High-Resolution Modelling of Coronae and Winds in Solar-type Stars with Varying Rotation Rates II. Stellar Winds

arXiv:2609.28067 · astro-ph.SR · Submitted 2026-09-23 · Read on arXiv

astro-ph.SR

Submitted: 2026-09-23

Updated: 2026-09-23

Terminology

• Calibration — 6× in this paper · explained in 7 episodes
• Angular Momentum Loss — 4× in this paper · explained in 1 episode
• Scaling Laws — 3× in this paper · explained in 4 episodes
• Trace — 3× in this paper · explained in 2 episodes
• Alignment — 2× in this paper · explained in 1 episode
• Active Regions — 1× in this paper · explained in 1 episode
• Benchmarking — 1× in this paper · explained in 3 episodes
• Degeneracy — 1× in this paper · explained in 3 episodes
• Inner Heliosphere — 1× in this paper
• Parker Solar Probe — 1× in this paper
• Robustness — 1× in this paper · explained in 5 episodes
• Solar Corona — 1× in this paper

Sources

• Atmospheric Escape Rates from Mars - If it Orbited an Old M-Dwarf Star

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