叠覆式三角洲——一种特殊的浅水三角洲

不同于常规三角洲以分流河道体系所形成的分流河道、河口坝、席状砂等微相为三角洲朵体的基本单元,叠覆式三角洲以内部结构简单的朵体为基本构成单元,朵体相互叠置,形成复合叠合体,进而构成三角洲骨架。单个朵体由河道扫描或扩展而成,复合朵体则是由单朵体侧向迁移或前(退)积而成。三角洲因大量朵体叠置而形成厚层状、内部结构复杂的复合砂体。不同朵体形成于不同时期,因而不存在统一的分流体系,单一沉积体具有层状特征,但不同期朵体受可容空间和地貌控制,呈三维叠置,而非简单的层状叠加,从而使得三角洲内部呈现出拼合式、立体式特点。单朵体是结构的基本单元,发育范围有限,与相邻朵体发育于不同时间单元,因而只能在复合体约束下小范围追踪。单一朵体接触关系及接触界面的渗流能力决定了油气富集和注水开发响应特征。朵体迁移、叠置造成大面积、巨厚的砂层可形成大型油气藏,而同时朵体间泥岩的不均匀分布也造就了砂体局部不连通或朵体间连通性变化,为岩性油气藏形成创造了条件,并且影响了注水开发中的注采对应性,进而影响水驱采油效果。     

福建省紫金山铜金矿床原生晕地球化学特征及深部找矿前景

通过系统采集紫金山铜金矿床4~11线共41个钻孔的岩矿样,绘制原生晕剖面图,建立垂向元素分带序列、矿体剥蚀程度准则,结合深部指示元素的特征,进行隐伏矿预测。该矿床金矿近矿晕为Au-Ag-Zn1,尾部晕为BiGa-Mo-Sn-Ti-Co-Ni-W1-V;铜矿前缘晕为Hg-Sb-As,近矿晕为Cu-Pb1-Zn2,尾部晕为Be-W2。矿体剥蚀程度评价表明,高硫型铜矿体往深部已尖灭。深部F-Mn-Pb2-Zn3的异常形态和元素组合符合典型斑岩矿床的外带特征,斑岩体延伸至矿床周边;深部的蚀变矿物组合、金属矿物组合、流体包裹体特征等均表明深部可能存在斑岩铜(钼)矿床。     

中国娱乐传媒产业全球生产网络的发展路径与地理特征

利用2012年和2017年《福布斯中国名人榜单》中娱乐明星行动轨迹数据探索中国娱乐传媒产业全球生产网络的空间组织模式。研究发现：① 中国娱乐传媒产业的全球化经历了“产品引进”“产品输出”“对外投资并购与跨国生产”几个阶段,具有明显的内需驱动式全球化特点;② 中国娱乐传媒产业生产网络形成较为明显的“核心-边缘”结构,相较于典型制造业生产网络表现出更加快速的动态演化特征;③ 娱乐传媒产业各类价值活动的地理分布呈现出显著的差异,反映出不同价值环节的需求与各区域平台、资源或市场条件的战略耦合关系;④ 中国娱乐传媒产业的国外活动呈现出向西方发达国家和亚洲邻近国家集聚的趋势,体现出发达国家主导的全球娱乐传媒市场结构以及“地理-文化邻近效应”的作用。     

Integrating a Raster Geographical Information System with Multi‐Objective Land Allocation Optimization for Conservation Reserve Design

The multi‐objective land allocation problem is to optimize the selection of land for different uses based on a set of decision objectives. For most applications, a geographical information system (GIS) is either absent or loosely coupled through file exchange. In this article the evolutionary algorithm (EA), a heuristic solution method for optimization problems, is integrated with a raster GIS to form a spatial decision support system (SDSS) for multi‐objective conservation reserve design. The SDSS effectively combines the functions of a GIS for data management, analysis, and visualization, with the optimization capability of the EA; and provides a uniform way to solve conservation reserve design problems with different types of constraints and objectives. The SDSS is demonstrated through application to the creation of conservation reserves in Bolivia to protect 17 endemic mammals.     

