重力驱动作用——滦平盆地下白垩统西瓜园组沉积时期主要的搬运机制

通过对冀北滦平盆地下白垩统西瓜园组沉积地层的实地考察,发现盆地内发育丰富的重力驱动作用沉积物。文中描述西瓜园组发育的滑动和滑塌现象,指出露头剖面中存在的挤压变形现象并非构造成因,而是由于滑动块体和滑塌块体前端的挤压应力环境造成的。在介绍西瓜园组重力流沉积发育环境的基础上,对露头中存在的若干重力流沉积进行了描述,并使用砂质碎屑流这一概念对这些现象进行了较为合理的成因解释。通过对滑动和滑塌(重力块体运动)和砂质碎屑流—浊流(重力流)沉积物研究,结合前人对该地区冲积扇—扇三角洲的研究成果,认为重力驱动作用是滦平盆地下白垩统西瓜园组沉积时期主要的搬运机制。     

A new approach for evaluating climate change communication

Many scholars study when climate change communication increases citizen engagement. Yet, past work has largely used public opinion-based measures of engagement to evaluate alternative frames. In this paper, we argue for a new approach to evaluation, which is premised on research on the policy-making process showing that space on the political agenda and, ultimately, policy change are more likely to arise in response to changes in both public opinion and collective political action. Thus, we argue that alternative frames should be evaluated based on their consequences for both. This is especially critical given that frames can have divergent effects on attitudes and behavior. Using a combination of field and survey experiments, we apply our approach to evaluate two frames related to climate change risks. We find that they heighten people’s concern about climate change yet decrease their rate of political action to express that concern. Our results suggest caution with regard to these frames in particular and that, more generally, frames that might seem advantageous when examining public opinion may not be when political behavior is analyzed.

     

鄂尔多斯盆地华池地区三叠系延长组长7段富有机质页岩岩相特征

鄂尔多斯盆地三叠系延长组长7油层组发育富有机质页岩和泥岩,目前已成为鄂尔多斯盆地页岩油气勘探的重要层位。综合岩心精细描述、薄片微观结构观察和粒度分析结果,将富有机质页岩和泥岩划分为黑色页岩岩相、纹层状泥岩岩相、粉砂质泥岩岩相。粉砂质泥岩岩相的脆性矿物含量高于黑色页岩岩相和纹层状泥岩岩相,后者比前者具有更高的黄铁矿含量,3种岩相的黏土矿物含量较接近。黑色页岩岩相有机质丰度高,有机质类型以I型干酪根为主,是最有利的富有机质岩相类型,其次为纹层状泥岩岩相。长7油层组沉积时期水体为分层的厌氧环境,有利于有机质的保存,低等水生生物是主要的母质来源。黑色页岩岩相和纹层状泥岩岩相形成于安静、缺少陆源碎屑影响的深湖环境下;粉砂质泥岩岩相形成于受陆源碎屑频繁影响的环境,有较多的陆源高等物质输入湖盆中,造成有机质类型复杂。将岩心精细描述和测井信息紧密结合,揭示了各类岩相纵向发育特征。受基准面变化和沉积物供给能力影响,长73以黑色页岩岩相和纹层状泥岩岩相为主,长72和长71以纹层状泥岩岩相和粉砂质泥岩岩相为主。长73暗色泥岩和页岩的岩相类型好,发育页理缝和纹层缝,有机质类型好、丰度高,是最有利的页岩油气勘探目的层系。     

碎屑岩与火山岩混积岩系层序地层学研究初探——以准噶尔盆地西北缘佳木河组为例

准噶尔盆地西北缘前陆冲断带是剖析西准噶尔地区盆山耦合关系、沉积体系发育的关键地段。该区二叠系佳木河组为火山岩、火山碎屑岩、碎屑岩组成的混积地层。火山岩与碎屑岩组成的地层单元有广义上的成因联系,因为它们都属于史密斯地层,并均具有旋回特征。针对不同的岩性区:碎屑岩岩性区、火山岩与碎屑岩共存区、纯火山岩区,找出由于构造火山活动、相对湖平面变化等因素形成的可作为层序界面的不整合面。碎屑岩岩性区不整合面在地震剖面上主要表现为削蚀、底超、双向下超、顶超、下切谷等;共存区为同时发育火山岩与碎屑岩的削蚀带,不整合面类型较复杂;纯火山岩区表现为相对湖平面下降形成的削蚀不整合面。故可以通过地震、钻测井资料识别各类不整合面,并依据火山喷发方式、火山旋回、沉积旋回,按照不同对比原则进行经典层序地层学划分。     

