A First Global Full-Vector Coronal Magnetic Field Inference Using MLSO CoMP and UCoMP Observations

arXiv:2609.35100 · astro-ph.SR · Submitted 2026-09-28 · Read on arXiv

astro-ph.SR

Submitted: 2026-09-28

Updated: 2026-09-28

Code: https://github.com/arparaschiv/solar-coronal-inversion

Terminology

• Alignment — 4× in this paper · explained in 1 episode
• Aperture — 3× in this paper · explained in 1 episode
• Mauna Loa Solar Observatory — 3× in this paper
• Core — 2× in this paper · explained in 2 episodes
• Fidelity — 2× in this paper · explained in 2 episodes
• Accuracy — 1× in this paper · explained in 1 episode
• Active Regions — 1× in this paper · explained in 1 episode
• Consistency — 1× in this paper · explained in 3 episodes
• Iterated Conditional Modes — 1× in this paper
• Local Optimization — 1× in this paper · explained in 2 episodes
• National Science Foundation — 1× in this paper
• Physical Constraints — 1× in this paper · explained in 7 episodes

Sources

• Untangling the global coronal magnetic field with multiwavelength observations
• NASA/NOAA MOU Annex Final Report: Evaluating Model Advancements for Predicting CME Arrival Time

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