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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 6.

Synthetic spacecraft profiles at r = 15 R⊙ for (a) Run A and (b) Run B. Each panel shows magnetic field magnitude as well as components in RTN coordinates for a different combination of θ and ϕ.

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