沉积盆地、结晶基底和油、气成因理念与第二深度空间勘探和开发

在石油、天然气的勘探和开发研究中,涉及到深部空间的介质、结构和属性,在沉积建造上涉及到陆相沉积、海相沉积和火山岩相,在油、气成因理论上涉及到有机成因和无机成因,在机制上涉及到深部流体的分异、调整、运移和动力作用.这些本质性问题的研究和探讨是人们十分关注的科学领域.基于油、气生、储和形成的理论、应用和成效的研究提出,有几个基础性的理念问题必须重新认识,特别是沉积建造与古老变质岩结晶基底;双相（海相和陆相）沉积建造与盆地的内涵和双基（有机和无机）混合油、气成因理念.清晰地厘定这些认识不仅有益于对油、气形成、聚集和勘探及开发给出一个更为科学的深部空间,即第二深度空间（5000~10000 m）的油、气勘探,而更为重要的是基于对这些理念的重新认识和深化研究可构建新的思路或理论,且在新的理念导向下,强化油、气深部勘探,以期能在理论研究和实践应用中取得新的成效,发现大型与超大型油、气田.     

扬子板块东北缘中元古代的大地构造划分

扬子板块东北缘存在四条主要的中元古代变质带,自南向北依次为江南变质带、沿江变质带、云台一张八岭变质带和连云港一泗阳变质带。它们分别为中元古代的古弧后盆地、火山岛弧、裂谷及弧前盆地,扬子板块东北缘中元古代为活动大陆边缘构造体系。苏（北）胶（南）变质造山带应解体,其中一部分属扬子大陆边缘体系。     

Ductile deformation and development of andalusite microstructures in the Hongusan area: Constraints on the metamorphism and tectonics of the Ryoke Belt

Abstract   The main mesoscopic features of the ductile deformation in the Hongusan region of the Ryoke Belt can be explained in terms of a single deformation phase, Dm . The associated stretching lineation is roughly east–west and has an associated top-to-the-west sense of shear. This information fills an important gap in our knowledge about the deformational history of the Ryoke metamorphic belt. Andalusite porphyroblasts are well-developed in the Hongusan area and their microstructure can be used to link the deformational history with the metamorphism. However, the andalusite porphyroblasts show both intertectonic and post-tectonic microstructures. Some porphyroblasts have an intertectonic core and post-tectonic rim. Analysis of associated metamorphic minerals and bulk-rock chemistry suggests that the distinct types of microstructure can be explained in terms of distinct formation reactions related to regional and contact metamorphism. The intertectonic microstructure shows the presence of a deformation pre-dating Dm , referred to as Dc . These two deformation stages are sufficient to account for all the main deformation features. The distribution of post-tectonic andalusite growth shows a very broad thermal effect around an intrusion in the area. This can help place constraints on the thermal history of the Ryoke metamorphic belt.     

Gamma-ray emission from individual classical novae

Classical novae are important producers of radioactive nuclei, such as ⁷Be, ¹³N, ¹⁸F, ²²Na and ²⁶Al. The disintegration of these nuclei produces positrons (except for ⁷Be) that through annihilation with electrons produce photons of energies 511 keV and below. Furthermore, ⁷Be and ²²Na decay producing photons with energies of 478 and 1275 keV, respectively, well in the γ-ray domain. Therefore, novae are potential sources of γ-ray emission. We have developed two codes in order to analyse carefully the γ-ray emission of individual classical novae: a hydrodynamical one, which follows both the accretion and the explosion stages, and a Monte Carlo one, able to treat both production and transfer of γ-ray photons. Both codes have been coupled in order to simulate realistic explosions. The properties of γ-ray spectra and γ-ray light curves (for the continuum and for the lines at 511, 478 and 1275 keV) have been analysed, with a special emphasis on the difference between carbon–oxygen and oxygen–neon novae. Predictions of detectability of individual novae by the future SPI spectrometer on board the INTEGRAL satellite are made. Concerning ²⁶Al, its decay produces photons of 1809 keV but this occurs on a time-scale much longer than the typical time interval between nova outbursts in the Galaxy, making it undetectable in individual novae. The accumulated emission of ²⁶Al from many Galactic novae has not been modelled in this paper.     

Comments on “Two-dimensional concentration distribution for mixing-controlled bioreactive transport in steady-state” by O.A. Cirpka and A.J. Valocchi

In this comment we present a re-analysis of the analytical solution presented by Cirpka and Valocchi for steady-state concentrations of dissolved bioreactive compounds and bacterial biomass in porous media. We discuss the validity range of the analytical solution. In particular, the criterion used to determine the sustainability of biomass is revisited. This re-analysis shows that the ω$\omega$ criterion used by Cirpka and Valocchi is only a necessary but not a sufficient criterion to determine the bioreactive zones. As a consequence, the analytical solution does not provide the exact distribution of compounds throughout the domain, but can serve as upper or lower boundaries for species concentrations at a given location. These conclusions are supported by the simulation results obtained from an established reactive transport model.     

