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Effects of Dynamo-generated Large-scale Magnetic Fields on the Surface Gravity (f) Mode

  • Authors: Rajesh Mondal, Nishant K. Singh

Rajesh Mondal and Nishant K. Singh 2026 The Astrophysical Journal Letters 1004 .

  • Provider: AAS Journals

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 .

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