A Systems Perspective on World-Systems Theory

Abstract

This article presents a conceptual framework that embeds ideas from world-systems theory within the larger systemic context known as the theory of dissipative structures. This article creates a theoretical perspective on global capitalism, both geographic and historical, that offers a sufficiently general and flexible model for this particular complex system in human geography. The goal is to provide a perspective that reflects the interconnectedness of individual and separate places into a larger global system that is a single functioning spatial entity. In this view, the modern world-system becomes a culmination of its past and a prologue to its future.     

黄土高原一次β中尺度大暴雨特征及成因分析

利用NCEP／NCAR逐日6h分析资料和常规观测资料,分析了2011年2月25日一28日山西连续降雪天气过程（以下简称2．25降雪）。①2．25降雪过程经历了三个阶段：2月25日为回流降雪阶段,26日一27日为倒槽冷锋与回流降雪共同影响降雪阶段,28日为低空切变线影响降雪阶段。②2．25降雪过程涵盖了华北地区大到暴雪的三个类型：回流类降雪、倒槽冷锋类降雪、低空切变线类降雪。③通过温湿场分析得出,对于低空切变线类降雪,对流层中层的湿核对降雪的开始有一定的指示意义。降雪未开始之前对流层中层有湿核,随着时间的推移,湿核向低层扩展,整个对流层中低层变为高湿区,降雪开始。当对流层中层变为干区,并向低层扩展,降雪过程结束。对于回流类降雪,低层回流对回流降雪起到冷垫的作用。④通过涡度场分析得出,对流层低层的负绝对涡度中心对其东侧的降水有指示意义,如果其东侧对流层低层配合有正涡度核,降雪强度较大,维持时间较长。⑤地面层出现的负绝对涡度中心说明近地面层有小高压系统的存在,这是因为低层回流冷垫作用形成的孤立小高压体。⑥28日降雪维持机制是条件性对称不稳定。     

一次缓慢东移的黄河气旋暴雨的诊断分析

利用NCEP/NCAR再分析资料和常规气象资料,对2001年6月28-29日发生在河南的一次黄河气旋暴雨过程进行了诊断分析。结果表明：黄河气旋的稳定少动是造成这次暴雨的直接原因,高层辐散与中层正涡度平流对黄河气旋形成和发展起了重要作用。这次过程的水汽主要来自副高东南侧的海上,孟加拉湾的水汽也有一定的贡献。暴雨区的中低层对称不稳定的存在,导致上升运动和水汽输送的加强,造成降水的增幅。     

南海台风Vongfong(2002)登陆前后内核结构和近海加强原因的数值模拟研究

利用6 km细网格区域的显式模拟结果分析了Vongfong(2002)的内核结构;对Vongfong近海加强的动力学机制进行了研究.结果表明:(1) 轴对称性结构中,Vongfong最大风速半径(RMW)在强盛期随高度递减.Vongfong在近海时,低层最强的流入在其移行的前方,而流出区在其后方.这些特征与大西洋飓风和西太平洋台风相反.(2) 动力场和热力场都有明显的不对称结构.在强盛期,对流西北强、东南弱;强对流云带与最大风速区的位置一致.在加强期,低层西冷东暖、中高层西暖东冷;到强盛期,低层和中高层都有明显的暖心结构.(3) 中纬度中上层冷低压系统和台风的相互作用是Vongfong近海加强的重要原因.①由于冷低压系统外围的冷空气从西北侧进入台风的中层,低层有暖湿空气配合,使得位势不稳定能量增加,对流发展.②因为冷低压中心的下沉气流正是二级环流的下沉支,冷低压南移填塞,台风近海加强.两个方面最终通过CISK(第二类条件不稳定)机制来实现.     

New doubly-symmetric families of comet-like periodic orbits in the spatial restricted (N + 1)-body problem

For any positive integer N ≥ 2 we prove the existence of a new family of periodic solutions for the spatial restricted (N +1)-body problem. In these solutions the infinitesimal particle is very far from the primaries. They have large inclinations and some symmetries. In fact we extend results of Howison and Meyer (J. Diff. Equ. 163:174–197, 2000) from N = 2 to any positive integer N ≥ 2.      

Radiation-induced defects in quartz. III. Single-crystal EPR,ENDOR and ESEEM study of a peroxy radical

The X- and W-band single-crystal electron paramagnetic resonance spectra of an electron-irradiated natural quartz permit quantitative analysis of a ²⁹Si hyperfine structure (A ~12.6 MHz) and an ²⁷Al hyperfine structure (A ≤ 0.8 MHz) for a previously reported hole-like center. The ²⁹Si hyperfine structure arises from interaction with two equivalent Si atoms and is characterized by the direction of the unique A axis close to a Si–O bond direction. The ²⁷Al hyperfine structure, confirmed by pulsed electron nuclear double resonance and electron spin echo envelope modulation spectra, is characterized by the unique A axis approximately along a twofold symmetry axis. These ²⁹Si and ²⁷Al hyperfine data, together with published theoretical results on peroxy radicals in SiO₂ as well as our own density functional theory (DFT) calculations on model peroxy centers, suggest this hole-like center to have the unpaired spin on a pair of oxygen atoms linked to two symmetrically equivalent Si atoms and a substitutional Al³⁺ ion across the c-axis channel, a first peroxy radical in quartz. The nuclear quadrupole matrix P also suggests that the Al³⁺ ion corresponds closely to the diamagnetic precursor to the [AlO₄]⁰ center. Electronic supplementary material  The online version of this article (doi:) contains supplementary material, which is available to authorized users.     

