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On the 3D Magnetic Structure of Coronal Mass Ejections through the Solar Corona

  • Authors: Erika Palmerio, Michal Ben-Nun, Tibor Török, Cooper Downs, Viacheslav S. Titov

Erika Palmerio et al 2026 The Astrophysical Journal Supplement Series 286 .

  • Provider: AAS Journals

Caption: Figure 8.

Snapshot (at t ≃ 9.5 hr) of the scaled radial magnetic field component (BR) for (a) Run A and (b) Run B projected onto the equatorial plane as seen from above the solar north pole. The synthetic spacecraft that cross the equatorial plane are represented by yellow spheres. The animated version of this figure shows the evolution of BR throughout the temporal domain of the simulations from 0 to 20 hr, corresponding to code units from 200.0 to 250.0 in increments of 0.5 (12 minutes). The animation has a total real-time duration of 7 s.

(An animation of this figure is available in the online article.)

(An animation of this figure is available.)

The video/animation of this figure is available in the online journal.

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