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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 10.

Snapshot (at t ≃ 9.5 hr) of the magnetic field lines connected to the 20 synthetic spacecraft located at ϕ = 0∘ for (a) Run A and (b) Run B projected onto (top) the meridional plane and (bottom) the equatorial plane. The synthetic spacecraft that cross the meridional plane are represented by yellow spheres. The field lines are colored by the (scaled) magnitude and sign of the BT component. The animated version of this figure shows the evolution of these 20 field lines 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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