鄂尔多斯盆地侏罗纪西界分析

鄂尔多斯盆地西界,特别是其早—中侏罗世盆地西界,由于不同期次、不同性质的构造相互叠加而模糊不清,究竟是在贺兰山以西还是现在银川盆地以东的问题,至今尚无共识,极大地影响着矿产资源的评价和找矿战略的部署。本文在前人工作的基础上,通过针对性的野外工作,分析和筛分了不同时期的古构造,探讨了晚侏罗世和早—中侏罗世盆地的西界。文章认为,鄂尔多斯盆地西部巨大的近南北向挤压构造形成于晚侏罗世,而东西向的挤压构造则出现于晚三叠世。两期方向截然不同的挤压构造相互叠加,构成了鄂尔多斯盆地西部复杂的叠加构造和不规则的盆地西界。晚期挤压构造较为清晰,表现为近南北向的逆冲推覆构造带和纵贯盆地南北的“古脊梁”,使盆地西界退缩到桌子山东麓断裂、横山堡—磁窑堡断褶带以及马儿庄冲断裂和崆峒山断裂以东。早期挤压构造受后期构造的叠加改造,断断续续,时隐时现。近东西向挤压构造受古亚洲域的影响,是印支运动的产物,近南北向挤压构造转受滨太平洋域的作用,是燕山运动的表现。在古亚洲域向太平洋域转换过程中的早—中侏罗世,鄂尔多斯盆地西部出现了近东西向的拉张伸展,在盆地内部表现为近东西向隆起凹陷的古地形,使盆地西缘波状弯曲,而非平直,“银川古隆起”和“汝箕沟—鄂尔多斯盆地”两者并存,并不矛盾。早—中侏罗世盆地西界可能远至阿拉善地块。上述中生代构造又经新生代构造改造,变得更加复杂多样,甚至面目全非。如不注意构造筛分,中生代构造乃至盆地边界的研究就会被误导,从而得出错误结论。     

A straightforward approach for using single time domain simulations to assess characteristic extreme responses

Short-term wave design approach of marine structures, using nonlinear time domain simulations, is a design procedure that is recognized by various modern standard codes. One of the most challenging points of this approach is the evaluation of the characteristic extreme values for response parameters used in the design check equations. The most straightforward and recommended way to evaluate a response characteristic value is by fitting an extreme value probability distribution to the N-sample of extreme values extracted from N independent time domain simulations with duration equal to the short-term period indicated by the code, which is usually taken as 3 h. However, this procedure would not be practical for some types of marine structures, such as risers and mooring lines, under numerous design load cases and demanding huge finite element models. A more feasible approach would be to assess the response extreme value distribution using only a single short-term time domain simulation with duration shorter than 3 h. But reduced time simulations always introduce some additional statistical uncertainty into the extreme values estimates. This paper discusses a workable way of properly taking into account the statistical uncertainty associated with the simulation length in the assessment of a characteristic short-term extreme response value based on a single time series.     

Comparison of Five Numerical Codes for Automated Tracing of Coronal Loops

The three-dimensional (3D) modeling of coronal loops and filaments requires algorithms that automatically trace curvilinear features in solar EUV or soft X-ray images. We compare five existing algorithms that have been developed and customized to trace curvilinear features in solar images: i) the oriented-connectivity method (OCM), which is an extension of the Strous pixel-labeling algorithm (developed by Lee, Newman, and Gary); ii) the dynamic aperture-based loop-segmentation method (developed by Lee, Newman, and Gary); iii) unbiased detection of curvilinear structures (developed by Steger, Raghupathy, and Smith); iv) the oriented-direction method (developed by Aschwanden); and v) ridge detection by automated scaling (developed by Inhester). We test the five existing numerical codes with a TRACE image that shows a bipolar active region and contains over 100 discernable loops. We evaluate the performance of the five codes by comparing the cumulative distribution of loop lengths, the median and maximum loop length, the completeness or detection efficiency, the accuracy, and flux sensitivity. These algorithms are useful for the reconstruction of the 3D geometry of coronal loops from stereoscopic observations with the STEREO spacecraft, or for quantitative comparisons of observed EUV loop geometries with (nonlinear force-free) magnetic field extrapolation models.     

Observations of Low-Latitude Coronal Plumes

Using Fe ix/x 17.1 nm observations from the Extreme-Ultraviolet Imaging Telescope (EIT) on the Solar and Heliospheric Observatory (SOHO), we have identified many coronal plumes inside low-latitude coronal holes as they transited the solar limb during the late declining phase of cycle 23. These diffuse, linear features appear to be completely analogous to the familiar polar plumes. By tracking them as they rotate from the limb onto the disk (or vice versa), we confirm that EUV plumes seen against the disk appear as faint, diffuse blobs of emission surrounding a brighter core. When the EIT images are compared with near-simultaneous magnetograms from the SOHO Michelson Doppler Imager (MDI), the low-latitude, on-disk plumes are found to overlie regions of mixed polarity, where small bipoles are in contact with unipolar flux concentrations inside the coronal hole. The birth and decay of the plumes are shown to be closely related to the emergence of ephemeral regions, their dispersal in the supergranular flow field, and the cancellation of the minority-polarity flux against the dominant-polarity network elements. In addition to the faint polar and nonpolar plumes associated with ephemeral regions, we note the existence of two topologically similar coronal structures: the giant plume-like features that occur above active regions inside coronal holes, and the even larger scale “pseudostreamers” that separate coronal holes of the same polarity. In all three cases, the basic structure consists of open field lines of a given polarity overlying a photospheric region of the opposite polarity; ongoing interchange reconnection at the X-point separating the open field domains from the underlying double-arcade system appears to result in the steady evaporation of material from the closed into the open region.