Stochastic resonance in geomagnetic polarity reversals

被引:22
作者
Consolini, G [1 ]
De Michelis, P
机构
[1] CNR, Ist Fis Spazio Interplanetario, I-00133 Rome, Italy
[2] Ist Nazl Geofis & Vulcanol, I-00143 Rome, Italy
关键词
D O I
10.1103/PhysRevLett.90.058501
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Among noise-induced cooperative phenomena a peculiar relevance is played by stochastic resonance. In this paper we offer evidence that geomagnetic polarity reversals may be due to a stochastic resonance process. In detail, analyzing the distribution function P(tau) of polarity residence times (chrons), we found the evidence of a stochastic synchronization process, i.e., a series of peaks in the P(tau) at T(n)similar or equal to(2n+1)T-Omega/2 with n=0,1,...,j and T(Omega)similar to0.1 Myr. This result is discussed in connection with both the typical time scale of Earth's orbit eccentricity variation and the recent results on the typical time scale of climatic long-term variation.
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页数:4
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