Kinematic Dynamo Modeling and Its Peculiarities in Polar Latitudes

N. A. Shatalov; Шаталов Н. А.; V. M. Chechetkin; Чечеткин В. М.; S. L. Shalimov; Шалимов С. Л.

doi:10.31857/S0002333723020114

Kinematic Dynamo Modeling and Its Peculiarities in Polar Latitudes

Authors: Shatalov N.A.¹, Chechetkin V.M.², Shalimov S.L.³
Affiliations:
1. National Research Nuclear University, Moscow Engineering Physics Institute
2. Keldysh Institute of Applied Mathematics, Russian Academy of Sciences
3. Schmidt Institute of Physics of the Earth, Russian Academy of Sciences
Issue: No 2 (2023)
Pages: 3-14
Section: Articles
URL: https://journal-vniispk.ru/0002-3337/article/view/138995
DOI: https://doi.org/10.31857/S0002333723020114
EDN: https://elibrary.ru/LIUETZ
ID: 138995

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Abstract
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Abstract

The results of calculations of the magnetic field structure in the kinematic approximation are presented, testifying to the consistency of the constructed numerical model with the structure of the flows of a conducting liquid: the instability of the convective process in a rotating spherical shell is reflected in the evolution of the magnetic field, manifesting itself in the pulsation regime of the field. It is shown that the features of the field evolution in the calculations are most clearly pronounced at high latitudes and have analogs in the behavior of the real geomagnetic field.

Keywords

kinematic dynamo, geomagnetic field, numerical model

References

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