Upper panels (a)–c)): power of the intensity oscillations measured from Ca ii H a); velocity oscillations at the Ba ii core b); and velocity oscillations in the Ba ii wing c), as a function of the magnetic field inclination in the photosphere. The values of inclination are averaged in time over the five TIP maps. Lower panels (d)–f)): same, but as a function of the photospheric magnetic field strength.
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