贵州岑巩区块下寒武统变马冲组黑色页岩沉积地球化学特征及其沉积环境意义

基于钻井岩心资料,对贵州岑巩区块下寒武统变马冲组黑色页岩取心段进行系统采样、主微量元素测试及沉积地球化学分析。研究结果表明：1）古盐度判别指标Sr/Ba及Rb/K分布显示,下寒武统变马冲组黑色页岩沉积时期属局限海背景下的半（微）咸水—淡水相沉积,变马冲组一段—三段古盐度垂向变化不大;Sr丰度与碳酸盐矿物含量之间具明显的响应关系;2）古氧相指标V/Cr、Ni/Co、U/Th比值及δU值分布表明变马冲组黑色页岩沉积为氧化为主、间或贫氧的环境,V/（V+Ni）比值判别偏于还原环境;3）古气候判别参数“C”、Sr/Cu及SiO2/Al2O3比值表明该套页岩沉积期主体属温湿气候,利于有机质形成;4）古水深及离岸远近判别参数Rb/Zr、Sr/Ba比值分布显示水体较浅、离岸较近的沉积特征,结合物源及沉积构造背景指征参数分析,变马冲组黑色页岩属大陆边缘离岸较近、水体较浅的陆源碎屑沉积。此研究认识揭示了岑巩区块下寒武统沉积环境的演化,进而为该套黑色页岩的有机质富集机理及页岩气选区评价提供一定的地质依据。     

北黄海盆地东部坳陷勘探突破对我国近海残留“黑色侏罗系”油气勘探的启示

最新的勘探和研究证实,北黄海盆地东部坳陷发育了中、上侏罗统2套有效烃源岩并以上侏罗统为主力烃源岩层,在其供烃范围内形成了上侏罗统-下白垩统"下生上储式"和中-上侏罗统"自生自储式"2类成藏组合,取得了我国东部海域以侏罗系为唯一源岩的含油气盆地勘探突破。为进一步探索我国近海盆地残留"黑色侏罗系"的资源潜力和勘探前景,本文采用地震-地质综合解释、烃源岩地球化学分析、盆地模拟等方法,综合分析了我国近海主要盆地残留"黑色侏罗系"的分布和地球化学特征。结果表明,我国近海残留侏罗系暗色泥岩烃源岩非均质性较强,多属"中等"级别,局部发育"中等-好"、"中等-差"级别烃源岩,侏罗系烃源岩大多存在早（J₃-K₁）、晚（E₂末-N₁）2期生、排烃高峰,生烃总量达1.4×10¹¹ t,资源前景乐观,预测可形成侏罗系"自生自储式"和侏罗系-白垩系（或新生界）"下生上储式"2类源储组合。     

Changes and opportunities for integrated management of the Razim-Sinoe Lagoon System

The aim of this paper is to identify the general trend of changes and the basic requirements of the most important lagoon system of the Black Sea, on the basis of critical analysis of existing data. A more coherent set of data sampled after 1988 on the basis of some intensive and extensive study and research programmes, including the main trophic parameters and the most representative structural and functional features of this complex of ecotonal lakes, is comparatively analysed together with more fragmentary data previously existing. The structural and functional changes within this complex of lakes were analysed based on 31 most representative variables belonging to the main abiotic and biological compartments of the two main lakes, Razim and Sinoe: dissolved organic carbon, dissolved oxygen, trophic state index TSI, nutrient content and ratio, salinity, chlorophyll, phytoplankton, zooplankton, submerged macrophytes, zoobenthos, fish and birds. Two stages were distinguised in the main structural changes, including morphometric connections with the Danube River and the Black Sea and hydrochemistry and its effects on communities. These transitions were associated with two main driving forces, water desalinisation and rapid eutrophication, and with other two kinds of man-induced changes, local hydrotechnical buildings and long-distance variables operating over the entire Danube River watershed. The information support system for sustainable management of the Razim-Sinoe Lagoon Complex as a part of the Danube Delta Biosphere Reserve, integrating existing data from research programmes and an integrated monitoring system for new data is a final conclusion on further needs.     

大质量黑洞吸积盘的径向自引力

本文研究了大质量黑洞吸积盘的自引力,用薄盘位形上积分的方法计算了吸积盘自引力的径向与垂向分量,着重讨论了径向自引力。主要结果为:对于大质量黑洞(M～10~8—10~(10)M_⊙)吸积盘,在(R/R_g)～10~5—10~4的距离上,径向自引力会超过中心天体引力。在这个距离上,吸积盘的动力学结构完全不同于开普勒盘。提出了径向自引力不稳定扰动作为一种能源机制。本文还得到吸积盘自引力与中心天体引力量级比较的两个判据,并由此得到大质量黑洞吸积盘外半径的近似解析估计。本文结果可用于类星体和星系核吸积盘。     

