Two-Mode Hereditary Model of Solar Dynamo

Two-Mode Hereditary Model of Solar Dynamo

The magnetic field of the Sun is formed by the mechanism of hydromagnetic dynamo. In this mechanism, the flow of the conducting medium (plasma) of the convective zone generates a magnetic field, and this field corrects the flow using the Lorentz force, creating feedback. An important role in dynamo...

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Bibliographic Details
Main Authors:	Evgeny Kazakov, Gleb Vodinchar, Dmitrii Tverdyi
Format:	Article
Language:	English
Published:	MDPI AG 2025-05-01
Series:	Mathematics
Subjects:	nonlinear dynamical system solar dynamo magnetohydrodynamics turbulence feedback memory
Online Access:	https://www.mdpi.com/2227-7390/13/10/1669
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