Successfully Reproducing Solar Orbiter Polar Field Observations with a Surface Flux Transport Model

arXiv:2609.32194 · astro-ph.SR · Submitted 2026-09-26 · Read on arXiv

astro-ph.SR

Submitted: 2026-09-26

Updated: 2026-09-26

Terminology

• Active Regions — 2× in this paper · explained in 1 episode
• Accuracy — 1× in this paper · explained in 1 episode

Sources

• Surface flux transport modeling for solar cycles 15--21: effects of cycle-dependent tilt angles of sunspot groups
• A coupled 2$\times$2D Babcock-Leighton solar dynamo model. I. Surface magnetic flux evolution

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