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Fig. 10.
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Time-distance image of the of the horizontal averages of a) the shear (wave) −Bz(vxBx + vyBy) and b) the flux advection vzBh2 components of the vertical Poynting flux. The horizontal dashed lines represent the photosphere z = 0 and base of the chromosphere ⟨τ500⟩havg = 10−5.
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