Helicity--vorticity turbulent pumping of magnetic fields in the solar dynamo
V.V. Pipin
TL;DR
This paper investigates how helical turbulence and differential rotation in the solar convection zone cause turbulent pumping of magnetic fields, influencing the solar dynamo process.
Contribution
It introduces a detailed discussion of the turbulent pumping mechanism and its role in the solar dynamo, highlighting the impact of helicity and vorticity.
Findings
Turbulent pumping significantly affects magnetic field distribution in the solar convection zone.
Helicity and vorticity play crucial roles in magnetic field transport.
The mechanism impacts the solar magnetic cycle dynamics.
Abstract
The interaction of helical convective motions and differential rotation in the solar convection zone results in turbulent drift of a large-scale magnetic field. We discuss the pumping mechanism and its impact on the solar dynamo.
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