$\begin{figure} \par\includegraphics[height=6.15cm,width=6cm,clip]{5679fg1a.eps}\... ....eps}\includegraphics[height=6.15cm,width=5.35cm,clip]{5679fg1c.eps}\end{figure}$ Figure 1: Left: MDI/SoHO magnetogram. Middle: G-band slit-jaw filtergram. Right: example spectrogram. The slit position is indicated by the vertical black line. In the magnetogram the completely black and white regions involve $\pm$ 300 G and higher field strengths. The regions at $y=0{-}55\hbox {$^{\prime \prime }$ }$ and $y=60{-}95\hbox {$^{\prime \prime }$ }$ (measured along the slit) are indicated as non-magnetic and magnetic, respectively.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{5679fg2.eps}\end{figure}$ Figure 2: Variations in the rms of the continuum intensity in the non-magnetic region. The triangles mark the records selected for inversion.
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In the text

$\begin{figure} \par\includegraphics[height=5.4cm,width=8.05cm,clip]{5679fg3a.eps... ...{5mm} \includegraphics[height=5.4cm,width=7.85cm,clip]{5679fg3b.eps}\end{figure}$ Figure 3: Example of synthetic profiles (solid lines) resulting from the inversion and the observed profiles (circles) taken at 09:32:12 UT in the granule at y=94 $^{\prime \prime }$ close to the upper border of the magnetic region. The lower panels show the relative residuals of the fits.
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In the text

$\begin{figure} \par\includegraphics[height=5.9cm,width=8.4cm,clip]{5679fg4a.eps}... ...1.5mm} \includegraphics[height=5.9cm,width=8.3cm,clip]{5679fg4b.eps}\end{figure}$ Figure 4: Left: temperature stratifications. The mean in the non-magnetic $\langle T \rangle_{\rm non-mag}$ and magnetic regions $\langle T \rangle_{\rm mag}$ obtained by the inversion, the starting model GS (Grevesse & Sauval 1999), the model atmospheres HOLMU by Holweger & Müller (1974), VALC by Vernazza et al. (1981), and temporally and spatially averaged temperature from the 3D simulation SN by Stein & Nordlund (1998). Right: the mean velocity in the non-magnetic $\langle v_{\rm los}\rangle_{\rm non-mag}$ and magnetic $\langle v_{\rm los}\rangle_{\rm mag}$ regions. Temporally and spatially averaged vertical velocity SN is from the 3D simulation by Stein & Nordlund (1998).
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In the text

$\begin{figure} \par\includegraphics[height=4.55cm,width=8.2cm,clip]{5679fg5a.eps... ...s}\par\includegraphics[height=5.15cm,width=8.2cm,clip]{5679fg5d.eps}\end{figure}$ Figure 5: Space-time evolution of the observed line-center intensities. The optical depth of formation of the line cores from top to bottom are: $\log\tau_5 = -1.0, -1.2, -1.7,$ and -4.7. The greyscales are given as fractions of the continuum intensity.
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In the text

$\begin{figure} \par\includegraphics[height=4.55cm,width=8.1cm,clip]{5679fg6a.eps... ...}\par\includegraphics[height=5.15cm,width=7.75cm,clip]{5679fg6d.eps}\end{figure}$ Figure 6: Space-time evolution of continuum intensity, temperature differences at $\log\tau_5=0.0$ compared to the mean temperaturs in the non-magnetic region, macroturbulent velocity, and line-of-sight velocities at $\log\tau_5=-0.2$ , respectively from top to bottom. The greyscales are given as fractions of the continuum intensity, K, km s^-1, and km s^-1, respectively. The gravitational redshift of -636 m s^-1 was subtracted from line-of-sight velocities. Negative velocities indicate upflows. The images were smoothed out by boxes of $3\times 3$ pixels.
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In the text

$\begin{figure} \par\includegraphics[height=4.7cm,width=8.4cm,clip]{5679fg7a.eps}... ...g.eps}\includegraphics[height=5.25cm,width=7.5cm,clip]{5679fg7h.eps}\end{figure}$ Figure 7: Space-time evolution of temperature differences compared to the mean temperature stratification in the non-magnetic region ( left) and line-of-sight velocities ( right) in the selected optical depths. The greyscales are expressed in Kelvin and km s^-1. The gravitational redshift of -636 m s^-1 was subtracted from line-of-sight velocities. Negative velocities indicate upflows. The images were smoothed out by boxes of 3 $\times$ 3 pixels.
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In the text

$\begin{figure} \par\hspace*{-1mm}\includegraphics[height=5.75cm,width=8.15cm,cli... ...e*{3mm} \includegraphics[height=5.75cm,width=8cm,clip]{5679fg8b.eps}\end{figure}$ Figure 8: Top: horizontally and temporally averaged rms temperature fluctuations in the non-magnetic $\Delta T_{\rm non-mag}$ and magnetic $\Delta T_{\rm mag}$ regions, as well as in the 3D numerical simulations WFSLH by Wedemeyer et al. (2004, see p. 1131, Fig. 9# and SN by Stein & Nordlund (1998). Bottom: horizontally and temporally averaged rms line-of-sight velocity fluctuations in the non-magnetic $\Delta v_{\rm los,non-mag}$ and magnetic $\Delta v_{\rm los,mag}$ regions, as well as in the 3D numerical simulation SN by Stein & Nordlund (1998).
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In the text

$\begin{figure} \par\includegraphics[height=5.75cm,width=8cm,clip]{5679fg9.eps}\end{figure}$ Figure 9: Scatter plot of observed continuum intensity versus line-of-sight velocity inferred by the inversion at the optical depth $\log\tau_5=-0.2$ in the non-magnetic and magnetic regions. The thin solid line outlines the extents of these quantities obtained at the optical depth $\tau =1$ in the 3D numerical simulation SN by Stein & Nordlund (1998, see p. 917, Fig. 3#. Negative velocities indicate upflows, and the intensity axis shows relative continuum intensity reduced by unity.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{5679fg2.eps}\end{figure}$	Figure 2: Variations in the rms of the continuum intensity in the non-magnetic region. The triangles mark the records selected for inversion.
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$\begin{figure} \par\includegraphics[height=5.4cm,width=8.05cm,clip]{5679fg3a.eps... ...{5mm} \includegraphics[height=5.4cm,width=7.85cm,clip]{5679fg3b.eps}\end{figure}$	Figure 3: Example of synthetic profiles (solid lines) resulting from the inversion and the observed profiles (circles) taken at 09:32:12 UT in the granule at y=94 $^{\prime \prime }$ close to the upper border of the magnetic region. The lower panels show the relative residuals of the fits.
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$\begin{figure} \par\includegraphics[height=4.55cm,width=8.2cm,clip]{5679fg5a.eps... ...s}\par\includegraphics[height=5.15cm,width=8.2cm,clip]{5679fg5d.eps}\end{figure}$	Figure 5: Space-time evolution of the observed line-center intensities. The optical depth of formation of the line cores from top to bottom are: $\log\tau_5 = -1.0, -1.2, -1.7,$ and -4.7. The greyscales are given as fractions of the continuum intensity.
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