Small-scale magnetic flux emergence in the quiet Sun

TL;DR

This study uses advanced 3D MHD simulations to investigate small magnetic flux emergence in the quiet Sun, revealing the formation of magnetic loops and sheets within granules, consistent with recent observations.

Contribution

It provides the first detailed simulation-based analysis of small-scale magnetic flux emergence and sheet formation in the quiet Sun's convection zone.

Findings

Magnetic loops emerge within granules from near-surface layers.

Organized horizontal magnetic sheets form covering entire granules.

Simulation results match recent observational findings.

Abstract

Small bipolar magnetic features are observed to appear in the interior of individual granules in the quiet Sun, signaling the emergence of tiny magnetic loops from the solar interior. We study the origin of those features as part of the magnetoconvection process in the top layers of the convection zone. Two quiet-Sun magnetoconvection models, calculated with the radiation-magnetohydrodynamic (MHD) Bifrost code and with domain stretching from the top layers of the convection zone to the corona, are analyzed. Using 3D visualization as well as a posteriori spectral synthesis of Stokes parameters, we detect the repeated emergence of small magnetic elements in the interior of granules, as in the observations. Additionally, we identify the formation of organized horizontal magnetic sheets covering whole granules. Our approach is twofold, calculating statistical properties of the system, like joint probability density functions (JPDFs), and pursuing individual events via visualization tools. We conclude that the small magnetic loops surfacing within individual granules in the observations may originate from sites at or near the downflows in the granular and mesogranular levels, probably in the first 1 or 1.5 Mm below the surface. We also document the creation of granule-covering magnetic sheet-like structures through the sideways expansion of a small subphotospheric magnetic concentration picked up, and pulled out of the interior, by a nascent granule. The sheet-like structures we found in the models may match the recent observations of Centeno et al. (2017).