△T球体异常的三元解释法

在△Ｔ异常解释课题中，一个新的角度参量─—视磁化特征角的拟定，最大限度地简化了球体磁场表达式。从而才有可能通过特殊解法，给出了球体磁场的极值与拐点公式。作者据此建立了四种不受正常场制约、仅需异常的局部持征曲线即可全面解释三度异常的解释方法。屏障分解、叠加判别、三元迭代的设计，为解释三度体叠加异常给出了简单而易行的途径。     

Strong magnetic field in W75N OH maser flare

A flare of OH maser emission was discovered in W75N in 2000. Its location was determined with the Very Long Baseline Array (VLBA) to be within 110 au from one of the ultracompact H  ii regions, Very Large Array 2 (VLA2). The flare consisted of several maser spots. Four of the spots were found to form Zeeman pairs, all of them with a magnetic field strength of about 40 mG. This is the highest ever magnetic field strength found in OH masers, an order of magnitude higher than in typical OH masers. Three possible sources for the enhanced magnetic field are discussed: (i) the magnetic field of the exciting star dragged out by the stellar wind; (ii) the general interstellar field in the gas compressed by the magnetohydrodynamic shock; and (iii) the magnetic field of planets which orbit the exciting star and produce maser emission in gaseous envelopes.     

Spine–sheath polarization structures in four active galactic nuclei jets

We present the results of multifrequency (15 + 8 + 5 GHz) polarization Very Long Baseline Array (VLBA) observations of the three BL Lacertae objects 0745+241, 1418+546 and 1652+398 together with 5-GHz VLBI Space Observatory Programme (VSOP) observations of 1418+546 and 1.6- and 5-GHz VSOP observations of the blazar 1055+018. The jets of all these sources have polarization structure transverse to the jet axis, with the polarization E vectors aligned with the jet along the jet spine and 'sheaths' of orthogonal E vectors at one or both edges of the jet. The presence of polarization aligned with the jet near the 'spine' may indicate that the jets are associated with helical B fields that propogate outward with the jet flow; the presence of orthogonal polarization near the edges of the jet may likewise be a consequence of a helical jet B field, or may be owing to an interaction with the ambient medium on parsec scales. We have tentatively detected interknot polarization in 1055+018 with E aligned with the local jet direction, consistent with the possibility that the jet of this source is associated with a helical B field.     

《南岭成矿带成矿规律图》研编创新点及其找矿意义

由中国地质科学院矿产资源所编制出版的《南岭成矿带成矿规律图（1∶80万）》,是迄今为止矿种最全、资料最新、信息量最大的全面反映我国南岭勘查成果与成矿规律的区带级别（Ⅲ级成矿单元）成矿规律图。该图件研编实现了4大创新点：① 涵盖了南岭已发现的2903处独立矿产地,包括能源、金属、非金属和水气矿产等4大类的76个矿种,实现了南岭成矿带矿种与矿产地的全覆盖;② 归并了地质底图的地层并淡化显示,突出华南岩体、隐伏岩体的特色,使得不同构造—建造层地质单元的分布格局一目了然;③ 实现了矿产地、规模、类型、时代、成矿系列五位一体的综合图例设计,矿产地表达更简洁、直观;④ 综合成矿系列图、表、成矿体系图、剖面图等,以区域规律图编制的新思路和新方法,更集中反映和彰显南岭成矿带最新科研成果。该图件的研编有助于直观展示南岭成矿带矿产的时空分布格局,深入总结成矿规律,科学圈定重要找矿远景区,对于全面指导南岭的地质找矿工作具有重要的意义。     

石英脉型钨多金属矿床的扇状成矿实例及找矿模型

石英脉型钨矿床是中国数量最多的钨矿床类型,但保有储量消耗迅速,迫切需要创新找矿模型,指导找矿突破。文章结合二十余年的找矿实践,通过详细分析扇状成矿矿床实例,构建了石英脉型钨矿床新的找矿模型。该模型强调赋矿裂隙为岩浆动力成因,在花岗岩体顶部呈扇状分布型式,岩浆期后热液恰在裂隙张开时充填其中而形成扇状成矿系统;提出“就岩找矿”、“就矿找矿”、“就矿找岩”的地质、地球化学和地球物理标志,指导矿床尺度的勘查工程部署。截至目前,该模型已在广东禾尚田钨锡矿床、广西珊瑚钨锡矿床、广西社垌钨钼矿床、江西盘古山钨铋矿床等获得了验证,找矿成效显著。     

中国含盐盆地成钾矿集区划分与找钾前景概述——纪念中国找钾60年

对中国含盐盆地戍钾矿集区、成钾准矿集区及成钾预备矿集区进行划分。矿集区的特点为①有一个主要的钾盐矿床;②每个盆地都有数个,有的迭10个以上钾盐矿床,地质资源合计储量KCl都达亿t以上;③钾盐戍因机制、模式复杂多样。对中国找钾60年进行回顾,提出深部找钾及科学找钾：①练好业务,即熟悉掌握找钾各种最新物探、化探、岩矿测试分析技术。②熟悉掌握中外找钾理论和经验;③二次开发找盐钾文献、资料和标本;④深入剖析一个盐盆的野外地质工作和室内分析资料,整理研究,找出规律,提出找钾有利层位和地点。⑤多学科多技术结合,老中新组成团队,发挥协作精神;⑥选有最利成盐钾和油气共生盆地（钾矿集区）开展工作,如四川、陕西、新疆等地。并对中国找钾前景进行预测。     

中亚地区阿拉伊盆地构造地质特征与油气条件分析

阿拉伊盆地位于特提斯构造带北缘,是在古生界基底之上发展起来的山间盆地,紧邻我国西部塔里木盆地。自中生代至新生代经历了陆表海沉积期、类前陆盆地期、山间盆地发育期、拗陷期、定形期等5个演化阶段,具有海陆交互、沉积多变、多期叠加、断-拗转换的性质。生储盖匹配良好;烃源岩为古近系、白垩系和中—下侏罗统的海相与潟湖相泥岩、石灰岩和泥灰岩;主要油气储集层为碳酸盐岩裂缝性储层和砂砾岩储层;多套泥岩、膏岩和泥灰岩为区域性和局部盖层;褶皱构造发育,以背斜、断块、断鼻等构造为主。盆地具有一定的油气勘探前景。