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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 3.

Synthetic spacecraft profiles for fixed (θ, ϕ) = (0∘, 0∘) at four radial distances (5, 10, 15, 20 R⊙) for (a) Run A and (b) Run B. Each plot shows, from top to bottom: magnetic field magnitude, magnetic field components in RTN coordinates, solar wind speed, density, and temperature. CME-driven sheaths are marked by vertical lines, while CME flux rope intervals are indicated by shaded areas. The y-axes are scaled uniformly across each row to highlight differences between the two runs.

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