Magnetic flux cancellation in a 3D magnetohydrodynamic simulation of an emerging flux tube with a non-uniform twist

arXiv:2610.11983 · astro-ph.SR · Submitted 2026-10-08 · Read on arXiv

astro-ph.SR

Submitted: 2026-10-08

Updated: 2026-10-08

Terminology

• Core — 11× in this paper · explained in 2 episodes
• Active Regions — 4× in this paper · explained in 1 episode
• Helioseismic and Magnetic Imager — 1× in this paper
• Interface Region Imaging Spectrograph — 1× in this paper
• Magnetohydrodynamics (MHD) — 1× in this paper · explained in 3 episodes
• Michelson Doppler Imager — 1× in this paper
• Solar Dynamics Observatory — 1× in this paper
• Trace — 1× in this paper · explained in 2 episodes

Sources

• Magnetic Fields and Velocity Structures around a Cancellation Site
• Magnetic flux cancellation in the solar atmosphere through 3D realistic numerical modeling
• Observations of the formation of a proto-spot in a pre-existing field environment

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