Dynamics of small-scale magnetic fields on the Sun: observations and numerical simulations

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Table 3:

Line-of-sight components of unsigned IN magnetic field $\langle \vert B_{\rm LOS}\vert\rangle$ , averaged over field of view, at disc centre.
Source	Method	Av. field strength [G]
Khomenko et al. (2003)	IR lines	2.7-4
Domínguez Cerdeña	speckle &
et al. (2003)	line ratio	17-21
Lites &
Socas-Navarro (2004)	$V_{\rm tot}$	8-10
Orozco Suárez
et al. (2007)	inversion	3.4
Lites et al. (2008)	$V_{\rm tot}$	6
Martínez González
et al. (2008)	inversion	4.1
Bello González	speckle &
& Kneer (2008)	COG	2.2
Trujillo Bueno
et al. (2004)	Hanle	$\sim$ 100
this work:
observed	speckle &
	COG	3.0-4.0
simulated, original	at 150 km	16.1
simulated, original	COG	10.3
simulated, degraded	COG	3.2

Source LaTeX | All tables | In the text

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