基于分形理论的公路交通网络与区域经济发展关系的研究   总被引：4，自引：3，他引：1  

沈惊宏  陆玉麒  兰小机 《地理科学》2012,(6):658-665

以安徽省17个地级市公路交通网络为研究对象,用分形技术测算出各等级公路网络的分维数,并构建了度量综合路网的权维数模型。经过实证得出区域路网分维数受路网面积大小影响,继而对地级市进行了面积区划,把各类区的路网权维数、干线分维数和综合经济指数做相关分析。研究发现各市的路网分维数与综合经济指数呈正相关,说明了路网覆盖度越均匀,交通网络越复杂地区经济发展越好。为进一步探求各市公路建设和经济发展之间的协调关系,通过引进公路规模与经济产出的分形模型测算出17个地级市的分维数,发现有合肥市等6城市经济发展超前于公路规模,铜陵等4城市基本一致,马鞍山等7城市经济发展滞后于公路建设规模。  相似文献   

1947～2007年上海中心城区居住空间分异变化——基于居住用地类型视角   总被引：4，自引：2，他引：2  

廖邦固  徐建刚  梅安新 《地理研究》2012,31(6):1089-1102

采用4种分异度测度模型,在街坊尺度和乡镇尺度下,对上海中心城区1947～2007年11个时相的各类居住用地空间分异程度进行计算。发现1949年后各类居住用地分异度呈现不同的波动过程。不同时期居住用地总体分异程度的计算表明,1949年前空间分异严重,计划经济时期有所降低,转型期则又明显上升。不同时期居住用地等级高低与其分异度大小呈现不同的结构特征,1949年前高等级居住用地分异度高、中低等级居住用地分异度较低,形成"一高两低"结构;计划经济时期则是居住用地等级越高,分异度越大的"正相关"结构;90年代后则是最高和最低等级的居住用地分异度高,而中等居住用地分异度最低的"V"型结构。不同时期居住用地空间分异结构特征间的演进,直接原因是新式住宅的建设和旧城的改造,深层次原因则是土地使用制度的变迁和城市空间组织模式的转变。  相似文献   

中国自然文化遗产的价值体系及保护利用   总被引：1，自引：0，他引：1  

陈耀华  刘强 《地理研究》2012,31(6):1111-1120

对自然文化遗产价值的正确认识是处理遗产地保护和利用关系的基础,也是解决遗产地"城市化、商业化、人工化"的前提。本文在梳理国内外对自然文化遗产价值的诸多认识的基础上,依据系统论观点,提出了中国自然文化遗产价值是由"本底价值、直接应用价值和间接衍生价值"构成的"价值体系"。该体系具有明显的层次性,其中本底价值是所有价值存在的基础,这决定了遗产资源必须在保护的前提下才能合理利用;该体系也有空间性,三种价值主要分别存在于遗产地范围以内、遗产地及相邻区域、遗产地范围以外的更大的区域。于是,对自然文化遗产的保护和利用要坚持三个基本原则:严格保护本底价值,确保遗产的真实性和完整性不受损害;适度利用直接应用价值,做到功能综合利用、产品综合开发、产业综合发展;大力发展间接衍生价值,充分发挥其空间结构关联效应和产业发展乘数效应,从而达到带动遗产地所在区域社会、经济发展的目的。  相似文献   

规模经济、对外贸易与区域双核结构模式探讨——以山东半岛济南—青岛双核结构为例     

盛科荣  孙威 《地理科学进展》2012,31(12):1636-1644

区域双核结构模式是一种重要的经济地理现象。基于新经济地理学的研究视角和分析框架,论文构建模型,分析了规模经济和对外贸易推动区域双核结构模式的生成过程和经济机理。模型研究表明,规模经济和对外贸易是塑造区域双核结构模式的基本力量:规模经济的增强放大了本地市场效应,导致了区域核心城市的出现;对外贸易影响着沿海地区的经济地理优势,决定着港口区位核心城市和内陆地区核心城市的并存。山东半岛济南—青岛双核结构模式生成过程的实证研究也表明,双核结构模式是制造业活动完成由以手工业为主导向现代化大生产为主导转变、区域发展环境完成由相对封闭向相对开放转变之后才产生的经济地理现象。  相似文献   

海冰离散元模型的研究回顾及展望   总被引：2，自引：0，他引：2       下载免费PDF全文

季顺迎  李春花  刘煜 《极地研究》2012,24(4):315-330

为描述极区及副极区海冰在不同尺度下的离散分布特性,以及海冰与海洋结构相互作用过程中的破碎性能,海冰的离散单元模型从上世纪80年代发展起来并不断完善。本文将海冰离散单元模型分为地球物理尺度( ~100km)、浮冰块尺度(10m ~ 10km)和海洋结构尺度(1m ~ 100m)等三种不同尺度,讨论了不同尺度下海冰的离散分布规律或海冰由连续状态向离散状态转化的动力过程。通过对块体、圆盘和颗粒不同形态的海冰离散单元模型的介绍,对其在极区海冰的动力特性、海冰重叠堆积及其与波浪的作用过程、海冰与海洋结构的相互作用中的应用进行了分析,对海冰强度的尺度效应进行了讨论。最后,讨论了海冰离散单元模型中存在的问题和重点研究内容。  相似文献   