西大别浒湾高压变质带变沉积岩锆石U-Pb年龄及地质意义

西大别山浒湾高压变质带是研究秦岭-大别山-苏鲁造山带演化的关键区域, 但是该地区榴辉岩相变质时间还存在较大争议.本文通过对浒湾变质带熊店附近的一个变沉积岩样品进行LA-ICPMS锆石U-Pb定年和微量元素分析, 来确定该地区榴辉岩相变质作用和碎屑锆石的年龄, 并确定该变质带的演化历史.该样品的变质锆石具有弱分带或无分带、低Th/U比值、重稀土含量低且相对平坦以及无明显的Eu负异常等特征.反映这些变质锆石形成时有石榴石, 而缺乏长石, 其形成对应于榴辉岩相变质作用条件.该样品中变质锆石的206Pb/238U加权平均值为310±3Ma, 这一年龄代表了该地区榴辉岩相峰期变质作用的时间, 因此浒湾地区榴辉岩相变质作用时间为石炭纪.碎屑岩浆锆石得到了3组近谐和的U-Pb年龄, 其206Pb/238U年龄变化范围分别为: 400±5Ma~419±5Ma、426±5Ma~449±5Ma以及496±5Ma~524±7Ma, 还有1个颗粒给出了580±7Ma的较老年龄.这些结果表明变沉积岩中的碎屑锆石可能大部分来自于华北板块南缘, 少量来自于扬子板块.      

中国东部上地幔岩石相转变及其意义

中国东部新生代玄武岩和大别-苏鲁超高压变质带中的含石榴石相橄榄岩, 带来了发生在上地幔的尖晶石→石榴石相转变和铝辉石→贫铝辉石+石榴石的重要信息, 为中国东部上地幔岩石结构分层奠定了重要基础.通过岩石学与实验岩石学的研究, 推导出发生相转变的P-T条件, 为建立中国东部大陆上地幔岩石分层结构提供了重要约束.尖晶石二辉橄榄岩向石榴石二辉橄榄岩相转变发生在55~70km, 随着深度增加, 石榴石二辉橄榄岩从富铝石榴石二辉橄榄岩(70~120km) 转变为贫铝石榴石二辉橄榄岩(> 120~150km).      

用陆块旋转解释藏东南渐新世-中新世伸展作用——来自点苍山及邻区变质核杂岩的证据

沿红河断裂带(RRFZ)分布的点苍山变质核杂岩是一个不完整的变质核杂岩,它由两个特征迥异的单元组成,包括被同构造二长花岗岩侵入角闪岩相构造岩组成的下盘和绿片岩相的拆离断层带。下盘岩石包括具有高温构造组合,具有指示左行走滑剪切运动方向的L型糜棱岩或LS型糜棱岩。拆离断层带是一个上盘向E到SE伸展剪切的低温剪切带,由具有剪应变和压应变的典型S-L糜棱岩构成。低温构造岩也包括发育于下盘的几个糜棱岩化似斑状二长花岗岩侵入体。变质核杂岩与西侧覆盖未变质的中生代沉积岩并置,东部受第四纪断层作用影响为沿洱海分布的更新世-全新世沉积盆地。通过对点苍山变质核杂岩的构造研究,结合邻区变质核杂岩的地质年代学及古地磁学分析,我们认为:位于东南亚红河断裂和实皆断裂带之间的扇形区域内出现的变质核杂岩与渐新世-中新世时期区域性伸展作用有关,而伸展作用是由印支地块的差异性旋转产生的,其原因是由于约33Ma开始斜向俯冲的印度板块的顺时针旋转和回退所致。     

大别山超高压变质岩的退变质赤微构造：折返过程的启示

大别山超高压变质岩中发现了一系列退变质显微构造,其主要类型有：①由于出溶而产生的定一包裹物;②由于多型转变而产生的假像替代;③固→固反应产生的冠状体;④涉及流体的退变质反应产生的冠状体或后成合晶。借助显微构造关系,可以建立超高压变质岩的退变质演化阶段,从而构筑其ＰＴ演化趋势、识别出碰撞造山和超高压变质峰期之后的两阶段隆升历史;早期为“挤出”作用诱发的近等温减压退变质;晚期则是地壳伸展体制下的退变质     

冀东太平寨-娄子山太古宙麻粒岩相变质峰期流体研究

冀东太平寨-娄子山地区太古宙麻粒岩系变质峰期流体包裹体首次见于夕线石中,按形 态 和产状可分三类,均形成于峰期至其稍后阶段。它们成分相似。特征是:①富碳质,XC　O2+C　H4=0.64～0.93; ②含少量H2O,XH 2O=0～0.22,且与峰期矿物 组合平衡热力学计算的水活度(aH2O=0.04～0.31)和含量( XH2O=0.03～0.22)完全吻合; ③有时含一定量H2S和SO2; ④盐水溶液 中阴离子总量极低(0.12～0.61mol/L)。石英和石榴石中也有特征相同的这期包裹体。峰 期包裹体中C　O 2均一温度多数 为-28℃～-22℃,密度为0.96～1.06g/cm3,包裹体整体密度应稍高,相应的压力为0.60 ～0.70G Pa。流体的氧逸度lgfO2在-17～-15之间。峰期流体上述各种特征在空间上较 均匀,相邻的不同岩石类型中aH2O值相似,结合地质和原岩特 征分析,认为流体中C　O2可能为深部地幔来源,其成因与基性岩浆底侵及其结晶作 用有关。