Image Details
Caption: Figure 8.
(Top) Same as Figure 6, but for WASP-6 using the MURaM magnetic models: with small-scale turbulent dynamo (SSD) baseline model (blue) and B-fields of 100 G, 200 G, and 300 G (orange, greed, purple respectively) shown. The change in LD parameters ℓ (middle) and δ (bottom) between the nonmagnetic model and model with B-fields is also shown.
© 2026. The Author(s). Published by the American Astronomical Society.