Petroleum Accumulation: from Continuous to Discontinuous

<正>1 Introduction Petroleum accumulations from the Earth’s crust can be grouped into conventional and unconventional ones.The history of the world’s petroleum exploration is a history from the exploration of conventional accumulations to that of unconventional ones.Nevertheless,petroleum accumulation is actually a contrary process starting from     

储层致密化与油气充注的关系:以三肇凹陷白垩系扶余油层为例

为了明确松辽盆地三肇凹陷扶余油层储层致密化与油气充注相关性,利用微米CT、流体包裹体显微分析、盆地模拟等方法,研究了该储层微观孔喉特征,且定量分析了其成藏期。根据储层孔隙演化信息分析了研究区储层致密化过程和油气成藏的关系。结果发现:三肇凹陷扶余致密储层岩石类型以长石岩屑砂岩和岩屑长石砂岩为主,孔喉特征表现为窄喉道、宽孔隙、孔喉配置差、微细喉道总体积大等特征。压实作用和胶结作用为储层致密化重要成因,储层致密时间应该在嫩江组末之前。流体包裹体分析结果表明三肇凹陷扶余储层油充注分为早期和晚期,相应的充注时间分别距今77~74 Ma、67~65 Ma,分别对应于嫩江组沉积期和明水组沉积末期。综合对比扶余油层油气成藏历史和储层孔隙演化特征,认为原油充注发生储层致密化之后,即先致密后成藏。     

A Numerical Simulation Study of Mass Segregation in Embedded Stellar Clusters

The initial condition of the formation of massive stars is still unclear at present. In particular, it is still debatable whether or not massive stars are formed in the cluster center. Some people considered from the viewpoint of time scale and thought that the mass segregation phenomena in embedded clusters means that the massive stars can only be born in the cluster center. In this paper we used the Monte Carlo method to make numerical simulation of the dynamical evolution of embedded clusters and the result is compared with the observations. It is assumed that at the initial time massive stars are randomly distributed. It was found that, due to the random motions of massive stars, temporary mass segregation may exist at certain times in the course of evolution of a given embedded cluster, and this phenomenon may be very prominent in some of them. It is pointed out that massive star formation in the center is not the only explanation for mass segregation in embedded clusters. In addition, dynamical friction from the gas can effectively reduce the time scale of the dynamical mass segregation. In consequence, the probability of temporary mass segregation is increased.     

Differences between Marine and Terrestrial Shale Gas Accumulation: Taking Longmaxi Shale Sichuan Basin and Yanchang Shale Ordos Basin as Examples

<正>1 Introduction With the rapid development of theory and practice,shale gas has gradually become an important part in diversified energy structure.Though a lot of research have been done mainly for shale gas exploration prospects,geological conditions and shale gas accumulation have been analyzed and summarized,prospective resources have been preliminarily predicted,and favorable exploration and     

Colonization of mine tailings by marine invertebrates

An experiment was conducted to determine if a tailings substrate would inhibit recolonization of benthic macrofauna upon closure of a submarine tailings disposal (STD) operation. Trays of defaunated marine sediment, serving as a reference, and trays of tailings from a proposed gold mine were placed at 21 m depth on the ocean floor to allow colonization via settlement from the water column. Trays of reference sediment and tailings, and cores of ambient sediment were collected 9, 17, and 22 months after tray placement. Probable tray effects, which were desirable given the objectives of this study, precluded direct comparison of ecological succession in the tray sediments to the ambient assemblage. The ambient macrofauna assemblage was distinguishable from the reference sediment and tailings assemblages throughout the experiment and displayed more pronounced seasonality. Differences between the reference sediment and tailings assemblages were generally insignificant, including total abundance, total biomass, number of taxa, average size of individuals, numerically dominant taxa, abundance by ecological guilds, and overall community composition. Upon cessation of STD, recolonization of a benthic macrofauna community should not be inhibited by the presence of these tailings as a benthic substrate.