Spatial Concentration in Australian Regional Development,Exogenous Shocks and Regional Demographic Outcomes: a South Australian case study     

Peter Smailes  Trevor Griffin  Neil Argent 《The Australian geographer》2016,47(4):527-545

ABSTRACT

As a tribute to the massive contribution of our friend and colleague Graeme Hugo to the population and settlement geography of Australian rural areas, this paper presents a longitudinal study from his home State. It forms part of a wider study of the long-term demographic relationships between Australia’s rapidly growing regional cities and their surrounding functional regions. Of particular interest is the question of what effect the accelerating concentration of population and economic activity into a given regional city will have for the longer term demographic sustainability of its functional region as a whole. Taking the case of Port Lincoln, regional capital of most of South Australia’s Eyre Peninsula, it examines the nature of change in the functional region over the period 1947–2011, and investigates the forces feeding, and partly counteracting, the population concentration process, informed by concepts of evolutionary economic geography. In particular it traces the demographic impact (particularly differential migration and ageing trends) of exogenous shocks to the region’s essentially primary productive economic base during the period of major change from 1981 to 2011.  相似文献   

冕洞阻碍太阳高能粒子事件形成的典型事例分析          下载免费PDF全文

申成龙  汪毓明  叶品中  王水 《地球物理学报》2006,49(3):629-635

通过对比两次快速晕状日冕物质抛射(CME)事件,分析相应的日面和行星际的观测资料,发现源区距离冕洞较远的CME引起了极强的太阳高能粒子(Solar Energetic Particle,SEP)事件,而源区非常靠近冕洞的CME则没有引起大的SEP事件.该结果表明,冕洞可能对CME形成SEP事件有阻碍作用.继而分析1997～2003年所有爆发在冕洞边缘的快速晕状CME,发现源区离冕洞距离小于02Rs(太阳半径)的CME均没有引起大的SEP事件.从而进一步证实了冕洞可能对邻近CME形成大SEP事件有影响,它阻碍SEP事件的形成.最后讨论了冕洞阻碍CME形成大SEP事件的可能原因.  相似文献   

1932年昌马地震构造力学特征探讨     

郭万武  张范民 《内陆地震》1994,8(1):75-80

１９３２年昌马地震构造力学特征探讨郭万武，张范民，邢成起，温增平（国家地震局兰州地震研究所，兰州）ＤＩＳＣＵＳＳＩＯＮＯＮＴＨＥＴＥＣＴＯＮＯＭＥＣＨＡＮＩＣＦＥＡＴＵＲＥＳＯＦ１９３２ＣＨＡＮＧＭＡＥＡＲＴＨＱＵＡＫＥＭｓ７．６￥ＧｕｏＷａｎｗｕ；...  相似文献   

多层电流片中双撕裂模耦合的压强效应          下载免费PDF全文

王传兵  王水 《地球物理学报》2001,44(2):145-153

应用边界层理论研究了等离子体压强对多层电流片中m≥2的双撕裂模耦合的线性和非线性发展行为的影响.考虑等离子体的压强效应，在一阶近似下，解析求得了环位形中双撕裂模的外区匹配参数Δ′.结果表明，当等离子体β<<1时，等离子体压强对双撕裂模的两有理面模之间通过撕裂模外区发生耦合作用的线性行为没有定性影响.虽然等离子体压强将影响双撕裂模耦合的非线性行为，但是主要表现在对其单模项的影响，而对由于两有理面模之间的耦合作用产生的耦合项的影响却很小.  相似文献   

Spatial distribution of upstream magnetospheric ≥50 keV ions     

G. C. Anagnostopoulos  G. Argyropoulos  G. Kaliabetsos 《Annales Geophysicae》1999,18(1):42-46

We present for the first time a statistical study of 50 keV ion events of a magnetospheric origin upstream from Earths bow shock. The statistical analysis of the 50–220 keV ion events observed by the IMP-8 spacecraft shows: (1) a dawn-dusk asymmetry in ion distributions, with most events and lower intensities upstream from the quasi-parallel pre-dawn side (4 LT-6 LT) of the bow shock, (2) highest ion fluxes upstream from the nose/dusk side of the bow shock under an almost radial interplanetary magnetic field (IMF) configuration, and (3) a positive correlation of the ion intensities with the solar wind speed and the index of geomagnetic index Kp, with an average solar wind speed as high as 620 km s^–1 and values of the index Kp 2. The statistical results are consistent with (1) preferential leakage of 50 keV magnetospheric ions from the dusk magnetopause, (2) nearly scatter free motion of 50 keV ions within the magnetosheath, and (3) final escape of magnetospheric ions from the quasi-parallel dawn side of the bow shock. An additional statistical analysis of higher energy (290–500 keV) upstream ion events also shows a dawn-dusk asymmetry in the occurrence frequency of these events, with the occurrence frequency ranging between 16%-34% in the upstream region.  相似文献   

