Small-scale Magnetic Flux Emergence in the Quiet Sun
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
Moreno-Insertis, F. et al.
Fecha de publicación:
6
2018