Domino model for geomagnetic field reversals

被引:11
|
作者
Mori, N. [1 ]
Schmitt, D. [2 ]
Wicht, J. [2 ]
Ferriz-Mas, A. [3 ,4 ]
Mouri, H. [5 ]
Nakamichi, A. [6 ]
Morikawa, M. [1 ]
机构
[1] Ochanomizu Univ, Dept Phys, Tokyo 1128610, Japan
[2] Max Planck Inst Sonnensyst Forsch, D-37191 Katlenburg Lindau, Germany
[3] Univ Vigo, Dept Fis Aplicada, Orense 32004, Spain
[4] CSIC, IAA, E-18080 Granada, Spain
[5] Meteorol Res Inst, Tsukuba, Ibaraki 3050052, Japan
[6] Kyoto Sangyo Univ, Koyama Astron Observ, Kyoto 6038555, Japan
来源
PHYSICAL REVIEW E | 2013年 / 87卷 / 01期
关键词
POLARITY REVERSALS; MAGNETIC-FIELD; DISK DYNAMO; GEODYNAMO; SIMULATION; GENERATION; MANTLE;
D O I
10.1103/PhysRevE.87.012108
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
We solve the equations of motion of a one-dimensional planar Heisenberg (or Vaks-Larkin) model consisting of a system of interacting macrospins aligned along a ring. Each spin has unit length and is described by its angle with respect to the rotational axis. The orientation of the spins can vary in time due to spin-spin interaction and random forcing. We statistically describe the behavior of the sum of all spins for different parameters. The term "domino model" in the title refers to the interaction among the spins. We compare the model results with geomagnetic field reversals and dynamo simulations and find strikingly similar behavior. The aggregate of all spins keeps the same direction for a long time and, once in a while, begins flipping to change the orientation by almost 180 degrees (mimicking a geomagnetic reversal) or to move back to the original direction (mimicking an excursion). Most of the time the spins are aligned or antialigned and deviate only slightly with respect to the rotational axis (mimicking the secular variation of the geomagnetic pole with respect to the geographic pole). Reversals are fast compared to the times in between and they occur at random times, both in the model and in the case of the Earth's magnetic field. DOI: 10.1103/PhysRevE.87.012108
引用
收藏
页数:11
相关论文
共 50 条
  • [21] A statistical analysis of polarity reversals of the geomagnetic field
    Sorriso-Valvo, Luca
    Stefani, Frank
    Carbone, Vincenzo
    Nigro, Giuseppina
    Lepreti, Fabio
    Vecchio, Antonio
    Veltri, Pierluigi
    PHYSICS OF THE EARTH AND PLANETARY INTERIORS, 2007, 164 (3-4) : 197 - 207
  • [23] STATE OF GEOMAGNETIC-FIELD AND ITS REVERSALS
    LEVY, EH
    ASTROPHYSICAL JOURNAL, 1972, 175 (02): : 573 - &
  • [24] NULLITY PHASE OF GEOMAGNETIC-FIELD REVERSALS
    MCDONALD, KL
    BULLETIN OF THE AMERICAN PHYSICAL SOCIETY, 1978, 23 (08): : 1011 - 1011
  • [25] PALEOMAGNETIC OBSERVATIONS OF GEOMAGNETIC-FIELD REVERSALS
    DODSON, RE
    DUNN, JR
    FULLER, M
    SCHMIDT, VA
    ITO, H
    TOKIEDA, K
    TRANSACTIONS-AMERICAN GEOPHYSICAL UNION, 1973, 54 (04): : 253 - 253
  • [26] DISTINCTIVE FIELD BEHAVIOR FOLLOWING GEOMAGNETIC REVERSALS
    BOGUE, SW
    PAUL, HA
    GEOPHYSICAL RESEARCH LETTERS, 1993, 20 (21) : 2399 - 2402
  • [27] ATMOSPHERIC HELIUM AND GEOMAGNETIC-FIELD REVERSALS
    SHELDON, WR
    KERN, JW
    JOURNAL OF GEOPHYSICAL RESEARCH, 1972, 77 (31): : 6194 - &
  • [28] FREQUENCY OF GEOMAGNETIC REVERSALS AND SYMMETRY OF NONDIPOLE FIELD
    COX, A
    REVIEWS OF GEOPHYSICS, 1975, 13 (03) : 35 - 51
  • [29] Behaviour of the Geomagnetic Field during Reversals and Excursions
    Reshetnyak, M. Yu.
    MOSCOW UNIVERSITY PHYSICS BULLETIN, 2024, 79 (01) : 107 - 112
  • [30] Behaviour of the Geomagnetic Field during Reversals and Excursions
    M. Yu. Reshetnyak
    Moscow University Physics Bulletin, 2024, 79 : 107 - 112