A comparative study of solar flux emergence and eruptivity in simulations of horizontal versus toroidal magnetic fields
Context. Magnetic flux emergence is a fundamental driver of eruptive activity in the solar atmosphere. While many numerical studies employed idealized horizontal flux tubes, toroidal tubes provide a more realistic geometry for finite emerging loops with anchored footpoints. Aims. We compare the evol...
Spremljeno u:
| Glavni autori: | , , , |
|---|---|
| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
EDP Sciences
2026-07-01
|
| Serija: | Astronomy & Astrophysics |
| Teme: | |
| Online pristup: | https://www.aanda.org/articles/aa/full_html/2026/07/aa60572-26/aa60572-26.html |
| Oznake: |
Bez oznaka, Budi prvi tko označuje ovaj zapis!
|