2 papers
astro-ph.SR2026
A comparative study of solar flux emergence and eruptivity in simulations of horizontal versus toroidal magnetic fields
Vaggelis Karantanis, Juxhin Zhuleku, Vasilis Archontis +1
Context: Magnetic flux emergence is a fundamental driver of eruptive activity in the solar atmosphere. While many numerical studies employed idealized horizontal flux tubes, toroid…
astro-ph.SR2025
Recurrent eruptions from the emergence of a toroidal flux tube
J. Zhuleku, V. Archontis, K. Moraitis
Solar eruptive behavior is often modeled with magnetohydrodynamic simulations of magnetic flux emergence. The usual geometry considered is that of a horizontal cylindrical magnetic…