Fig. 5: Single-point FFT spectrum obtained from the Gmunu simulation of T1K6 model under \({{{{{\mathcal{l}}}}}}\) = 0 perturbation.
From: Oscillations of highly magnetized non-rotating neutron stars

The FFT data are computed from the time evolution of the r-component of three velocity fields at the spatial point (r, θ) ≃ (re/2, π/2). The parabolic interpolations of the prominent peaks are shown as an example. The FFT spectrum at a single spatial point usually shows peaks that are sharp enough for analysis.