The quasisteady primordial magnetic field of the sun, and the intensity variations of the solar cycle

Physics

Scientific paper

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Magnetic Flux, Solar Cycles, Solar Magnetic Field, Stellar Evolution, Poloidal Flux, Solar Physics, Stellar Models

Scientific paper

The behavior of the solar activity cycle is analyzed on the basis of
Leighton's model, assuming the presence of a primordial, nondecaying
poloidal magnetic field. The primordial field would significantly
influence the cyclicity, causing relatively intense cycles to alternate
with less intense ones.

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