Image Details
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.
© 2026. The Author(s). Published by the American Astronomical Society.