Probing quiet Sun magnetism using MURaM simulations and Hinode/SP results: support for a local dynamo

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Table 1:

Details of the three Hinode/SP data sets used.
	Date	Time	FOCUS	$\mu$	Size	Exposure	Noise	$\langle B^{\rm T}_{\rm app}\rangle$	$\langle \vert B^{\rm L}_{\rm app}\vert\rangle$	$\langle B^{\rm L}_{\rm app}\rangle$
	[dd/mm/yy]	UT			[arcsec]	time [s]	$10^{-3} I_{\rm c}$	Mx/cm²	Mx/cm²	Mx/cm²
set I	10/09/07	08:00:00	2031	1	$58 \times 164$	9.6	0.8	56.7	9.7	1.6
set II	27/02/07	00:20:09	2048	1	$0.16 \times 164$	67.2	0.25	54.6	11.0	1.7
set III	09/09/07	13:05:05	2029	0.4	$160 \times 32$	9.6	1	53.5	6.8	0.3

Notes. The last three columns, from left to right, give the mean values of the transversal (with respect to the line of sight), unsigned longitudinal, and signed longitudinal magnetic flux density.

Source LaTeX | All tables | In the text

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