康定杂岩时代及成因探讨

康定杂岩是康滇地轴上一套复杂岩系，由紫苏辉长质暗色杂岩、英云闪长质浅色杂岩及复成分混合杂岩构成。岩石结构构构造，铀、钍及稀土特表明，主体为岩浆杂岩，包含大量具层状痕迹的变质杂岩。大量的锆石Ｕ－Ｐｂ年龄及其它同位素年龄表明，岩浆岩属晋宁－澄江期。变质杂岩时代与河口群相当。     

成都粘土裂隙成因研究

根据成都粘土中裂隙特征与地质环境条件的分析，提出成都粘土中途中眩要裂隙类型的成因模式，上升剥蚀引起的垂向卸荷作用产生波状水平裂隙，冲沟切割引起的侧向卸荷作用，产生平行斜列隙裂。     

山东归来庄金矿区g(Au/Ag)的空间信息统计学特征

空间信息统计学是一门集数学、空间信息科学及计算机技术于一体,在时空域内对区域化变量的随机性与结构性进行定量研究的技术。以山东归来庄金矿床为例,对其g(AuAg)异常进行空间信息统计学研究。利用指示克立格法研究g(AuAg)的空间变异结构特征,建立空间结构模型。在对结构模型和估计方案进行交叉验证后,对g(AuAg)的空间分布进行估计。根据g(AuAg)的空间分布规律,探讨其与Au空间分布的关系,并对今后该区的找金工作提出建议。     

南秦岭金龙山微细浸染型金矿成矿时代

 金龙山金矿带是南秦岭新发现的卡林型金矿带,主要产于上泥盆统南羊山组细碎屑岩—碳酸盐岩建造中,在上泥盆统冷水河组、下石炭统碳酸盐建造中也有产出,可分为明显受断裂控制的脉型金矿化和受有利岩性及小规模断裂、节理控制的浸染型矿化。     

天然气的无机元素的土壤化探元素预测指标的探索

通过德阳新场气田化探成果与气田上有机元素异常，物探异常和钻孔实际见气的对比，以及对成都地区，宜宾地区化探成果的综合研究，认为As,Sb,Hb,Ba,Mn五元素及Cu,Pb,Zn,Mo,Cd,Ni,V,P等是预测天然气的指标，用该指标对新场气田和成都地区实际勘察结果对照，证实预测指标是正确的，从而探索出一条利用化探无机元素异常寻找天然气的新路。     

甘肃新生代气候环境变化与哺乳动物群演替

甘肃省境内新生代沉积中富含动物化石,以早渐新世晚期、晚渐新世、早中新世早期、中中新世晚期、晚中新世、早更新世和晚更新世的哺乳动物化石最为丰富.新生代青藏高原形成、快速隆升,改变了东亚的大气环流和中国的地理格局,使甘肃的气候和地理面貌发生了巨变.甘肃省境内的哺乳动物群在这些变化背景下发生了一次次的更替.本文通过对不同时代...     

河北省邯邢地区高岭石伊利石粘土矿床特征及找矿方向

邯邢地区高岭石、伊利石粘土矿赋存于石炭系本溪组、太原组,二叠系山西组、下石盒子组、上石盒子组的7个层位.矿体主要呈层状产出,厚度变化较大.矿石主要由片状高岭石组成,次要和少量矿物为绢云母、石英、黑云母等.矿床成因包括沉积矿床(如石炭-二叠系高岭石伊利石粘土矿)、风化残积矿床(如软质高岭石粘土矿床).该地区可划分出临城竹...     

北欧海的锋面分布特征及其季节变化

利用多年月平均格点数据分析了北欧海主要锋面的分布特征和季节变化规律,并讨论了月平均数据分析锋面适合使用的方法。月平均数据显示的锋面出现间断或多重的现象是锋面侧向摆动造成的,这是月平均数据的一大特点。北欧海各锋面主要水文和季节变化特征差异很大。东格陵兰极地锋在夏季锋面强度大,锋面较连续完整,而冬季强度小,锋面结构零散。9月由于东格陵兰寒流势力最强,可观察到温度梯度较大且连续的东格陵兰锋。北极锋的季节变化在水平方向呈＂哑铃型＂分布,中段摆动较南北两端小。由于挪威海流在冬季出现的最大流量引起挪威海流的流幅在该处加宽,莫恩海脊锋冬季向西北移动,对前人文章中基本上没有季节性移动的说法进行了修正和补充。冰岛—法罗群岛锋随深度增加向南移动,锋面强度增强,这是溢流造成的。     

云南鹤庆蜡硅锰矿的矿物学特征

对云南省鹤庆锰矿的物质组成及工艺矿物学研究中首次发现,也是国内第一次发现的锰矿物—蜡硅锰矿[Mn_5Si_4O_(10)(OH)_6],进行了大量研究工作。现就蜡硅锰矿的矿物学特征作简要报道。     

Gas accumulation from oil cracking in the eastern Tarim Basin: A case study of the YN2 gas field

Oil and gas exploration in eastern Tarim Basin, NW China has been successful in recent years, with several commercial gas accumulations being discovered in a thermally mature to over-mature region. The Yingnan2 (YN2) gas field, situated in the Yingnan structure of the Yingjisu Depression, produces gases that are relatively enriched in nitrogen and C₂₊ alkanes. The δ¹³C₁ (−38.6‰ to −36.2‰) and δ¹³C₂ values (−30.9‰ to −34.7‰) of these gases are characteristic of marine sourced gases with relatively high maturity levels. The distributions of biomarkers in the associated condensates suggest close affinities with the Cambrian–Lower Ordovician source rocks which, in the Yingjisu Sag, are currently over-mature (with 3–4%Ro). Burial and thermal maturity modeling results indicate that paleo-temperatures of the Cambrian–Lower Ordovician source rocks had increased from 90 to 210 °C during the late Caledonian orogeny (458–438 Ma), due to rapid subsidence and sediment loading. By the end of Ordovician, hydrocarbon potential in these source rocks had been largely exhausted. The homogenization temperatures of hydrocarbon fluid inclusions identified from the Jurassic reservoirs of the YN2 gas field suggest a hydrocarbon emplacement time as recent as about 10 Ma, when the maturity levels of Middle–Lower Jurassic source rocks in the study area were too low (<0.7%Ro) to form a large quantity of oil and gas. The presence of abundant diamondoid hydrocarbons in the associated condensates and the relatively heavy isotopic values of the oils indicate that the gases were derived from thermal cracking of early-formed oils. Estimation from the stable carbon isotope ratios of gaseous alkanes suggests that the gases may have been formed at temperatures well above 190 °C. Thus, the oil and gas accumulation history in the study area can be reconstructed as follows: (1) during the late Caledonian orogeny, the Cambrian–Lower Ordovician marine source rocks had gone through the peak oil, wet gas and dry gas generation stages, with the generated oil and gas migrating upwards along faults and fractures to form early oil and gas accumulations in the Middle–Upper Ordovician and Silurian sandstone reservoirs; (2) since the late Yanshanian orogeny, the early oil accumulations have been buried deeper and oil has undergone thermal cracking to form gas; (3) during the late Himalayan orogeny, the seals for the deep reservoirs were breached; and the gas and condensates migrated upward and eventually accumulating in the relatively shallow Jurassic reservoirs.