Prediction of satellite orbits contraction due to diurnally varying oblate atmosphere and altitude-dependent scale height using KS canonical elements     

Xavier James Raj 《Planetary and Space Science》2009,57(11):1312-1320

A new non-singular analytical theory for the motion of near-Earth satellite orbits with the air drag effect is developed in terms of uniformly regular KS canonical elements. Diurnally varying oblate atmosphere is considered with variation in density scale height dependent on altitude. The series expansion method is utilized to generate the analytical solutions and terms up to fourth-order terms in eccentricity and c (a small parameter dependent on the flattening of the atmosphere) are retained. Only two of the nine equations are solved analytically to compute the state vector and change in energy at the end of each revolution, due to symmetry in the equations of motion. The important drag perturbed orbital parameters: semi-major axis and eccentricity are obtained up to 500 revolutions, with the present analytical theory and by numerical integration over a wide range of perigee height, eccentricity and inclination. The differences between the two are found to be very less. A comparison between the theories generated with terms up to third- and fourth-order terms in c and e shows an improvement in the computation of the orbital parameters semi-major axis and eccentricity, up to 9%. The theory can be effectively used for the re-entry of the near-Earth objects, which mainly decay due to atmospheric drag.  相似文献   

Contraction of near-Earth satellite orbits using uniformly regular KS canonical elements in an oblate atmosphere with density scale height variation with altitude     

M. Xavier James Raj 《Planetary and Space Science》2009,57(1):34-41

A new non-singular analytical theory for the contraction of near-Earth satellite orbits under the influence of air drag is developed in terms of uniformly regular Kustaanheimo and Stiefel (KS) canonical elements using an oblate atmosphere with variation of density scale height with altitude. The series expansions include up to fourth power in terms of eccentricity and c (a small parameter dependent on the flattening of the atmosphere). Only two of the nine equations are solved analytically to compute the state vector and change in energy at the end of each revolution, due to symmetry in the equations of motion. It is observed that the analytically computed values of the semi-major axis and eccentricity are consistent with the numerically integrated values up to 500 revolutions over a wide range of the drag-perturbed orbital parameters. The theory can be effectively used for re-entry of near-Earth objects.  相似文献   

Towards quantitative control on discreteness error in the non-linear regime of cosmological N-body simulations     

M. Joyce  B. Marcos  T. Baertschiger 《Monthly notices of the Royal Astronomical Society》2009,394(2):751-773

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The kinematics and zero-point of the log P–〈M_K〉 relation for Galactic RR Lyrae variables via statistical parallax     

A. K. Dambis 《Monthly notices of the Royal Astronomical Society》2009,396(1):553-569

We use accurate absolute proper motions and Two-Micron All-Sky Survey   K_s   -band apparent magnitudes for 364 Galactic RR Lyrae variables to determine the kinematical parameters of the Galactic RR Lyrae population and constrain the zero-point of the   K_s   -band period–luminosity relation for these stars via statistical parallax. We find the mean velocities of the halo- and thick-disc RR Lyrae populations in the solar neighbourhood to be  [ U ₀(Halo), V ₀(Halo), W ₀(Halo)]= (−12 ± 10, −217 ± 9, −6 ± 6) km s⁻¹  and  [ U ₀(Disc), V ₀(Disc), W ₀(Disc)]= (−15 ± 7, −44 ± 7, −25 ± 5) km s⁻¹  , respectively, and the corresponding components of the velocity-dispersion ellipsoids,  [σ V_R (Halo), σ V _θ(Halo), σ W (Halo)]= (167 ± 9, 86 ± 6, 78 ± 5) km s⁻¹  and  [σ V_R (Disc), σ V _θ(Disc), σ W (Disc)]= (55 ± 7, 44 ± 6, 30 ± 4) km s⁻¹  , respectively. The fraction of thick-disc stars is estimated at  0.25 ± 0.03  . The corrected infrared period–luminosity relation is     , implying a Large Magellanic Cloud (LMC) distance modulus of  18.27 ± 0.08  and a solar Galactocentric distance of  7.58 ± 0.40 kpc  . Our results suggest no or slightly prograde rotation for the population of halo RR Lyraes in the Milky Way.  相似文献   

Microstructure of Turbulence in the Stably Stratified Boundary Layer   总被引：1，自引：1，他引：0  

Zbigniew Sorbjan  Ben B. Balsley 《Boundary-Layer Meteorology》2008,129(2):191-210

The microstructure of a stably stratified boundary layer, with a significant low-level nocturnal jet, is investigated based on observations from the CASES-99 campaign in Kansas, U.S.A. The reported, high-resolution vertical profiles of the temperature, wind speed, wind direction, pressure, and the turbulent dissipation rate, were collected under nocturnal conditions on October 14, 1999, using the CIRES Tethered Lifting System. Two methods for evaluating instantaneous (1-sec) background profiles are applied to the raw data. The background potential temperature is calculated using the “bubble sort” algorithm to produce a monotonically increasing potential temperature with increasing height. Other scalar quantities are smoothed using a running vertical average. The behaviour of background flow, buoyant overturns, turbulent fluctuations, and their respective histograms are presented. Ratios of the considered length scales and the Ozmidov scale are nearly constant with height, a fact that can be applied in practice for estimating instantaneous profiles of the dissipation rate.  相似文献