Geochemical characteristics and geological implication of Zijinshan alkaline rocks in Lin County in the west of North China Craton

The Zijinshan rocks in Lvliang area of Shanxi Province, are one of the famous alkaline plutons in China. The petrography and petrogeochemistry of the main rocks of the rock mass were studied to explore the material source and geological significance of Zijinshan alkaline rock mass. The results show that Zijinshan rocks of all stages show characters of low silicon, rich alkali and high potassium, which indicates zijinshan rocks belong to potassium alkaline rocks. These rocks demonstrate a high degree of fractionation and are characterized by the richness of LREE and the poorness of HREE, without obvious Eu anomaly. The trace element pattern exhibits the enrichment of large ion lithophile elements, such as Rb, Ba, K and Sr, and relative depletion of high field strength elements, such as Th, Nb, Ta, La, Ce, Nd, P and Ti. The magma of Zijinshan rocks comes from a deeper source and is closely related to the enriched mantle. The mechanism of magma evolution is mainly partial melting and it may be inter-contamination of continental crust materials. Combined with the characteristics of alkaline and partial alkaline rocks of same age in many places in Shanxi, the authors deduce that the alkaline magma activity in the middle of North China during the Early Cretaceous is closely to the destruction of North China Craton under the background of the subduction of Pacific plate.     

The symbiotic star CH Cygni – I. Non-thermal bipolar jets

Very Large Array surface brightness and spectral index maps of the evolving extended emission of the triple symbiotic star CH Cygni are presented. These are derived from observations at 4.8, 8.4 and 14 GHz between 1985 and 1999. The maps are dominated by thermal emission around the central bright peak of the nebula, but we also find unambiguous non-thermal emission associated with the extended regions. Our observations confirm that this is a jet. The central region has been associated with the stellar components through Hubble Space Telescope imaging. If the jets are the result of ejection events at outburst, expansion velocities are consistent with those from other measurement methods. We propose that the non-thermal emission is caused by material ejected in the bipolar jets interacting with the circumstellar wind envelope. The resulting shocks lead to local enhancements in the magnetic field from the compact component of the order of 3 mG.     

Coherent Chemical Variation Trends of the 55-25 Ma Magmatic Rocks in SE Tibet:N-S Direction Lithospheric Stretching of Eurasia during Early Stage of India-Eurasia Collision

The progressive indentation of India into Eurasia generated an E–W-trending orthogonal collision belt and a N–S-trending oblique collision belt. Compiling available data reveals that ～70% of the Cenozoic igneous rocks in eastern and southeastern Tibet are concentrated within an ENE-trending, ～550-km long and ～250-km wide magmatic zone(CMZ) that once separated the orthogonal and oblique collision belts. The Latitude 26°N Line is now its southern boundary. The onset timing of magmatism of the CMZ ...     

渭河盆地岩石圈热结构模拟及其对地热系统热源机理的启示

深部温度场与岩石圈热结构特征是认识地热系统深部热源机理的重要途径。本文在系统分析渭河盆地及其邻区现今大地热流特征基础上,基于旬邑—西峡宽角反射/折射地震测深剖面揭示的地壳分层结构,采用二维有限元方法,对渭北隆起、渭河盆地以及北秦岭构造带的深部温度场和岩石圈热结构开展数值模拟研究,在此基础上分析渭河盆地地热系统深部热源机理。结果表明,旬邑—西峡剖面上大地热流介于57.6～75.7mW/m²之间,平均为(70.4±4.7)mW/m²;地幔热流在29.5～38.6mW/m²之间,平均值为34.1mW/m²;莫霍面温度变化范围约在600～740℃之间;“热”岩石圈厚度约为95～110km。从渭北隆起—渭河盆地—秦岭造山带,大地热流、莫霍面温度和地幔热流值表现出低→高→低的变化规律,相应地“热”岩石圈厚度则表现出厚→薄→厚的变化趋势。渭河盆地地壳厚度减薄明显,莫霍面温度显著高于渭北隆起和秦岭造山带,暗示着渭河盆地地壳活动性显著。然而,从渭北隆起—渭河盆地—秦岭造山带,“热”岩石圈厚度变化范围不大,且渭河盆地内...     

