长江经济带城市水资源利用效率的空间关联网络及形成机制

探讨城市水资源利用效率空间关联网络特征及其形成机制可为实现区域用水效率协同提升提供新的政策视角。本文以长江经济带107个地级及以上城市为研究样本,首先,利用随机前沿分析法（SFA）测算出其2009—2018年水资源利用效率,并基于此构建其空间关联矩阵,继而采用社会网络分析法考察城市水资源利用效率空间关联网络的整体结构、个体结构及其空间聚类方式,最后采用二次指派程序法探讨网络形成机制。结果表明：① 城市水资源利用效率整体仍处于较低水平,但研究期内提升显著,空间关联网络格局显现,且整体网络可达性较强,几乎不存在非对称性可达的联系对,仍存在关联不紧密、网络结构稳定性欠佳等问题;② 上中下游地区的中心城市发挥着中心行动者、中介沟通者的重要作用,呈现“中心城市—非中心城市”的“核心—边缘”空间分布特征;③ 城市水资源利用效率空间关联板块可划分为净溢出、主受益和双向溢出板块,各板块成员组成符合长三角城市群、长江中游城市群、成渝城市群的分布特征;④ 城市间地理邻近性差异、经济发展水平差异、对外开放程度差异等自然地理条件和社会经济因素对城市水资源利用效率关联网络的形成具有显著影响。     

基于行动者网络理论的乡村绅士化演化过程与机制解析——以广西巴马盘阳河流域为例

乡村绅士化是城乡要素双向流动背景下乡村转型与振兴的新型路径。基于对广西巴马盘阳河流域乡村绅士化现象的历时性田野调查,采用行动者网络理论解析乡村绅士化演化的过程、类型与机制。研究表明：在巴马盘阳河流域乡村人类行动者与非人类行动者、“草根”行动者与机构行动者共同缔结的行动者网络的转换过程中,伴随关键行动者从“候鸟人”先锋、屯社精英向地方政府、投资开发商的更替,乡村绅士化路径从“草根”绅士化向机构绅士化演替,乡村产业从接待“候鸟人”、发展旅游转向大健康产业融合发展,乡村绅士化类型从单一的舒适移民绅士化向舒适移民、旅游和地产共构的“一地多类”绅士化演化。关键行动者更替及其功能角色转换、绅士化路径变迁和主导产业更替与融合发展、宏观乡村发展制度与地域自然人文环境共同作用于乡村绅士化的阶段演替与类型共生。行动者网络理论与方法利于呈现乡村绅士化的阶段演替脉络与共生演化特征,并揭示乡村绅士演化的一般机制与地域机制。     

面向全域全要素的广州市国土空间规划传导体系研究

建立科学清晰的传导体系是保障规划治理效力的重要前提。随着全国各层级国土空间规划编制与改革的推进,空间规划体系雏形初显,明确各级、各类规划编制内容、管理权限和传导路径,已成为各级政府十分关切的问题。文章基于广州国土空间规划试点的编制实践,针对原有规划体系中指标分解难、控制线管控标准不一、用地管控尺度和精度不一、设施管控缺乏分级等问题,以全域全要素管控为目标,提出了广州建立“四级三类”规划传导体系及实施评估监督的建议,认为一是要在纵向传导上,强化规划编制和“市—区—街道”行政管理体系的衔接,构建“市域—区—单元—地块”4个纵向传导层级,重点围绕“目标战略、底线管控、功能与用地管控、设施管控”4类核心管控内容明确各层级编制内容和深度;二是要在横向传导上,构建专项规划与各层级规划的“联系-反馈”机制,推进专项规划与总体层面规划同步编制,达成管控要求、核心指标等方面的共识,并加强详细规划层面的设施评估反馈,细化详细规划在指标、名录、位置、结构4个方面的传导要求。     

海南省城乡关系演化及驱动机制研究

推进城乡一体化协调发展是事关海南自由贸易港建设成效的重点任务之一,新的发展环境及政策框架正促使海南省城乡关系快速转型。采用变异系数法、耦合协调度模型、回归模型,从城乡空间、经济和社会等维度,分析了建省办特区以来海南省城乡关系演化特征及驱动机制。结果表明：①建省办特区以来,海南省城乡协调综合指数呈现明显的先降后升态势,由1988年的0.319 9到1993年的0.153 9,2019年达0.851 9;②海南省城乡各子系统耦合度和耦合协调度均呈波动上升态势,耦合度主要处于磨合和高水平耦合阶段,耦合协调度由轻度失调转变为初级协调,最后达到中级协调,城乡各子系统间相互作用增强;③海南省城乡关系演化经历城乡二元加剧、城乡二元固化、城乡关系趋缓和城乡一体化初期四个阶段,低水平城乡均衡发展是重要特征,高质量推进城乡一体化协调发展是关键;④经济发展对城乡协调发展影响最为明显,但呈负相关,其次为市场消费、产业结构、乡村发展、交通通达性、城镇发展和政府行为,对外开放对城乡关系演化影响相对较弱;⑤制度创新、对外合作、产业优化、城镇建设和乡村振兴是推进城乡融合发展的重要路径。     

