1998-2009年间台风不活跃期间热带云团活动分析

热带云团是台风生成的前兆,虽然一些研究将近20 a来台风不活跃与大尺度环境场相联系,但是还没有人分析台风不活跃期热带云团的活动特点。本文利用目前仅有的1989-2009年全球热带云团资料,分析了西北太平洋热带云团近20 a的变化特征。1998年以后西北太平洋台风生成减少主要发生在7-10月,集中在南海（13～23°N,110～120°E）和西北太平洋台风活动区域的东部（13～23°N,145～170°E）。热带云团除1月外各月都有增加的趋势,特别是与台风生成显著减少区域相联系的热带云团活动具有显著的增加趋势。通过对NCEP/NCAR再分析资料分析发现,1998年后热带云团活动增加与环境风垂直切变增加有关,而增强的垂直切变不利于台风生成。     

孔隙性砂岩中单条变形带与簇状变形带的特征与区别——以远安地堑上白垩统红花套组中变形带为例

孔隙性砂岩中的变形带研究近年来取得长足进展,但有关单条变形带与簇状变形带如何区分和界定仍是一个较模糊的问题。本文以远安地堑上白垩统红花套组高孔砂岩中发育的剪切增强压实带和压实剪切带为例,对单条及簇状变形带的特征和区别做出系统分析。研究表明,虽然单条变形带的长度、宽度、错断位移、凸起高度等均明显小于簇状变形带,但是不同运动学成因的变形带宏观特征、微观结构不同,因此不能单纯以规模大小区分二者,需要结合带密度将簇状变形带与变形带列、网格构造等相区分,还需要结合其微观结构特征进行准确鉴定。单条及簇状剪切增强压实带特征类似,均不具核心碎裂带,颗粒主要为中等破碎,多表现为多个不连续分布的碎裂核。簇状剪切增强压实带内部的非均质性更强。单条压实剪切带具有核心碎裂带,依剪切力大小不同,其核心碎裂带内颗粒粉碎程度及边缘过渡带宽度不同,常伴随微小剪切缝痕迹。簇状压实剪切带在镜下可清晰识别出不同的核心碎裂带、带间区域及微小剪切缝,可见S—C组构和断续分布的滑动面。单条及簇状变形带的发育会不同程度地改变储层的物性并可能会对油气运移和开采产生影响。     

青藏高原云团东传过程及其中中尺度对流系统的统计特征

利用逐小时风云卫星TBB资料、逐小时中国自动站与CMORPH降水产品融合数据以及国家级地面观测站24小时累积降水量,统计分析2010～2016年夏季,伴随下游地区（104°E以东）降水的青藏高原云团东传过程以及东传过程中镶嵌于云团中的中尺度对流系统（Mesoscale Convective System,简称MCS）特征。结果表明,共出现120次伴随下游降水的高原云团东传过程,6月出现最频繁,但持续时间较长的过程多出现在7月。云团向东传播的主要三条路径是平直东传、沿长江折向东传和复合东传。其中路径二——沿长江折向东传中的过程是高影响过程,因为过程次数较多（46次）,过程平均持续时间较长（62小时）,在下游地区引发的降水日数和暴雨日数最多。属于东传过程的MCS在7月形成最多,集中分布在青藏高原东坡、云贵高原东部、长江沿岸及其以南地区。高原MCS影响长江中下游地区降水主要是通过向东传播的形式实现,因为即使生命史更长的中α尺度对流系统（Meso-α Convective System,简称MαCS）也鲜少直接移动至110°E以东地区。不同区域的中α尺度持续性拉长形对流系统（Permanent Elongated Convective System,简称PECS）的日变化特征显示,东传过程MCS更容易在夜间从高原东坡向东传播至下游地区。在三条路径中,路径二中的东传过程MCS数量最多、在下游地区发展最旺盛并与降水日数和覆盖范围存在更好的对应关系。     

制造业活动地理转移视角下的中国产业集群问题

在简要回顾产业集群理论的基础上,在制造业活动地理转移的视角下,结合案例重新审视了我国劳动密集型产业集群的形成及发展.作者认为,一些锁定在低成本竞争的集群正在或已经老化,甚至衰亡.另一些集群中的企业有过度集聚的问题,还有一些中小企业集聚的区域根据产业特征需要增加产业集中度.因为集群的这些问题,随成本上升,出现了集群中企业的加工制造环节外移的现象.这种现象挑战了新产业区理论中集群是"在流动的全球空间中的粘结的区位"的观点.根据集群中企业外移现象,就产业承接地的规划和发展,以及转出地那些正在升级的集群的地理稳定性和生产者服务业的发展问题,提出了几点看法.     

