Image Details
Caption: Figure 5.
Left: normalized vertical magnetic field Bz/Beq at the end of the kin interval (top) and at the beginning of the sat interval (bottom), as defined in the text. Right: variation of different f-mode characteristics with ﹩{\tilde{k}}_{x}﹩ for different runs. (a) Mode strength (μf), (b) relative frequency shift, and (c) full width at half-maximum (FWHM) of the f-mode, all as functions of ﹩{\tilde{k}}_{x}﹩. Tick marks at the top indicate the corresponding spherical harmonic degree ℓ.
© 2026. The Author(s). Published by the American Astronomical Society.