Photospheric plasma and magnetic field dynamics during the formation of solar AR 11190
Photospheric plasma and magnetic field dynamics during the formation of solar AR 11190
The Sun features on its surface typical flow patterns called the granulation, mesogranulation, and supergranulation. These patterns arise due to convective flows transporting energy from the interior of the Sun to its surface. In this paper we will shed light on the interaction between the convective flows in large-scale cells …