Macroscopic control parameter for avalanche models for bursty transport

被引:10
作者
Chapman, S. C. [1 ,3 ]
Rowlands, G. [1 ]
Watkins, N. W. [2 ,3 ]
机构
[1] Univ Warwick, Ctr Fus Space & Astrophys, Coventry CV4 7AL, W Midlands, England
[2] British Antarctic Survey, Div Phys Sci, Cambridge CB3 0ET, England
[3] Kavli Inst Theoret Phys, Santa Barbara, CA 93106 USA
基金
英国工程与自然科学研究理事会;
关键词
plasma transport processes; plasma turbulence; self-organised criticality; SELF-ORGANIZED CRITICALITY; SOLAR-FLARES; DYNAMIC MAGNETOSPHERE; TURBULENT TRANSPORT; TIME CORRELATIONS; CONFINED PLASMA; EDGE TURBULENCE; SANDPILE MODEL; ENERGY-RELEASE; SYSTEMS;
D O I
10.1063/1.3057392
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
Similarity analysis is used to identify the control parameter R(A) for the subset of avalanching systems that can exhibit self-organized criticality (SOC). This parameter expresses the ratio of driving to dissipation. The transition to SOC, when the number of excited degrees of freedom is maximal, is found to occur when R(A)-> 0. This is in the opposite sense to (Kolmogorov) turbulence, thus identifying a deep distinction between turbulence and SOC and suggesting an observable property that could distinguish them. A corollary of this similarity analysis is that SOC phenomenology, that is, power law scaling of avalanches, can persist for finite R(A) with the same R(A)-> 0 exponent if the system supports a sufficiently large range of lengthscales, necessary for SOC to be a candidate for physical (R(A) finite) systems.
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页数:7
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