The solar fast dynamo action extended to A, Ap and Am type stars
D. V. Sarafopoulos

TL;DR
This paper proposes an extended fast dynamo mechanism explaining magnetic field generation in the Sun and A, Ap, Am stars through charge separation and Torus structures, linking stellar rotation and plasma properties to magnetic activity cycles.
Contribution
It introduces a novel dynamo model involving charge separation and Torus structures, extending the fast dynamo concept to A, Ap, and Am stars.
Findings
Magnetic fields in these stars are due to large-scale charge separation.
Torus structures determine the stellar activity cycle durations.
Differential rotation and plasma speed are key to magnetic field generation.
Abstract
Initially, we present our original fast dynamo mechanism being potentially at work concerning the Sun and the solar type stars. Then, based on this new prototype model, a dynamo action model explaining the generation of the magnetic fields for A, Ap and Am type stars will be derived. We argue that their magnetic behavior is essentially due to locally exotic plasma properties leading to large scale charge separation in their interior. Their powerful magnetic fields are generated by the revolution speed of these excess positive or negative charges tightly associated with the formation of one or two so called Torus structures. The lifespan of the Torus charge defines the stellar activity cycle. In the solar case, two Torus structures are formed preserving their charge for 11 years. The Torus charging results from two processes: First, the stellar differential rotation with its shear layers…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Astro and Planetary Science · Stellar, planetary, and galactic studies