Urban land development intensity: New evidence behind economic transition in the Yangtze River Delta,China

Over the past 20 years, China has experienced multiple economic transitions characterized by marketization, globalization, decentralization, and urbanization; as a result, urban land development intensity (ULDI) has become a significant issue for sustainable development. As China’s largest globalized urban area, the rapid socio-economic development of the Yangtze River Delta has created a huge demand for urban land. We apply a theoretical framework for a four-dimensional analysis tool to understand the dynamic evolution of the ULDI in the context of economic transition. It reveals that marketization, globalization, decentralization, and urbanization affect the ULDI in the economic transition of Yangtze River Delta. Marketization, especially the continuous improvement of land marketization, optimizes the spatial allocation of land resources and encourages urban land users to improve ULDI. Globalization promotes the rapid growth of economy and population through an increase in foreign direct investment. In the process of decentralization, local governments rely on developing a mode of land finance, resulting in a disordered urban space and low ULDI. Population growth and agglomeration during urbanization stimulates residents’ consumption capacity and promotes economic growth, thus creating a greater demand for urban land. However, a low level of development and utilization restricts the improvement of development intensity. Economic development can improve the level of land-intensive use by promoting the adjustment, optimization, and upgrade of urban industrial structures.     

The Zeeman effect in the Sobolev approximation: applications to spherical stellar winds

Modern spectropolarimeters are capable of detecting subkilogauss field strengths using the Zeeman effect in line profiles from the static photosphere, but supersonic Doppler broadening makes it more difficult to detect the Zeeman effect in the wind lines of hot stars. Nevertheless, the recent advances in observational capability motivate an assessment of the potential for detecting the magnetic fields threading such winds. We incorporate the weak-field longitudinal Zeeman effect in the Sobolev approximation to yield integral expressions for the flux of circularly polarized emission. To illustrate the results, two specific wind flows are considered: (i) spherical constant expansion with   v ( r ) = v _∞  and (ii) homologous expansion with   v ( r ) ∝ r   . Axial and split monopole magnetic fields are used to schematically illustrate the polarized profiles. For constant expansion, optically thin lines yield the well-known 'flat-topped' total intensity emission profiles and an antisymmetric circularly polarized profile. For homologous expansion, we include occultation and wind absorption to provide a more realistic observational comparison. Occultation severely reduces the circularly polarized flux in the redshifted component, and in the blueshifted component, the polarization is reduced by partially offsetting emission and absorption contributions. We find that for a surface field of approximately 100 G, the largest polarizations result for thin but strong recombination emission lines. Peak polarizations are approximately 0.05 per cent, which presents a substantial although not inconceivable sensitivity challenge for modern instrumentation.     

Evolution of the mass function of dark matter haloes

We use a high-resolution ΛCDM numerical simulation to calculate the mass function of dark matter haloes down to the scale of dwarf galaxies, back to a redshift of 15, in a  50 h ⁻¹ Mpc  volume containing 80 million particles. Our low-redshift results allow us to probe low-σ density fluctuations significantly beyond the range of previous cosmological simulations. The Sheth & Tormen mass function provides an excellent match to all of our data except for redshifts of 10 and higher, where it overpredicts halo numbers increasingly with redshift, reaching roughly 50 per cent for the  10¹⁰–10¹¹ M_⊙  haloes sampled at redshift 15. Our results confirm previous findings that the simulated halo mass function can be described solely by the variance of the mass distribution, and thus has no explicit redshift dependence. We provide an empirical fit to our data that corrects for the overprediction of extremely rare objects by the Sheth & Tormen mass function. This overprediction has implications for studies that use the number densities of similarly rare objects as cosmological probes. For example, the number density of high-redshift  ( z ≃ 6) QSOs  , which are thought to be hosted by haloes at 5σ peaks in the fluctuation field, are likely to be overpredicted by at least a factor of 50 per cent. We test the sensitivity of our results to force accuracy, starting redshift and halo-finding algorithm.