Multi-height probing of horizontal flows in the solar photosphere

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Table 2.

Pearson’s correlation coefficients between simulated velocities and FLCT velocities at the mid-photosphere and temperature minimum.

	FWHM [km]	log τ₅₀₀ = −1		log τ₅₀₀ = −2		log τ₅₀₀ = −3		log τ₅₀₀ = −4
	FWHM [km]	r_{v_x}	r_{v_y}	r_{v_x}	r_{v_y}	r_{v_x}	r_{v_y}	r_{v_x}	r_{v_y}
T	600	0.72	0.73	0.38	0.41	−0.05	−0.06	0.03	0.04
T	300	0.64	0.65	0.33	0.35	0.05	0.05	0.11	0.12

B_z	600	0.90	0.90	0.87	0.88	0.86	0.85	0.87	0.88
	300	0.91	0.91	0.90	0.90	0.86	0.85	0.85	0.86

Notes. Here, FLCT velocities are recovered from either temperature or B_z, at log τ₅₀₀ = { − 1, −2, −3, −4}. Correlations are shown only for filtered simulation velocities.

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