A non-extensive statistical physics approach to the polarity reversals of the geomagnetic field

被引:47
|
作者
Vallianatos, Filippos [1 ,2 ]
机构
[1] Technol Educ Inst Crete, Lab Geophys & Seismol, Iraklion, Greece
[2] UCL, Dept Earth Sci, London WC1E 6BT, England
关键词
Non-extensive statistical physics; Polarity reversals; Geomagnetic field; CORE; SUPERSTATISTICS; DRIVEN;
D O I
10.1016/j.physa.2010.12.040
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Using the CK95 database of Cande and Kent (1995) 171, we apply the concepts of non-extensive statistical physics (NESP) to the time intervals between two consecutive geomagnetic reversals, called inter-reversal times. The application of NESM is appropriate to systems such as the geomagnetic field where non-linearity, long-range interactions, memory effects and scaling are important. We calculate the probability density function for the inter-reversal times and using the CK95 geomagnetic reversals and we estimate a thermodynamic q parameter of q = 1.5, which supports the conclusion that the geomagnetic system is a sub-extensive one with long-range memory effects. The results discussed using the complementary to the NESP approach of superstatistics which is based on a superposition of ordinary local equilibrium statistical mechanics, using a suitable intensive parameter beta that fluctuates on a relatively large temporal scale, leading to the conclusion that two degrees of freedom describe the process which generates the geomagnetic reversals. (C) 2011 Elsevier B.V. All rights reserved.
引用
收藏
页码:1773 / 1778
页数:6
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