《海西交通图集》的编制探讨

《海西交通图集》是以省基础地理信息为基础框架,运用计算机制图技术、数据库技术和全数字桌面出版一体化技术集成制作的综合交通图集,也是一本反映海西交通基础设施及主要成就的图集。对图集的技术创新、内容选题、设计特点等进行分析与探讨。     

Relation between the “Double-Hump” Behavior in the Radio Band and the Broad-Line Luminosity for Blazars

The physics behind the spectral energy distribution (SED) of blazars remains open. We assembled 36 blazars to tackle the factors that control their SED. Now, many blazar spec- tra have the "double hump" feature in the radio and far-IR frequencies. For these a parameter, , is created to characterize the behavior of the SED. We found a significant correlation be- tween the broad-line luminosity (LBLR) and . Because LBLR is an indicator of the accreting power of the source in blazars, we derived a linear correlation, ∝ M˙1/3.18, which suggests that the SED of blazars may depend on the accretion rate, like that of BL Lac objects. We also found a significant correlation between ■ and for a sample of 11 blazars (out of one of 36) with available black hole masses. This implies the Eddington accretion ratio may influence the shape of the SED of blazars.     

ANALYSIS OF MESOSCALE CONVECTIVE SYSTEMS OVER TIBETAN PLATEAU IN SUMMER

1INTRODUCTION In meteorological satellite cloud images, the features of Mesoscale Convective System (MCS) are shown in white bright cloud cluster, cloud band, cloud line, vorti- calcloudsystem,etc. The MCSlife cycle and spatial size usuallyvaryfrom several hours to one day and 100km to approximately 1000km, respectively. In the last two decades, it has been proven that storm and intensive con- vective weather, such as spasmodic thunderstorm and gale, tornado and short macro-precipitati…     

恒星内部电荷屏蔽对电子俘获反应的影响

本文分析了在恒星环境下，电荷强屏蔽对原子核电子俘获反应的影响，分析中忽略了电荷屏蔽对核跃迁矩阵元的影响．作为例子，分别讨论了电荷屏蔽对核素33S、30P和57Fe的电子俘获率的影响．结果表明：在较低温度和较高密度下，由于电荷屏蔽，其电子俘获率相对于无屏蔽情形有明显降低，这可能对恒星晚期演化和超新星爆发理论带来明显的影响．     

The Doppler Effect and Spectral Energy Distribution of Blazars

The relativistic beaming model is adopted to discuss quantitatively the observational differences between radio-selected BL Lac objects (RBLs) and X-ray-selected BL Lac objects (XBLs), and between BL Lac objects and flat spectrum radio quasars (FSRQs). The main results are the following:(1) In the Doppler corrected color-color(αro^in-αox^in) diagram,XBLs and FSRQs occupy separated regions, while RBLs bridge the gap between them. These properties suggest that similar intrinsic physical processes operate in all the objects under a range of intrinsic physical conditions. (2) Our results are consistent with the results of Sambruna, Maraschi and Urry (1996) from other methods. We show the αxox introduced by Sambruna to be a good index for describing the energy distribution because it represents the intrinsic energy distribution and includes the Doppler correction. (3)The Doppler effect of relativistic beaming is the main mechanism, and the physical differences(such as magnetic fields, electron energies) are also important complementary factors for understanding the relation between XBLs and RBLS.     

类星体红移分布△ln（1＋z）＝0．205周期性的一种解释

根据红移定义１＋ｚ＝λｉ／λ０ｉ，我们认为类星体红移分布ｌｎ（１＋ｚ）周期性受两个因素影响。首先，决定类星体红移的主要线（如Ｌα１２１６，ＣＩＶ１５４９，ＣＩＩＩ１９０９，ＭｇＩＩ２７９８，ＮｅＶ３４２６，ＯＩＩ３７２７，ＮｅＩＩＩ３８６８，Ｈγ４３４０，Ｈβ４８６１，ＯＩＩＩ５００７）固有波长可能构成０．２０５的周期性；另外，这些谱线的观测波长进入一定光学窗口对红移有一定限制，在一定条件下，它正好在某些红移出现峰值，并与ｌｎ（１＋ｚ）＝０．２０５预言峰值一致。我们还在这两个基本考虑下进行模拟取样，发现有明显周期性，定量上证实了我们的基本考虑。本文是类星体红移分布的一种解释，它能说明为什么统计分布不同样品能得到不同的结论。进而，我们认为红移分布周期性不能成为内禀红移观点的观测支持。