# Confinement of the solar tachocline by a cyclic dynamo magnetic field

## TL;DR

This study models how a cyclic dynamo magnetic field can confine the solar tachocline by suppressing turbulent spreading, showing that weak turbulence and realistic magnetic fields enable magnetic confinement.

## Contribution

It introduces a simplified 1D model analyzing magnetic confinement of the tachocline, exploring parameter regimes where dynamo fields prevent spreading.

## Key findings

- Magnetic fields can confine the tachocline under weak turbulence conditions.
- Weak turbulence with high ohmic diffusivity allows magnetic suppression of spreading.
- Dynamo magnetic fields can prevent inward burrowing of the tachocline.

## Abstract

The surprising thinness of the solar tachocline is still not understood with certainty today. Among the numerous possible scenarios suggested to explain its radial confinement, one hypothesis is based on Maxwell stresses that are exerted by the cyclic dynamo magnetic field of the Sun penetrating over a skin depth below the turbulent convection zone. Our goal is to assess under which conditions (turbulence level in the tachocline, strength of the dynamo-generated field, spreading mechanism) this scenario can be realized in the solar tachocline. We develop a simplified 1D model of the upper tachocline under the influence of an oscillating magnetic field imposed from above. The turbulent transport is parametrized with enhanced turbulent diffusion (or anti-diffusion) coefficients. Two main processes that thicken the tachocline are considered; either turbulent viscous spreading or radiative spreading. An extensive parameter study is carried out to establish the physical parameter regimes under which magnetic confinement of the tachocline that is due to a surface dynamo field can be realized. We have explored a large range of magnetic field amplitudes, viscosities, ohmic diffusivities and thermal diffusivities. We find that, for large but still realistic magnetic field strengths, the differential rotation can be suppressed in the upper radiative zone (and hence the tachocline confined) if weak turbulence is present (with an enhanced ohmic diffusivity of $\eta > 10^{7-8} \, cm^2/s$), even in the presence of radiative spreading. Our results show that a dynamo magnetic field can, in the presence of weak turbulence, prevent the inward burrowing of a tachocline subject to viscous diffusion or radiative spreading.