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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 11.

Snapshot (at t ≃ 9.5 hr) of the scaled magnetic field magnitude (∣B∣) for (a) Run A and (b) Run B projected onto the meridional plane at ϕ = 0∘. The synthetic spacecraft that cross the meridional plane are represented by yellow spheres. The animated version of this figure shows the evolution of ∣B∣ 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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