Probing the magnetic field of a coronal mass ejection with PSR J1022+1001

arXiv:2603.18051 · astro-ph.SR, astro-ph.HE, astro-ph.IM · Submitted 2026-03-17 · Read on arXiv

astro-ph.SR, astro-ph.HE, astro-ph.IM

Submitted: 2026-03-17

Updated: 2026-09-01

Comments: Submitted to A&A on the 17 of march 2026

Code: https://github.com/louisbondonneau/NenuPlot

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

Terminology

• Core — 5× in this paper · explained in 2 episodes
• Forward modeling — 3× in this paper · explained in 2 episodes
• Consistency — 2× in this paper · explained in 3 episodes
• APEX — 1× in this paper · explained in 1 episode
• Alignment — 1× in this paper · explained in 1 episode
• Calibration — 1× in this paper · explained in 7 episodes
• Community Coordinated Modeling Center — 1× in this paper
• Graduated Cylindrical Shell — 1× in this paper

Sources

• Real-time prediction of two geomagnetic storms using Solar Orbiter as a far upstream solar wind monitor
• The SOHO LASCO CME Catalog -- Version 2
• First observations of a geomagnetic superstorm with a sub-L1 monitor

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