中国-东盟自贸区城市群空间经济关联研究——基于社会网络分析法的视角

从城市群的角度运用社会网络分析法对中国-东盟自贸区空间经济联系进行研究,首先从度、入度、出度3个角度对自贸区内的44个城市建立网络模型分析城市之间的复杂关系。其次对网络图进行中心度分析,判断城市的经济辐射范围,基于核心-边缘理论对自贸区内44个城市划分。最后利用派系过滤算法对城市网络图进行社团结构分析,利用K-plex算法进行凝聚子群分析。分析结果表明自贸区内城市之间存在密切的联系,核心城市群与边缘城市群圈层明显;同时中国在自贸区内扮演着重要角色,带动国家经济关系建设,促进区域经济的繁荣发展。     

Is the world's economic centre of gravity already in Asia?

This paper proposes a novel and simple measure of the world's economic centre of gravity. Over the recent decades, this centre has shifted towards Asia, but is still located in Europe.     

一种优化的交通网络及其在实践中的应用

增长三角是协调城市体系功能、加速区域发展的有效方式。根据中点优先极化的原理和重心极化原理,容易推出两种具有分形特征的三角网络:中点极化网和重心极化网。引入分枝维的概念,对两种分形网络进行维数计算;认为中点极化网既有增长三角的优势又有优化的分形维数,是较为理想的城市体系交通网络配置。基于这种认识,以河南省中心城市群为例,计算出该区的交通网络分维数为1.4375,根据与中点极化网分维数的差距和该网络现有问题,规划了理想的交通网络模式。     

登陆北上影响山东的9216号强热带风暴

对北上影响山东造成重大灾害的９２１６号强热带风暴进行了分析。涡度诊断分析和能量场分析表明，该热带风暴低压一直沿着正涡度中心及高能轴方向移动。暴雨中心集中在高能舌顶热附近，并与正涡度中心相一致。     

基于重心基准的平面坐标转换研究

不同平面直角坐标系的转换包括平移、旋转和尺度因子4个参数,当转换系数矩阵严重病态时,参数解不可靠。考虑到自由网平差中的重心基准条件与转换模型的相关性,通过附加重心基准条件消去两个平移参数来解决转换矩阵严重病态的问题,从而求出正确的坐标转换参数。用实例对该方法进行了验证。     

The circumnuclear material in the Galactic Centre: a clue to the accretion process

On the basis of 'sticky particle' calculations, it is argued that the gas features observed within 10 pc of the Galactic Centre — the circumnuclear disc (CND) and the ionized gas filaments — as well as the newly formed stars in the inner 1 pc can be understood in terms of tidal capture and disruption of gas clouds on low angular momentum orbits in a potential containing a point mass. The calculations demonstrate that a dissipative component forms a 'dispersion ring', an asymmetric elliptical torus precessing counter to the direction of rotation, and that this shape can be maintained for many orbital periods. For a range of plausible initial conditions, such a structure can explain the morphology and kinematics of the CND and of the most conspicuous ionized filament. While forming the dispersion ring, a small cloud with low specific angular momentum is drawn into a long filament which repeatedly collides with itself at high velocity. The compression in strong shocks is likely to lead to star formation even in the near tidal field of the point mass. This process may have general relevance to accretion on to massive black holes in normal and active galactic nuclei.     

从金矿的找矿矿物学研究看量子矿物学的发展

在太行山地区用几种新的矿物学方法对金矿床的载金矿物-黄铁矿和石英进行了矿物物理学方面的测试研究,从中获得了石英红外吸光度、O~--Al心浓度、红外光谱以及黄铁矿的热电性质、热电系数等与矿体的含金性具有密切相关关系,可以作为金矿找矿的有效方法。这些方法的引入,说明新的边缘学科——量子矿物学已经形成,并正在发展。     

上海洋山深水港建设的地域空间作用分析

论述上海洋山深水港的建港条件及其港区工程组合特征,分析洋山港建成后的地域空间作用。建成后的洋山港水深达15 m以上,并由32.5 km长的东海大桥连接洋山深水港区和上海芦潮港物流园区,可以解决上海河口港不能停靠第五、六代集装箱船的问题,改变了上海港的格局。同时提高了上海国际航运中心在东北亚地区港口中的竞争力,带动了长江三角洲、长江流域及全国的经济发展。     

Kinematics of hypervelocity stars in the triaxial halo of the Milky Way

Hypervelocity stars (HVSs) ejected by the massive black hole at the Galactic Centre have unique kinematic properties compared to other halo stars. Their trajectories will deviate from being exactly radial because of the asymmetry of the Milky Way potential produced by the flattened disc and the triaxial dark matter halo, causing a change of angular momentum that can be much larger than the initial small value at injection. We study the kinematics of HVSs and propose an estimator of dark halo triaxiality that is determined only by instantaneous position and velocity vectors of HVSs at large Galactocentric distances ( r ≳ 50 kpc). We show that, in the case of a substantially triaxial halo, the distribution of deflection angles (the angle between the stellar position and velocity vector) for HVSs on bound orbits is spread uniformly over the range 10°–180°. Future astrometric and deep wide-field surveys should measure the positions and velocities of a significant number of HVSs, and provide useful constraints on the shape of the Galactic dark matter halo.     

Polarization of X-ray emission from the Sgr B2 cloud

The Sgr B2 giant molecular cloud is claimed to be an 'X-ray reflection nebula'– the reprocessing site of a powerful flare of the Sgr A* source, which occurred a few hundred years ago. The shape of the X-ray spectrum and the strength of the iron fluorescent line support this hypothesis. We argue that the cleanest test of the origin of X-rays from Sgr B2 would be a detection of polarized emission from this source.