辽宁晚侏罗世里阿斯箭蜓科－新属（昆虫纲，蜻蜓目）

本文描述了我国辽宁省北票市上侏罗统义县组中的里阿斯箭蜒科（Ｌｉａｓｓｏｇｏｍｐｈｉｄａｅ）一新属（Ｃｈｒｙｊｏｇｏｍｐｈｕｓｇｅｎ．ｎｏｖ．）。这是里阿斯箭蜒科昆虫化石在我国的首次发现,对研究这个类群的起源、演化和地理分布都具有重要意义．     

贵州省的亚洲象(Elephas maximus L.)和其它脊椎动物化石

本文报导的亚洲象化石,发现于贵州铜仁,代表这一物种在该省地层中的首例记录。在我国,贵州是以脊椎动物化石丰富和重要而称著的省份之一,但文献不集中,参考不便利。为此,作者集中了该省全部属类及其地质地理分布的主要资料,并讨论了相关问题,以冀为该省的进一步发现或研究提供一个初步的基础。     

甘肃老虎山闪长岩的地球化学特征及其成因

位于北祁连造山带东端的老虎山闪长岩侵位在晚奥陶统阴沟群砂板岩中,闪长岩的单颗粒锆石Ｕ－Ｐｂ年龄为４２３．５±２．８Ｍａ,是中志留世侵位的。老虎山闪长岩属于钙碱性岩系,富集ＬＲＥＥ和大离子亲石元素（ＬＩＬＥ）,Ｃｅ／Ｙｂ比值大于１３,Ｔｈ／Ｔａ比值大（１３～４２）,在微量元素分布图中呈现明显的Ｎｂ负异常,具岛弧或活动陆缘环境的特征。虽然老虎山闪长岩具有岛弧地球化学特征,但并不能认为它就产于岛弧环境,因为,在奥陶纪末期,早古生代的北祁连洋盆已经发生闭合,华北板块与柴达木板块已发生碰撞。因此,老虎山闪长岩是造山后侵位的,其成因可能与岩石圈拆沉作用有关。     

河北尚义侏罗系后城组节理研究

研究区侏罗系后城组地层发育着多组节理,根据其方位及相互关系,自早到晚分为５个节理组,其定向分别为１７４°、７７°、５８°、１４５°和１１９°,反映出节理形成的最大主压应力方向交替变化和偏转。岩石应变强度具有由弱至强,再由强至弱的演化趋势,而节理型式趋向不规则。区内节理多属构造成因,推测形成于侏罗纪末至白垩纪初近南北向的区域挤压过程。热液活动在区内节理形成之后,而后１１９°方位节理组发生右行走滑。     

青藏高原大地形对华南持续性暴雨影响的数值试验

利用新一代中尺度数值预报模式WRF3.2及NCEP/NCAR 逐日4次1°×1°的FNL再分析资料,通过有、无青藏高原以及将高原高度降低到临界高度的数值试验,研究了青藏高原大地形对我国华南地区2010 年5 月一次持续性暴雨过程的影响。试验结果表明:高原大地形对降水的影响显著,随着高原高度的升高,降水增多,高原以东地区的雨带也由北向南移动;高原地形的机械阻挡作用使迎风坡一侧的近地面层附近为强上升运动,背风坡为下沉运动,并分别对应降水的峰值和谷值区;高原对西风气流的爬流、绕流作用明显,高原升高后爬坡作用减弱,以绕流作用为主;高原的加热作用使气流过高原时南支减弱,北支加强,并加强了高原及其东部地区低层的正涡度和高层的负涡度,使高原上空为强烈的上升运动;高原的热力作用使西太平洋副热带高压位置偏南、偏西并稳定维持;高原大地形对形成稳定的高原季风环流圈有重要作用;高原地形高度的作用有利于定常波的形成,波动中心对应强上升运动,形成降水的大值区,稳定维持的定常波使得降水持续集中在同一地区,造成持续性暴雨。     

The Okavango giant mafic dyke swarm (NE Botswana): its structural significance within the Karoo Large Igneous Province

The structural organization of a giant mafic dyke swarm, the Okavango complex, in the northern Karoo Large Igneous Province (LIP) of NE Botswana is detailed. This N110°E-oriented dyke swarm extends for 1500 km with a maximum width of 100 km through Archaean basement terranes and Permo-Jurassic sedimentary sequences. The cornerstone of the study is the quantitative analysis of N>170 (exposed) and N>420 (detected by ground magnetics) dykes evidenced on a ca. 80-km-long section lying in crystalline host-rocks, at high-angle to the densest zone of the swarm (Shashe area). Individual dykes are generally sub-vertical and parallel to the entire swarm. Statistical analysis of width data indicates anomalous dyke frequency (few data <5.0 m) and mean dyke thickness (high value of 17 m) with respect to values classically obtained from other giant swarms. Variations of mean dyke thicknesses from 17 (N110°E swarm) to 27 m (adjoining and coeval N70°E giant swarm) are assigned to the conditions hosting fracture networks dilated as either shear or pure extensional structures, respectively, in response to an inferred NNW–SSE extension. Both fracture patterns are regarded as inherited brittle basement fabrics associated with a previous (Proterozoic) dyking event. The Okavango N110°E dyke swarm is thus a polyphase intrusive system in which total dilation caused by Karoo dykes (estimated frequency of 87%) is 12.2% (6315 m of cumulative dyke width) throughout the 52-km-long projected Shashe section. Assuming that Karoo mafic dyke swarms in NE Botswana follow inherited Proterozoic fractures, as similarly applied for most of the nearly synchronous giant dyke complexes converging towards the Nuanetsi area, leads us to consider that the resulting triple junction-like dyke/fracture pattern is not a definitive proof for a deep mantle plume in the Karoo LIP.     