The hydrogen emission spectrum of a shock wave in a stellar atmosphere     

Yu. A. Fadeyev 《Astronomy Letters》2003,29(11):775-782

Based on a self-consistent solution of the equations of gas dynamics, kinetics of hydrogen atomic level populations, and radiative transfer, we analyze the structure of a shock wave that propagates in a partially ionized hydrogen gas. We consider the radiative transfer at the frequencies of spectral lines by taking into account the effects of a moving medium in the observer's frame of reference. The flux in Balmer lines is shown to be formed behind the shock discontinuity at the initial hydrogen recombination stage. The Doppler shift of the emission-line profile is approximately one and a half times smaller than the gas flow velocity in the Balmer emission region, because the radiation field of the shock wave is anisotropic. At Mach numbers M₁?10 and unperturbed gas densities σ₁=10^?10 g cm^?3, the Doppler shift is approximately one third of the shock velocity U₁. The FWHM of the emission-line profile δ _? is related to the shock velocity by δ _? ≈ k _? U₁, where k _? = 1, 0.6, and 0.65 for the Hα, Hβ, and Hγ lines, respectively.  相似文献   

The Earth's quasi-parallel bow shock: Review of observations and perspectives for Cluster     

William P. Wilkinson 《Planetary and Space Science》2003,51(11):629-647

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Tangential discontinuities as diagnostics for disordered (e.g. quasi-parallel) shocks     

B.A. Hausman 《Planetary and Space Science》2003,51(11):703-712

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用小波包识别地震和矿震   总被引：6，自引：0，他引：6  

和雪松  李世愚  沈萍  冯全雄 《中国地震》2006,22(4):425-434

在能检测到天然地震和矿震的区域，这两类地震的快速识别无论对于区域台网和矿区台网都具有现实意义。这两类震动都是非稳态信号，用传统的Fourier变换不能提取出信号的特征信息，小波包分析方法却能很好提取出信号的特征信息。本文提供了一种基于非参数识别算法，即把信号变换到频域，然后再用奇异值分解作为统计工具，提取出信号的特征信息，作为识别天然地震和矿震的识别因子。以辽宁抚顺2001年1月1日到2003年6月30的18个矿震和16个天然地震，以及北京门头沟2001年1月1日到2002年12月31日的15个矿震和14个天然地震为样本，提取出识别因子。最后，用其它的天然地震和矿震资料检验了识别因子的识别率。  相似文献   

Signatures of interplanetary transients behind shocks and their associated near-surface solar activity     

S. Bravo  X. Blanco-Cano 《Annales Geophysicae》1998,16(4):359-369

Interplanetary transients with particular signatures different from the normal solar wind have been observed behind interplanetary shocks and also without shocks. In this paper we have selected four well-known transient interplanetary signatures, namely: magnetic clouds, helium enhancements and bidirectional electron and ion fluxes, found in the solar wind behind shocks, and undertaken a correlative study between them and the corresponding solar observations. We found that although commonly different signatures appear in a single interplanetary transient event, they are not necessarily simultaneous, that is, they may belong to different plasma regions within the ejecta, which suggests that they may be generated by complex processes involving the ejection of plasma from different solar regions. We also found that more than 90% of these signatures correspond to cases when an H flare and the eruption of a filament occurred near solar central meridian between 1 and 4 days before the observation of the disturbance at 1 AU, the highest association being with flares taking place between 2 and 3 days before. The majority of the H flares were also accompanied by soft X-ray events. We also studied the longitudinal distribution of the associated solar events and found that between 80% and 90% of the interplanetary ejecta were associated with solar events within a longitudinal band of ±30° from the solar central meridian. An east-west asymmetry in the associated solar events seems to exist for some of the signatures. We also look for coronal holes adjacent to the site of the explosive event and find that they were present almost in every case.  相似文献