Multi-height probing of horizontal flows in the solar photosphere

Open Access

Fig. 10.

Comparison between velocity divergence calculated using v_o (left panels) at log τ₅₀₀ = −1 and v_f inferred from the Fe I line (right panels). Top: Results with an apodizing window of 600 km. Bottom: Results with an apodizing window of 300 km.

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