Table 3: Top: continuum contrasts, $C_{\rm cont}$ , derived from synthetic spectra, with respect to the FAL C-model atmosphere. The listed values from observation refer to the average (maximum) over all observed bright point interiors with respect to the spectrum of the reference region. Bottom: filling factors derived from Eqs. (3) and (4).
Observation FAL F FAL P Net

$C_{\rm cont}$ (430.31 nm) -0.04 (0.14) 0.00 0.09 0.77

$C_{\rm cont}$ (569.20 nm) 0.02 (0.13) 0.00 0.18 -

$C_{\rm cont}$ (526.46 nm) -0.01 (0.13) 0.03 0.25 -

**Table 3:** *Top*: continuum contrasts, $C_{\rm cont}$ , derived from synthetic spectra, with respect to the `FAL C`-model atmosphere. The listed values from observation refer to the average (maximum) over all observed bright point interiors with respect to the spectrum of the reference region. *Bottom*: filling factors derived from Eqs. (3) and (4).
	Observation	`FAL F`	`FAL P`	`Net`
$C_{\rm cont}$ (430.31 nm)	-0.04 (0.14)	0.00	0.09	0.77
$C_{\rm cont}$ (569.20 nm)	0.02 (0.13)	0.00	0.18	-
$C_{\rm cont}$ (526.46 nm)	-0.01 (0.13)	0.03	0.25	-

Filling factors based on... FAL P Net

.. G-band intensity contrast 0.35 (0.91) 0.08 (0.20)

.. Bright Point Index 0.55 (1.01) 0.18 (0.32)

Source LaTeX | All tables | In the text

Filling factors based on...	`FAL P`	`Net`
.. G-band intensity contrast	0.35 (0.91)	0.08 (0.20)
.. Bright Point Index	0.55 (1.01)	0.18 (0.32)