塔里木盆地天然气运聚系统与运聚模式

对塔里木盆地东部地层压力结构和天然气性质差异的研究表明,塔里木盆地东部具有多个独立的天然气运聚系统。这些运聚系统具有流体封存箱的特征。天然气只能在运聚系统内部进行短距离的运移,不能进行大规模侧向运移。因此天然气藏的形成具有近源的特点。由于不同运聚系统特征的差异,塔里木盆地大致有三种天然气运聚模式。     

百色盆地低熟油的地球化学特征及成因机制

对百色盆地几个典型低熟油进行了常规的有机地球化学分析,并重点以百－５井低熟油为对象,详细总结了饱和烃,芳烃生物标志物地球化学特征及其组合,结果表明陆生高等植物和微生物大量繁衍及其对高等植物的改造的贡献可能是形成百色盆地第三系低熟油的主要原因。     

寿昌—临浦火山岩带赋矿流纹岩特征及归属雏议

本文介绍的火山岩带,有层状流纹岩及穹丘状、岩颈状等非层状流纹岩,分别属溢流相、侵出相及火山管道相,三种流纹岩均受火山岩带核中断裂及晚期火山构造控制,复盖或穿发寿昌组一段地层,又被寿昌组一段之后的次火山岩及隐爆岩所穿切,局部被横山组不整合复盖。该类流纺岩同位素年龄值较小,多数在１３０Ｍａ左右,处于晚侏罗世与早白垩世过渡期。根据其层序、穿切关系及同位素年龄等,认为三种流纹岩均属火山岩带晚期不同岩相的产     

后压浆方案的技术可行性论证

从地层选择、效果预测、经济分析和施工应用４个方面对钻孔灌注桩后压浆方案进行可行性论证,并对承载力增幅进行了分析。     

有机酸对高岭石形成影响的模拟试验研究

利用富里酸、胡敏酸和盐酸与天然矿物－长石、蒙脱石和云母在常温常压下进行反应,探讨矿物溶解及高岭石形成机理。实验表明富里酸对这些矿物具有较大的溶解能力,其原因是由于形成了具有较大溶解度和活动性的有机硅和有机铝复合体。在中性－碱性条件下有利于有机硅复合体的形成,酸性条件下有利于有机铝复合体的形成。在富里酸作用下,蒙脱石和云母分别在４个月和８个月有少量转化成高岭石,说明层状硅酸盐矿物比架状硅酸盐矿物更易     

冀东地区长城系高于庄组岩相古地理及黄铁矿生物成因探讨

冀东地区中元古界长城系高于庄组可划分为７个自然岩性段,硫等赋矿层位为其２～５段,由含锰页岩 含锰白云岩 含锰页岩 含锰白云岩组成二个正旋回。高于庄组沉积早期（即下旋回第２段）,在遵化 北汤道河水下高地的阻隔下,形成了蓟县 迁西泻湖,属封闭的还原环境,控制了“蓟县式”锰方硼石矿床。高于庄组沉积晚期（即上旋回第４段和第５段）沉积时期,高板河泻湖形成,由于泻湖南侧受北东东向同生断裂控制,北侧又受生物礁制约,在生物作用及滞流的还原环境下,形成了“高板河式”黄铁（铅锌）矿床。上旋回生物礁相和泻湖相区是寻找黄铁（铅锌）矿的靶区。     

西藏江孜地区上白垩统宗卓组沉积混杂堆积基本特征及构造意义

分布于藏南江孜一带的上白垩统宗卓组沉积混杂堆积岩呈近东西向与雅鲁藏布江缝合带平行相伴,由“基质”、原地岩块、外来岩块三部分组成。“基质”以正常沉积的细碎屑岩为主;原地岩块是沉积物未完全固结时,由于重力或其它地质作用使之变形变位后形成的;外来岩块成分复杂、形态各异、大小悬殊,不同岩块中产晚三叠世—早白垩世的箭石、双壳类等化石。岩块间很少直接接触,地貌上明显突起,其变形变质程度与“基质”极不协调,它是早白垩世以来,喜马拉雅板片向冈底斯－念青唐古拉板片俯冲,于被动陆缘形成近东西向的狭长海槽,而仰冲板片受到强烈的破碎,大小不等的岩块滑落于海槽中构成的沉积混杂堆积岩。     

Radiative acceleration of coronal gas in Seyfert nuclei

The line ratios from coronal gas in Seyferts can be successfully fitted with photoionized clouds of high densities and low volume filling factor. The ionization parameter implied is sufficiently high that models must consider the effect of radiation pressure from the active nucleus. In spite of the gravitational force of the nucleus, radiation pressure is sufficiently strong to compress and radially accelerate the internally stratified gas clouds provided that these contain small amounts of dust (≃ 10 per cent of the solar neighbourhood value). This radial acceleration could explain the blueshift of the coronal lines relative to the systemic velocity without the need to invoke an ambient 'pushing' wind. Embedded dust has the interesting effect of making the photoionized clouds marginally ionization-bounded instead of matter-bounded.     

Gamma-ray bursts from stellar remnants: probing the Universe at high redshift

A gamma-ray burst (GRB) releases an amount of energy similar to that of a supernova explosion, which combined with its rapid variability suggests an origin related to neutron stars or black holes. Since these compact stellar remnants form from the most massive stars not long after their birth, GRBs should trace the star formation rate in the Universe; we show that the GRB flux distribution is consistent with this. Because of the strong evolution of the star formation rate with redshift, it follows that the dimmest known bursts have z  ∼ 6, much above the value usually quoted and beyond the most distant quasars. This explains the absence of bright galaxies in well-studied GRB error boxes. The increased distances imply a peak luminosity of 8.3 × 10⁵¹ erg s⁻¹ and a rate density of 0.025 per million years per galaxy. These values are 20 times higher and 150 times lower, respectively, than are implied by fits with non-evolving GRB rates. This means either that GRBs are caused by a much rarer phenomenon than mergers of binary neutron stars, or that their gamma-ray emission is often invisible to us due to beaming. Precise burst locations from optical transients will discriminate between the various models for GRBs from stellar deaths, because the distance between progenitor birth place and burst varies greatly among them. The dimmest GRBs are then the most distant known objects, and may probe the Universe at an age when the first stars were forming.     

Lattice dynamical system modelling of molecular clouds

Because a comprehensive microscopic treatment of interstellar molecular clouds is out of reach, an alternative approach is proposed in which most of the crucial ingredients of the problem are considered, but at some 'minimal' level of modelling. This leads to the elaboration of a lattice dynamical system , i.e. a time-dependent, spatially extended, deterministic system of macroscopic cells coupled through radiative transfer. Each cell is characterized by a small set of variables and supports a caricatural chemistry possessing the essential dynamical features of more realistic reaction schemes.   This approach naturally precludes quantitative results, but allows heretofore unavailable insights into some of the basic mechanisms at play. We focus on the response of the transfer process and the chemistry to a frozen 'turbulent' velocity field. It is shown that the system settles generically into a state where the effective coupling between cells is neither local nor global, and for which no single length-scale exists.   The spectral lines reconstructed from the spatiotemporal evolution of our model may, depending on the velocity field, exhibit profiles ranging from Gaussian to bimodal with strong realization effects. In the bimodal case, the model intrinsically displays an energy cascade transport mechanism to the cells that cool most efficiently: the feedback of chemistry on radiative transfer cannot be neglected.   Finally, extensions of this work are discussed and future developments are outlined.