千山 东北大地上的一颗明珠

辽宁千山系长白山支脉,辽河与鸭绿江的分水岭,是辽东半岛的脊骨。据地质考察,大约4亿年前,千山一带是一片海洋,到古生代末期开始隆起露出水面形成陆地。经历海陆沧桑5次变迁,1．8亿年前,形成现在典型的粗粒花岗岩地貌……     

辽宁省工程技术学校

辽宁省工程技术学校隶属于辽宁省地质矿产勘查局,是一所为地质行业、矿业行业、珠宝行业及其他相关行业培养技能型人才的全日制中等专业技术学校。校园环境幽雅、交通便利     

《地球科学与环境学报》编委简介

陈骏教授男,汉族,1954年10月出生,江苏省扬州市人。1979年毕业于南京大学地质系,1982年获南京大学地球化学专业硕士学位,1985年获南京大学矿床学专业博士学位。1986年起在南京大学任教。1988-1989年在英国帝国理工学院从事博士后研究工作。1992年晋升为南京大学教     

Variable Star Status of Two Stars： V204 and I-I-39 in M3

The star 1-1-42 （=vZ1390）, a cluster member in M3, located near the red edge of the instability strip of the horizontal branch, was discovered by Roberts and Sandage as a low amplitude variable, it was designated as V204 in the ＂second catalogue of variable stars in globular clusters＂, but its coordinates given in all versions of this catalogue are wrong since 1955. We argue that V204 is indeed a low amplitude HB variable star, located near to the red edge of the instability strip, with a period of 0.74785d and an amplitude of about 0.04 mag in V. We also find that the red cluster member star 1-1-39 is a low amplitude variable with a period of 1.16^d and amplitude of about 0.03 mag in V which might be pulsating at the second overtone.     

An Alternative Explanation for a Screw-like Meteoric Train Photographed by Double-Station Observations

Two-station observation of meteors, especially a meteor trains, provides an effective approach to the measurement of the physical parameters. We have collected four special groups of photographs of meteoric trains taken at two stations during Leonids 2001. One representative group has been measured and analyzed in detail. An analysis has been reported in our first paper. In this paper, an alternative explanation for the screw-like meteoric train is suggested based on some physical calculations. The results reveal that this train has a screw-like structure and, apparently, spoke beams. The mother meteor of this train may be negatively charged and moves forward along a left-hand screw trajectory under the effect of the geomagnetic field. The spoke beams might be the visual effect of the long time exposure of many particles released from the disintegrated meteoroid.     

宇宙信息

中日科学家发现新褐矮星,我国第24次南极考察全面展开,LAMOST天体测量支持系统完成测试,SETl@home期待你参与,彗星物质形成于太阳系的不同区域地外行星形成盘中发现有机分子,天文学家成功预言地外行星,     

大地构造和海陆起源的内波假说（Ⅱ）──建立假说的大地构造学与运动学基础

介绍建立大地构造内波假说的根据，即：（１）全球海陆分布的低阶球谐特征；（２）全球大洋中脊体系的存在；（３）大陆永存及生长的事实；（４）地壳均衡及莫霍面的化学分界面性质；（５）地槽活动的现象、规律等。在分析以在事实的基础上，研究了大地构造运动中主要的物质运动过程，认为从薄地壳底部向厚地壳底部迁移的地壳物质流，引起地壳厚度的自激波动，推动地槽运动和大陆生长。     

首届全国大中学生海洋知识竞赛优胜选手赴西涉考察

5月19日上午,首届全国大中学生海洋知识竞赛的优胜选手结束了在西沙的考察活动,乘中国海监83船抵达广州长洲码头。本次考察活动的主题为“踏浪西沙,放飞梦想”,20名优胜选手来自中国海洋大学和山东省畜牧兽医学院,他们15日下午从广州出发,17日登上西沙永兴岛进行了为期1天的考察访问。     

湘赣边界鹿井铀矿床流体包裹体及成矿机制

位于南岭成矿带南西部的鹿井矿床是华南热液型铀矿的典型代表.为查明其成矿流体来源、性质与演化以及成矿机制,开展了不同成矿阶段石英、萤石及方解石中流体包裹体的显微测温和不同阶段石英的氢?氧同位素分析.矿床地质特征表明成矿过程可划分为(I)粗晶石英+黄铁矿±绿泥石±绢云母、(II)沥青铀矿+硫化物+绿泥石+绢云母+暗灰色微晶...