Oscillations of the solar photospheric magnetic field caused by the m = 1 high-latitude inertial mode

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Fig. 2.

Oscillations of $⟨ B_{avg}^{+} ⟩$ $\langle B_{\mathrm{avg}}^{+} \rangle$ and $⟨ V_{zonal}^{-} ⟩$ $\langle V_{\mathrm{zonal}}^{-} \rangle$ in the time series from HMI and GONG data in 2019. A 180-day average was removed, and for clarity, the maps were smoothed with a Gaussian kernel with σ = 1 day. Vertical lines are spaced at intervals of 34 days.

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