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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 7.

Fits with the expansion-modified force-free cylinder flux rope model applied to representative in situ profiles for (a) Run A and (b) Run B. Simulated data are shown in black, single-rope fits considering a positive helicity sign are shown in magenta, two-rope fits performed for the (θ, ϕ) = (0∘, −20∘) profiles are shown green, and single-rope fits assuming a negative helicity sign performed for the (θ, ϕ) = (−20∘, −20∘) profiles are shown in blue.

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