A comparative study of solar flux emergence and eruptivity in simulations of horizontal versus toroidal magnetic fields

arXiv:2606.19029 · astro-ph.SR · Submitted 2026-06-17 · Read on arXiv

Vaggelis Karantanis, Juxhin Zhuleku, Vasilis Archontis, Kostas Moraitis

astro-ph.SR

Submitted: 2026-06-17

Journal ref: A&A, 711, A69 (2026)

DOI: 10.1051/0004-6361/202660572

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Active Regions — 5× in this paper · explained in 1 episode
• APEX — 4× in this paper · explained in 1 episode
• Core — 1× in this paper · explained in 2 episodes
• Magnetohydrodynamics (MHD) — 1× in this paper · explained in 3 episodes
• Model Drift — 1× in this paper · explained in 4 episodes

Related papers

• HXI-DLA2: A Physics-Constrained Deep Learning Algorithm for the ASO-S Hard X-ray Imager
• Effect of Neutron Star Jets on Common Envelope Evolution
• Ongoing and Post-Mass-Transfer Binaries: A Living Catalog and Unified Review of Binary Mass Transfer Products
• Finite-Element Asteroseismology I: Two-Dimensional Adiabatic Oscillations of Rapidly Rotating N=3 Polytropes
• Constraining the origin of magnetic white dwarfs
• EPRV Asteroseismology of the K dwarfs GJ 570 A and GJ 783 A with ESPRESSO. Empirical mode-amplitude scaling in tension with 3D convection simulations