Mantle property of Hegenshan ophiolite in Inner Mongolia: Constrains from element geochemistry and Re-Os isotopes of harzburgiteSCIEI北大核心CSCD

贺根山蛇绿岩带是中亚造山带东部出露面积最大的晚古生代蛇绿岩带,然而研究者对它是大洋岩石圈的残余还是陆内岩石圈地幔伸展的产物仍存在较大争议,主要归因于一直缺少橄榄岩Re-Os同位素的有效制约。基于此,本文对贺根山蛇绿岩中方辉橄榄岩进行了系统的岩石学、地球化学和Re-Os同位素研究。方辉橄榄岩主要由橄榄石、斜方辉石、粗粒的铬尖晶石和少量单斜辉石组成。贺根山方辉橄榄岩具有难熔地球化学特征,显示出高的MgO(45.1%~48.1%)含量,低的CaO(0.09%~0.26%)和Al 2O 3(0.58%~0.90%)含量及Tb/Yb比值,低于原始上地幔的^(187)Os/^(188)Os(0.1236~0.1263)同位素组成;橄榄石具有较高的Fo值(91.0~91.7)和NiO含量(0.26%~0.48%),而且单斜辉石具有低的重稀土含量,暗示了贺根山方辉橄榄岩是尖晶石相陆下岩石圈地幔高程度(20%~30%)部分熔融的难熔残余。另外,方辉橄榄岩相对富集LREE和大离子亲石元素,亏损高场强元素(例如Nb、Ta),且单斜辉石具有高Ti/Eu值和低的La/Yb,揭示了地幔源区受到硅酸盐熔体交代作用的改造。另一方面,方辉橄榄岩显示出相对年轻的Re亏损模式年龄,t RD为454~825Ma,表明贺根山地区岩石圈地幔形成的时代应该在0.8Ga之前,而后经历过多期熔体抽离和交代,与区域上大规模地壳增生时代吻合,可能是罗迪尼亚超大陆裂解的响应。结合蛇绿岩中大量深源矿物(金刚石等)和捕获锆石的存在、南北两侧一致的地质记录,本文认为贺根山方辉橄榄岩可能是陆内伸展环境下深部地幔物质上涌减压熔融的产物。     

Thermal doming-extension metallogenic system of Jiaodong type gold depositsSCIEI北大核心CSCD

胶东型金矿具有独特的成矿特征和成因机制,不同于国际已知金矿类型。为了深化认识控制矿床形成、变化和保存的地质要素及成矿过程,本文综合分析了胶东半岛晚中生代岩浆作用、构造活动和成矿特征及其构造背景,提出该区深部岩浆活动与地壳快速隆升及浅部变质核杂岩、张性断层、断陷盆地等伸展构造,共同控制了以Au为主的矿床成矿系列及成矿演化过程,谓之热隆-伸展成矿系统。阐明了晚中生代岩浆演化过程中的元素变化规律,发现了金矿化蚀变带中的低Ba、Sr含量异常及早白垩世胶东地壳中金丰度的显著变化,揭示了壳幔物质混合和伟德山型花岗岩岩浆活动对金成矿的贡献。认为这一成矿系统形成于古太平洋板块俯冲后撤的后俯冲伸展环境,由于软流圈上涌导致岩石圈地幔性质由富集向亏损转化,从而引起岩浆岩地球化学特征变化,地球化学元素重新调整,幔源含金流体与由重熔下地壳析出的壳源含金流体混合形成富金流体库,并产生贫金花岗岩。大规模岩浆活动为成矿元素的活化、迁移提供了热动力条件,上地壳伸展产生的断裂构造则为成矿元素聚集提供了良好空间。热隆-伸展成矿系统是中国东部晚中生代重要的成矿系统。     

基于斯通利波及电成像测井数据对火成岩裂缝地层的特征分析

随着石油勘探类型的转变和发展,如何高效且准确地识别地层中的裂缝变得十分重要。本文构建了斯通利波在裂缝地层中传播的理论模型,得到了斯通利波在经过裂缝带时会形成反射斯通利波,以及地层中裂缝的条数越多、斯通利波反射系数越大的理论结果。在此基础上,对辽河盆地火成岩地层的声波测井数据进行了斯通利波波场分离（中值滤波）,得到反射斯通利波,并计算了裂缝地层的反射系数。同时对该地层的电成像测井数据进行了孔隙度分布谱和区间孔隙度分析。研究表明：在裂缝发育的地层,反射斯通利波能量增强,反射系数变大;裂缝发育地层电成像孔隙度分布谱明显变宽,电成像区间孔隙度中大孔隙占比增大,显示次生孔隙（裂缝）发育。