Image Details
 
                    Caption: Figure 1.
Schematic illustration (not to scale) of symmetric (upper panel) and antisymmetric (lower panel) perturbation modes. Note that the symmetries are indicated in terms of field line geometries (which should refer to ∫d ζ δ b), not the values of δ b (Section 2.2).
© 2024. The Author(s). Published by the American Astronomical Society.