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Fig. 4.

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Time evolution of the velocity perturbation along field line 3 ( v ̂ $ \hat{v}_{\parallel} $) in the simulation with a photospheric wave driver, the temperature along field line 3, and the density perturbation ( ρ ̂ $ \hat{\rho} $) along field line 3 calculated using Equation (1). An animated version of this figure is available online.

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