Modeling of solar magnetic field using the kinematic-gravitational ion dynamo model

Author:

Kochnev V A

Abstract

Abstract In present article the kinematic-gravitational ion dynamo model accounting for influence of tidal forces on electric currents in ionized substances is applied to modeling of the magnetic field of the Sun. Estimates of currents and field values obtained using a seven-layer model indicate that tidal forces influence is not insignificant. A correlation method for assessment of the Sun’s polarity was created and applied for a detailed analysis of the polarity of magnetic field of the Sun in the 21 and 22 cycles.

Publisher

IOP Publishing

Subject

General Physics and Astronomy

Reference18 articles.

1. How Could a Rotating Body such as the Sun Become a Magnet;Larmor;Reports of the British Association,1919

2. Planetary Magnetic Fields and Fluid Dynamos;Jones;Annu. Rev. Fluid Mech.,2011

3. A model of a tidally synchronized solar dynamo;Stefani;Solar Physics,2019

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