2021
DOI: 10.1051/epjconf/202125402015
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The modes of magnetic field generation in a low-mode model of αΩ-dynamo with α-generator varying intensity regulated by a function with an alternating kernel

Abstract: The low-mode model αΩ-dynamo is used in this paper to simulate the modes of magnetic field generation with insignificant changes in the velocity field of a viscous fluid. In the framework of those model the α-effect intensity is regulated by the process that is included in the magnetohydrodynamic system (MHD-system) as an additive correction as a functional Z(t) depended on the magnetic field energy. Function that determines damped oscillations with variable damping frequency and constant damping coefficient, … Show more

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Cited by 5 publications
(6 citation statements)
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“…This article generalizes research in one of the directions of the cycle of papers of the IKIR FEB RAS on the study of a low-mode model of Earth's dynamo [1][2][3][4][5][6][7][8]. Despite the progress made in geomagnetism theory, the problem of the origin of the Earth's magnetic field and that of space objects has not been fully resolved.…”
Section: Introductionmentioning
confidence: 92%
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“…This article generalizes research in one of the directions of the cycle of papers of the IKIR FEB RAS on the study of a low-mode model of Earth's dynamo [1][2][3][4][5][6][7][8]. Despite the progress made in geomagnetism theory, the problem of the origin of the Earth's magnetic field and that of space objects has not been fully resolved.…”
Section: Introductionmentioning
confidence: 92%
“…Therefore, the scalar parametrization can be given by a function α(r, θ) = α 0 a(r) cos θ = α 0 α(r, θ), where the coefficient α 0 is positive and determines the highest intensity of the α-effect, α(r, θ) is a dimensionless quantity that satisfies the condition max|α(r, θ)| = 1 and the radial component a(r) = r. In accordance with the considered dynamo model, it is assumed that the action of the Archimedean (buoyancy) force with a mass density f out determines the differential rotation of the averaged flow v [14,15,21]. Thus, the MHD-equations, including the equations of the Navier-Stokes and the magnetic field induction B, taking into account the turbulent α-effect, the continuity condition of the velocity field v, the solenoidality condition of the magnetic field B and boundary conditions of adhesion, take the form [8]:…”
Section: Statement Of a Problemmentioning
confidence: 99%
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