A review of the occurrence, form and origin of C-bearing species in the Khibiny Alkaline Igneous Complex, Kola Peninsula, NW Russia

The Khibiny Complex hosts a wide variety of carbon-bearing species that include both oxidized and reduced varieties. Oxidised varieties include carbonate minerals, especially in the carbonatite complex at the eastern end of the pluton, and Na-carbonate phases. Reduced varieties include abiogenic hydrocarbon gases, particularly methane and ethane, dispersed bitumens, solid organic substances and graphite. The majority of the carbon in the Khibiny Complex is hosted in either the carbonatite complex or within the so-called “Central Arch”. The Central Arch is a ring-shaped structure which separates khibinites (coarse-grained eudialite-bearing nepheline-syenites) in the outer part of the complex from lyavochorrites (medium-grained nepheline-syenites) and foyaites in the inner part. The Central Arch is petrologically diverse and hosts the major REE-enriched apatite–nepheline deposits for which the complex is best known. It also hosts zones with elevated hydrocarbon (dominantly methane) gas content and zones of hydrothermally deposited Na-carbonate mineralisation. The hydrocarbon gases are most likely the product of a series of post-magmatic abiogenic reactions. It is likely that the concentration of apatite-nepheline deposits, hydrocarbon gases and Na-carbonate mineralisation, is a function of long lived fluid percolation through the Central Arch. Fluid migration was facilitated by stress release during cooling and uplift of the Khibiny Complex. As a result, carbon with a mantle signature was concentrated into a narrow ring-shaped zone.     

福建宁化丹霞地貌及特征

福建宁化白垩纪红层盆地位于华夏古陆武夷隆起西南部,地处中亚热带湿润区,自上新世以来,盆地内上白垩统崇安组紫红色巨厚层复成分砾岩、砂砾岩经漫长地质时期流水侵蚀、风化剥蚀、重力崩塌等外力作用缓慢雕塑,发育丹霞崖壁、石堡、石峰、石柱、石墙等正地貌,局部发育线谷、巷谷、峡谷等负地貌,构成一幅老年期丹霞地貌景观,是开展老年期丹霞地貌科研、科考的理想场所.     

湘东北中生代基性岩脉岩石地球化学及构造意义

湘东北中生代发育以辉绿岩类和煌斑岩类为代表的基性岩脉,属陆内拉斑玄武岩系,部分煌斑岩属于碱性系列。岩石富集LREE,δEu负异常不明显,其形成主要受软流圈地幔部分熔融作用制约。煌斑岩类微量元素总体上具有洋岛玄武岩(OIB)岩浆源区特征,富集Nd、P、Cs而K、Rb、Sr、U、Th等富集程度不明显,Ta、Nb略有富集。辉绿岩类表现出Ta、Nb、Ti亏损,但LILE并不富集,反映地壳混染程度的增强。基性岩脉形成于陆内拉张带的构造环境,岩浆活动未受到中生代大洋板块俯冲的影响。基性岩脉在时、空及物质组成上与湘东南玄武质岩石基本一致,属于整个湘东南岩石圈拉张-减薄带的一部分。     

海南岛抱板群岩石高温高压实验及金成矿机理探讨

高温高压实验岩石学是地质学、岩石学领域中的“硬科学”犤1999,王德滋,等犦。目前高温高压实验岩石学研究主要是针对单一岩石的熔化和融离实验,而针对多物源成因的花岗岩模拟其物源贡献大小的实验岩石学及同时发生的成矿作用研究基本上是一个空白。文章根据海南岛戈枕含金剪切带中元古代花岗岩的物源特征及与之有关的戈枕式金矿成因特点,通过高温高压实验岩石学模拟,初步探讨古中元古代抱板群岩石高温高压下的熔融行为及金的成矿机理。实验结果表明,具原地-半原地性质的中元古代花岗岩很可能是由6份(或4份)石英绢云母片岩+1份斜长角闪片麻岩、在压力为1.879～2.143GPa、温度849～901℃的条件下部分熔融形成的,部分熔融过程同时还发生了金的聚集和活化迁移。