2017/01/13 by I. Ermolli, A. Cristaldi, F. Giorgi +6
Biochemistry, Genetics and Molecular Biology · Physics and Astronomy · #Astrophysics #Computational physics #Flux (metallurgy) #Flux tube #Geology #Geomagnetism and Paleomagnetism Studies #Ibis #Ionosphere and magnetosphere dynamics #Magnetic field #Magnetic flux #Materials science #Mechanics #Nuclear physics #Physics #Plasma #Solar and Space Plasma Dynamics #astro-ph.SR
paper · pdf · doi:10.1051/0004-6361/201526144
Accepted for publication in Astronomy and Astrophysics
openalex publication_date 2017/01/13 · arxiv created 2017/01/23 · arxiv updated 2017/01/24 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Aims. Recent simulations of solar magneto-convection have offered new levels of understanding of the interplay between plasma motions and magnetic fields in evolving active regions. We aim at verifying some aspects of the formation of magnetic regions derived from recent numerical studies in observational data.