创意再生视域宁波老工业区绅士化动力机制

绅士化成为全球各类城市更新的核心现象,受地理、城市和规划等学科关注。以宁波和丰创意广场形成为例,运用问卷调查和访谈数据,借助扎根理论和结构方程模型分别构建和验证涵盖空间生产、推拉模式和创意集群孕育在内的老工业区绅士化动力机制。研究发现：① 生成和丰创意广场的创意修复过程呈现典型绅士化现象,且该现象具有高端写字楼主导的开放性和多元景观特征,入园企业私营化、生产要素创意化和生产关系外向化的业态特征以及年轻化、情怀化、创意化和服务化的群体特征;② 和丰绅士化现象是老工业区以推拉方式形成的社会空间置换,权力、资本和创意联结而成的再生产关系主导空间实践;建筑规划师和创意阶层主导的物质性空间营造和创意实践形成空间表征;空间表征推动创意集群内生发展和演化,催化了基于文化、理想和情感体验的文化共识和身份认同,升华为表征性空间,形成了“地方元素的感性认可→资本要素和关系力量的理性约束→地方元素、资本要素和关系力量协同→关系力量的反馈”逻辑路径,激活了老工业区空间演化。③ 和丰创意集群育成取决于文化氛围、办公环境、经济区位、政府政策和社会关系网络等要素相互作用。     

A density-based approach for detecting network-constrained clusters in spatial point events

Existing spatial clustering methods primarily focus on points distributed in planar space. However, occurrence locations and background processes of most human mobility events within cities are constrained by the road network space. Here we describe a density-based clustering approach for objectively detecting clusters in network-constrained point events. First, the network-constrained Delaunay triangulation is constructed to facilitate the measurement of network distances between points. Then, a combination of network kernel density estimation and potential entropy is executed to determine the optimal neighbourhood size. Furthermore, all network-constrained events are tested under a null hypothesis to statistically identify core points with significantly high densities. Finally, spatial clusters can be formed by expanding from the identified core points. Experimental comparisons performed on the origin and destination points of taxis in Beijing demonstrate that the proposed method can ascertain network-constrained clusters precisely and significantly. The resulting time-dependent patterns of clusters will be informative for taxi route selections in the future.     

Density profiles and luminosity functions of the globular clusters M3 and M92

Tautenburg Schmidt plates with the globular clusters M3 and M92 were measured on the APM facility in Cambridge, mainly for astrometric purposes. The data were used to derive the radial density profiles and the luminosity functions of these clusters. There is a good agreement of our results with formerly ones derived by other authors. In both clusters effects of mass segregation are observed.     

Essential properties of the cD galaxy in Abell 1795 — II. Radio structure

We consider current problems connected with the evolution of central dominant (cD) galaxies in clusters. In the second part of this series, internal properties of the cD galaxy — in particular its radio structure — are related to the appropriate ones of the cluster. The observations point to an earlier jet ejection along the major axis of the galaxy and a following change of the jet axis. From the existence of “hot-spot” like regions in different directions it is suggested that the radio engine would have to be intermittent with a relatively short period. Alternatively to the intermittent ejection scenario, the radio morphology of 4C 26.42 can be explained in the frame of the “standard” beam or jet model. The radio structure of 4C 26.42 being an inversion-symmetric configuration, which is probably due to galactic cannibalism, could be interpreted as a transition at the inner hot spots (at about 1 kpc) from supersonic, stable Fanaroff-Riley type II jets to subsonic, unstable FR I type structures (“plumes”). A quantitative investigation of the two scenarios for jet interaction with the surroudning interstellar/intercluster medium in 4C 26.42 gives parameter values in reasonable agreement with the ones discussed in the literature for related objects.     

On the periodical structures in populations of galaxies and of clusters of galaxies

Analysing the distribution of the redshift of clusters of galaxies, obtained from the catalogue of SCHMIDT (1986), two already known periodical structures were confirmed and both periods were extended by a number of periods — approximately by two times (We elucidated 5 new periods in the first structure and 4 in the second.). The statistical significance of these structures was estimated to 0.01 in the first case and to 0.02 in the second one. Particularly, the second structure may be the largest known object in the Universe (about 900 Mpc at H = 75 km s^-1 Mpc^-1). These results agree with the predictions of the axion-dominated early Universe. In addition, we discovered periodical structures of an another type — in luminosity functions of galaxies, which are members of rich clusters. Bei der Analyse des Katalogs von SCHMIDT (1986) wurden zwei periodische Strukturen in den Verteilungen der Rotverschiebungen von Galaxienhaufen festgestellt. In den beiden Strukturen wurden 5 bzw. 4 neue Perioden beobachtet, weshalb sich die Periodenzahl in jeder der beiden Strukturen etwa verdoppelt hat. Die statistische Signifikanzen dieser Strukturen wurden zu 0.01 und 0.02 abgeschätzt. Möglicherweise entspricht die zweite Struktur dem größten bekannten Objekt des Weltalls (etwa 900 Mpc bei H = 75 km s^-1 Mpc^-1). Diese Resultate stützen die Theorie eines axiondominierten frühen Universums. Außerdem wurden weitere periodische Strukturen in der Leuchtkraftfunktion von Galaxien aus reichen Galaxien-haufen entdeckt.