福建龙海牛头山新生代玄武岩橄榄岩包体的水

对福建龙海牛头山新生代玄武岩中橄榄岩包体进行了傅利叶变换红外光谱(FTIR)分析,结果显示,二辉橄榄岩中的辉石包体含有结构水,均以OH的形式存在,结构水含量分别如下: 单斜辉石为(151~845)×10-6,斜方辉石为(40~710)×10-6,全岩为(25~90)×10-6.无论是辉石中的水含量还是全岩中的水含量,福建牛头山地区均高于华北克拉通的安徽女山、河北汉诺坝和苏北盆地,而与同是华北克拉通的河北阳原地区水含量相当.实验证明辉石是牛头山地区上地幔重要的水储库.初步推断福建牛头山经历了洋壳俯冲作用及底侵作用.      

扬子西缘荥经地区三叠纪碎屑物源分析

扬子西缘早三叠世处于伸展环境,而晚三叠世为前陆盆地.扬子西缘三叠系保存较好,是研究三叠纪构造转换物源响应方面的理想场所.本文根据重矿物电子探针和碎屑锆石测年,分析三叠系的物质来源,进而探讨与构造环境的对应关系.电气石探针结果显示,下三叠统主要源自贫锂花岗岩类伴生伟晶岩和细晶岩、变质板岩、变质砂岩、钙质硅酸盐岩和电气石石...     

STUDY ON THE PHYSICAL PROCESS OF WINTER VALLEY FOG IN XISHUANGBANNA REGION

Xishuangbanna of Yunnan Province is a famous tropical foggy region. A field experiment wascarried out from November 23 to 30 of 1997 during which fogs occurred regularly every day. In thepaper the characteristics of macrostructure of fog are analyzed and the physical processes offormation and dissipation of fog are studied. The results show that the Xishuangbanna valley fogforms firstly in the lower atmosphere with two-layer structures and then develops suddenly in thevertical direction after reaching the ground. Furthermore, the vegetation effect on the formationand dissipation of fog is discussed specially.     

鲁西铜石金矿田找矿成果及成矿机制探讨

铜石金矿田为山东省鲁西地区重要的金矿集区,1989-1994年勘查评价的归来庄金矿床,被原地质矿产部定义为"新地区、新类型、新发现",更是改写了鲁西地区无大型金矿床的格局.近年来,铜石金矿田金矿找矿取得了可喜的成果,累计发现大型金矿床1处、中型金矿床1处、小型金矿床3处、金矿点10余处,已查明上表的金金属量近50吨,目...     

遥感影像在六库城市地质灾害调查中的应用

根据地质灾害的特点,以六库城区排路坝滑坡和芭蕉河泥石流两地为遥感影像判译地质灾害实例,提出了六库城市地质灾害遥感影像特征判译标志     

云南南华地区大龙潭金矿之发现及其矿床地质特征

简要报道了在云南省南华县发现的大龙潭金矿床的地质特征。大龙潭金矿主矿体长360m,斜深大于60m。矿体形态呈似层状,局部呈透镜状,形态变化中等。矿体厚度的变化系数为71.2%～149.6%,较稳定;Au品位变化系数为87.5%～218%,较均匀;矿体产于向斜两翼,被断层错动,构造影响程度中等。据以上矿床地质特征将该矿区确定为Ⅱ勘查类型。     

云南东川播卡-拖布卡地区含金石英脉的^40Ar／^39Ar年龄及其地质意义

东川播卡-拖布卡地区金矿是云南中部"康滇地轴"中、新元古界昆阳群岩石中发现的第一个金矿,位于接近三江褶皱带的扬子地块西缘.原生金矿化为含金黄铁矿石英脉、细脉、网脉和浸染状石英黄铁矿.四个不同产状的典型含金石英脉的石英的阶段加热40Ar/39Ar年龄谱为马鞍形,坪年龄值范围为59.93±0.21～42.38±0.32 Ma,最小视年龄范围59.30±4.30～41.90±1.8 Ma,与计算坪年龄加热阶段相应数据的40Ar-39Ar等时线年龄范围59.34±0.17～41.25±0.10 Ma,三者基本一致.等时线年龄计算的相关系数大于0.998,40Ar/3 6Ar初始值范围为293.17±1.40～295.2±0.43,与尼尔值一致.石英形成后没有受到后期地质作用.石英样品的坪年龄没有受到过剩氩和氩丢失的影响,可以作为石英和金矿的年龄.金矿形成于新生代第三纪古新世和始新世初的陆内拉张地质构造环境中.     

Origin of power-law X-ray emission in the steep power-law state of X-ray binaries

We present a new explanation for the origin of the steep power-law(SPL) state of X-ray binaries.The power-law component of X-ray emission is the synchrotron radiation of relativistic electrons in highly magnetized compact spots orbiting near the inner stable circular orbit of a black hole.It has a hard spectrum that extends to above MeV energies,which is determined by the electron acceleration rate.These photons are then down-scattered by the surrounding plasma to form an observed steep spectrum.We discuss ...     

External photon fields in Fermi bright blazars

The external Compton(EC) model is used to study the high energy emission of some blazars,in which the external photon field is considered to dominate inverse Compton radiation. We explore the properties of the external photon field through analyzing the FERMI LAT bright AGN sample within three months of the start of operations in sky-survey mode. In the sample,assuming the high energy radiation of low synchrotron peaked blazars is from the EC process,we find that the external photon parameter Uext/νext may ...     

Stellar kinematics and populations out to 1.5 effective radii in the elliptical galaxy NGC 4636

We present high quality long slit spectra along the major and minor axes out to 1.5 effective radii of the massive galaxy NGC 4636 taken by the Hobby-Eberly Telescope. Using the Fourier Correlation Quotient method,we measured the stellar line-of-sight velocity distribution along the axes. Furthermore,six Lick/IDS indices(Hβ,Mgb,Fe5015,Fe5270,Fe5335,Fe5406) are derived from the clean spectrum. By comparing the measured absorption line strengths with the predictions of Simple Stellar Population(SSP) models,we...