2015
DOI: 10.5194/npg-22-361-2015
|View full text |Cite
|
Sign up to set email alerts
|

Reversals in the large-scale αΩ-dynamo with memory

Abstract: Abstract. Inversion of the magnetic field in a model of largescale α -dynamo with α-effect with stochastic memory is under investigation. The model allows us to reproduce the main features of the geomagnetic field reversals. It was established that the polarity intervals in the model are distributed according to the power law. Model magnetic polarity timescale is fractal. Its dimension is consistent with the dimension of the real geomagnetic polarity timescale.

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
2

Citation Types

1
6
0

Year Published

2016
2016
2024
2024

Publication Types

Select...
4
2

Relationship

1
5

Authors

Journals

citations
Cited by 11 publications
(9 citation statements)
references
References 31 publications
1
6
0
Order By: Relevance
“…The slow amplitudes of such magnetic-temperature oscillations will obey the Lorentz-like dynamical system if we exclude fast changes by averaging over high frequency oscillations. Another way to obtian the equations for a low-mode dynamo is the Galerkin's method [26][27][28][29]. But this method has a harmonic number selection problem that cannot be solved without a general relaxation approach.…”
Section: Three Regimes Of Convection and Oscillationsmentioning
confidence: 99%
See 2 more Smart Citations
“…The slow amplitudes of such magnetic-temperature oscillations will obey the Lorentz-like dynamical system if we exclude fast changes by averaging over high frequency oscillations. Another way to obtian the equations for a low-mode dynamo is the Galerkin's method [26][27][28][29]. But this method has a harmonic number selection problem that cannot be solved without a general relaxation approach.…”
Section: Three Regimes Of Convection and Oscillationsmentioning
confidence: 99%
“…Only in this case, the kinematic approximation for dynamo problem may be used. This is not applicable for solar activity but may be used for planetary dynamo [26][27][28][29].…”
Section: Three Regimes Of Convection and Oscillationsmentioning
confidence: 99%
See 1 more Smart Citation
“…The consideration of memory in low-mode dynamo models can affect essentially the dynamic regimes. For instance, the introduction of memory into Rickitake two-disc dynamo leads to the emergence of hyperchaotic oscillations [17]; non-Markovian fluctuations of α-effect intensity lead to power distributions of polarity intervals and realistic fractal dimension of polarity scales [18].…”
Section: Introductionmentioning
confidence: 99%
“…In addition, the full equations contain a lot of parameters, which estimations differ by several orders, or unknow. Therefore, using simple low-dimensional dynamical systems are trying to explain the physical cause, features, the most important properties of this phenomenon, for example [4][5][6][7][8].…”
Section: Introductionmentioning
confidence: 99%