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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 5.

Synthetic spacecraft profiles for fixed (r, ϕ) = (10 R⊙, 0∘) at five latitudes (20∘, 10∘, 0∘, −10∘, −20∘) for (a) Run A and (b) Run B. The magnetic field magnitudes for each profile are shown to the left, while the corresponding magnetic field components in RTN coordinates are shown to the right. CME-driven sheaths are marked by vertical lines, while CME flux rope intervals are indicated by shaded areas.

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