一次特大沙尘暴成因的卫星云图分析

运用1小时间隔的GMS-4数字展宽红外资料和部分常规气象资料,分析了1993年5月5日下午至夜间发生在甘肃和宁夏等省(区)部分地区罕见的特大沙尘暴的形成原因。结果指出,这场特大沙尘暴主要由强冷锋前部的中尺度对流系统(MCS)及其伴随的飑线造成的。它们的移动大体与地面强冷锋及700～500hPa间的平均气流方向一致。最后对此MCS及其伴随的飑线的可预报性问题作了简要讨论。     

中国黑戈壁地区日照时数时空变化及影响因素

利用1960～2011年中国黑戈壁地区11个气象站日照时数数据,分析了该地区日照多年变化特征。研究表明,该地区近52a来日照时数减少的变化并不明显,其趋势变化率为-2．0h／10a,远小于周边地区。四季之中,春季日照时数呈增加趋势,其他三季呈减少趋势。从空间分布上看,不同区域,年日照时数变化也不相同。黑戈壁地区年日照时数的减少与年降水量的显著增加和年平均风速的减小密切相关。     

Normal modes of black hole accretion disks

This article studies the hydrodynamical problem of normal modes of small adiabatic oscillations of relativistic barotropic thin accretion disks around black holes (and compact weakly magnetic neutron stars). Employing Wentzel-Kramers-Brillouin (WKB) techniques, we obtain the eigenfrequencies and eigenfunctions of the modes for different values of the mass and angular momentum of the central black hole. We discuss the properties of the various types of modes and show for the first time that modes covering the whole extension of the disk (full-disk p-modes) can exist within the studied thin disk model. However, these modes have relatively short wavelengths.     

黑碳气溶胶研究进展Ⅰ：排放、清除和浓度

黑碳气溶胶是近几年非常活跃的一个研究课题，因为黑碳气溶胶吸收太阳和地球大气的辐射，对全球气候变暖有重要的影响。中国黑碳气溶胶的排放和浓度比同纬度的高，在全球气候变暖的大背景下，中国黑碳气溶胶一直受到国外的关注。综述了国内外黑碳气溶胶研究的最新进展，受篇幅的限制，文章分两篇，第一篇是黑碳气溶胶的排放、清除和浓度，第二篇是黑碳气溶胶的气候效应和拓展的研究领域。从黑碳排放的估算和大气浓度的测量方法进行描述，列出有关的测量结果，对黑碳气溶胶的排放和大气浓度进行国内外的初步比较分析。还对黑碳气溶胶排放和浓度测量误差进行了讨论，并对今后黑碳气溶胶研究提出了几点建议。     

中国地区黑碳气溶胶直接辐射效应的数值模拟研究

利用意大利国际理论物理研究中心（ICTP）提供的2000年各月气溶胶资料（包括人类活动和生物质燃烧所产生的气溶胶）,使用并行版本区域气候模式RegCM3,研究了黑碳气溶胶对中国区域气候的影响。结果表明,引入黑碳气溶胶后,冬、夏季中国大部分地区大气顶出现了正辐射强迫,其分布与垂直负荷分布基本相似。在仅考虑黑碳气溶胶的直接辐射效应时,中国大部分地区冬、夏季地面气温呈下降趋势,降温的高值区均位于中国东南部,冬季最大降温幅度约为0．9℃,夏季最大降幅约为2．4℃,夏季降温幅度明显大于冬季。相对于温度变化,黑碳气溶胶引起的降水变化较为复杂,无论是冬季还是夏季,降水量减小的区域均大于增加区。冬季降水量最大减幅约为20mm,夏季降水量最大减幅超过100mm,夏季降水量减幅明显大于冬季。冬、夏季仅西北和华南部分地区降水量有所增加。冬季中国大部分地区痕量降水和弱降水日数呈增加趋势;夏季黄河以北中国北方地区痕量降水和弱降水日数也是以增加为主。     

Numerical Simulation of Small Perturbation on an Accretion Disk Due to the Collision of a Star with the Disk Near the Black Hole

In this paper, perturbations of an accretion disk by a star orbiting around a black hole are studied. We report on a numerical experiment, which has been carried out by using a parallel-machine code originally developed by Dönmez (2004). An initially steady state accretion disk near a non-rotating (Schwarzschild) black hole interacts with a “star”, modeled as an initially circular region of increased density. Part of the disk is affected by the interaction. In some cases, a gap develops and shock wave propagates through the disk. We follow the evolution for order of one dynamical period and we show how the non-axisymetric density perturbation further evolves and moves downwards where the material of the disk and the star become eventually accreted onto the central body. When the star perturbs the steady state accretion disk, the disk around the black hole is destroyed by the effect of perturbation. The perturbed accretion disk creates a shock wave during the evolution and it loses angular momentum when the gas hits on the shock waves. Colliding gas with the shock wave is the one of the basic mechanism of emitting the X-rays in the accretion disk. The series of supernovae occurring in the inner disk could entirely destroy the disk in that region which leaves a more massive black hole behind, at the center of galaxies.