阐述了长治盆地中更新世转型期的环境变化与湖泊演化特征.结果显示,1.8 Ma以来,孢粉组合中乔木花粉含量多高于60％,但个别时段草本植物花粉占优,显示区域植被多数阶段为森林,但存在明显冷期,并且1.1 Ma和0.55 Ma是研究区环境转变的重要转折点.中更新世转型期前(～1.1 Ma):沉积物粒度总体较细,黏土含量多高于25％,EM1组分(湖相沉积)多高于60％,EM3(河流相组分)在个别时段出现,总体显示该阶段沉积物组成以湖相沉积为主,个别阶段受到河流影响大;中更新世转型时期(1.1～0.55 Ma):沉积物粒度较上一阶段更细,黏土含量(平均为30％)、EM1占比和孢粉浓度均达到研究段最高,沉积物颜色以棕灰色为主,EM3组分占比降至最低,其中1.1～0.95 Ma喜冷的云杉属花粉出现,显示该时期研究区气候总体偏冷湿,湖泊面积较1.1 Ma之前扩大;中更新世转型后(～0.55 Ma):沉积物粒度明显变粗,达到钻孔最高值,沉积物颜色变黄,EM2(风成组分)和EM3占主导,草本植物含量增加,尤其是喜干的蒿属花粉增加明显,表明气候较之前变干,沉积物类型以风力沉积为主,湖泊消亡.综合对比显示,构造运动是影响长治古湖消长的主要驱动力,气候变干加剧了湖泊消亡.     

安徽滁州和管店早白垩世高镁埃达克质侵入岩的成因:锆石U-Pb年代学和Sr-Nd-Hf同位素的制约

本文以华北陆块东部早白垩世滁州闪长玢岩和管店石英闪长岩为研究对象,报道了新的全岩地球化学（主量元素、微量元素以及Sr-Nd同位素）以及锆石U-Pb年代学和Hf同位素的综合研究结果,进而约束其岩石成因和构造意义。滁州闪长玢岩中锆石发育振荡环带,管店石英闪长岩中锆石具条痕状吸收的特点,它们均为岩浆成因。锆石LA-ICP-MS U-Pb定年结果显示,滁州和管店闪长质锆石年龄分别为128±1Ma和130±2Ma,表明二者均形成于早白垩世。地球化学特征显示,滁州和管店闪长质岩石具有类似的主量元素和微量元素组成,整体具中等的SiO₂含量（58.55%~60.12%）和富MgO（4.43%~5.10%,Mg^#=57~61）的特征,Na₂O/K₂O比值为1.20~1.47,属于高钾钙碱性系列岩石;富集轻稀土元素和大离子亲石元素（如Rb、Ba）,亏损重稀土元素和高场强元素（如Nb、Ta、Zr、Hf）,并具不同程度的Eu负异常（δEu=0.85~0.93）。它们具高的Sr（575×10^-6~1035×10^-6）和低的Y含量（10.2×10^-6~15.3×10^-6）以及高的Sr/Y比值（57~69）,属于埃达克质岩石。此外,滁州和管店闪长质岩石具有类似的Sr-Nd以及锆石Hf同位素的特征,滁州闪长玢岩的⁸⁷Sr/⁸⁶Sr初始比值介于0.7061~0.7066之间,ε_Nd（t）值为-17.7~-16.9,锆石ε_Hf（t）值变化于-23.1~-19.1之间,而管店石英闪长岩的⁸⁷Sr/⁸⁶Sr初始比值为0.7046~0.7059,ε_Nd（t）值为-18.7~-15.8,锆石ε_Hf（t）值为-25.6~-20.0。综合上述,滁州和管店闪长质岩石均属于高镁埃达克质岩石,起源于拆沉的加厚下地壳部分熔融的熔体与地幔橄榄岩反应的产物,形成于早白垩世华北东部陆块拆沉作用下的伸展背景。     

扬子地块西缘峨山新元古代A2型花岗闪长岩的成因及构造意义

在扬子地块西缘出露有大量的新元古代岩浆岩,这些岩石对于重建罗迪尼亚超大陆有着重要的意义。本文对云南峨山岩体的花岗闪长岩和似斑状黑云母二长花岗岩开展了详细的岩石学、岩石地球化学和年代学研究,结果表明,似斑状黑云母二长花岗岩侵位于826.6±2.5 Ma,而花岗闪长岩有着较年轻的结晶年龄818.3±2.8 Ma,花岗闪长岩比似斑状黑云母二长花岗岩有着更低的SiO₂含量,但是更高的Al₂O₃、MgO、Fe₂O₃、TiO₂和P₂O₅含量。在稀土元素配分曲线和微量元素蛛网图上,两种岩性呈现出相似的特征,都是具有右倾的稀土元素配分样式,呈现出Eu负异常,相对于大离子亲石元素（LILEs）更亏损高场强元素（HFSEs）。似斑状黑云母二长花岗岩富集Nd同位素组分,而花岗闪长岩与之有着相似的Nd同位素值。地球化学数据显示可能的岩石学成因是变质火成岩源区在826 Ma时发生部分熔融形成了峨山似斑状黑云母二长花岗岩并且残留下来了一个麻粒岩化的源区;麻粒岩源区在818 Ma时再次发生部分熔融形成了具有A型属性的峨山花岗闪长岩。结合前人的数据和本文的研究,认为扬子西缘在新元古代时期是一个活动大陆边缘,而华南地块当时在罗迪尼亚的位置更可能是在边缘而不是中心。     

一次拖曳型飑线过程雨滴谱演变特征研究

利用Thies激光雨滴谱仪观测资料和CINRAD/SA多普勒雷达观测资料,分析了2017年7月18日一次典型中纬度拖曳型飑线过程不同发展阶段雨滴谱和积分参数的演变特征,主要结果为：1）成熟飑线回波包括对流带、过渡区和拖曳层状云区三部分,对流带前侧不断有对流带生成并合并到主对流带中,使得对流带的前沿具有强的反射率因子,并且有多个雨强大值中心。2）垂直穿过飑线对流带,雨强增加阶段有较少的小粒子（直径小于1 mm）和特大粒子（直径大于5 mm）,以及较低的雨滴浓度和反射率因子,而雨强减弱阶段有较多的小粒子和特大粒子,以及较高的雨滴浓度和反射率因子;飑线加强阶段,雨滴谱有较大的峰值直径（0.44 mm）、较多的大（直径大于3 mm）和特大粒子,而飑线减弱阶段,雨滴谱有较小的峰值直径（0.19 mm）、较少的大粒子。3）对流带、过渡区和层状云降水雨滴谱的Gamma谱三参数N0、μ、λ随雨强增大有明显的分层特征,相同雨强时,对流云和过渡区降水的三参数比层状云降水的数值大;而飑线不同发展阶段、不同降水类型的λ-μ关系具有一致性,二次多项式可以很好地拟合λ-μ关系。4）归一化雨滴谱参数NW和D0的分布可以用来区分对流云和层状云降水,并给出了新的分离线方程;另外,飑线在发展和减弱阶段的雨滴谱特征有明显差异,表明飑线演变过程降水形成的微物理机制发生变化,前期冷云过程有重要影响,而后期暖云过程起主导作用。