All Figures

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{0728Fig1.eps}\end{figure}$ Figure 1: Recorded spectrum with several investigated F III spectral line profiles.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0728Fig2.eps}\end{figure}$ Figure 2: The dependence of the position of the observed line center ( $X_{\rm C}$ ) as a function of the electron density (N) during the plasma decay.
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In the text

$\begin{figure} \par\includegraphics[width=7.1cm,clip]{0728F3.eps}\end{figure}$ Figure 3: F II Stark widths (W in pm) as a function of the electron temperature (T) in the $\rm 3s{-} 3p$ transition at 10²³m^-3 electron density. $\bullet$ , our experimental results, $\vartriangle$ , Platisa et al. (1977) and $\circ$ , Djenize et al. (1991). SCPF (full line) represents our calculations using the semiclassical perturbation formalism. Error bars include the uncertainties of the width and electron density measurements $({\pm } 20\%).$
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In the text

$\begin{figure} \par\includegraphics[width=7.1cm,clip]{0728Fig4.eps}\end{figure}$ Figure 4: F II Stark widths (W in pm) as a function of the electron temperature (T) in the $\rm 3s{-} 3p$ , $\rm 3p{-}3d$ and $\rm 3d{-} 4f$ transitions at 10²³ m^{- 3} electron density. $\bullet ,$ our experimental results; $\vartriangle ,$ Platisa et al. (1977) and $\circ$ , Djenize et al. (1991). SCPF (full line) represents our calculations using the semiclassical perturbation formalism. G (dashed lines), denotes values calculated by Griem (1974). Error bars include the uncertainties of the width and electron density measurements $({\pm } 20\%)$ . $\langle\lambda\rangle$ is the mean wavelength in the multiplet.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{0728F5.eps}\end{figure}$ Figure 5: F II Stark shifts (d in pm) as a function of the electron temperature (T) at 10²³ m^-3 electron density. $\bullet ,$ our experimental results and $\circ ,$ results from Djenize et al. (1991). SCPF (full line) represents our calculations using the semiclassical perturbation formalism. $\langle\lambda\rangle$ is the mean wavelength of the multiplet.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{0728F6.eps}\end{figure}$ Figure 6: F II electron Stark shifts (d in pm) as a function of the electron temperature (T) in the $\rm 3s{-} 3p$ , $\rm 3p{-}3d$ and $\rm 3d{-} 4f$ transitions at 10²³ m^-3 electron density. $\bullet ,$ our experimental results and $\circ$ , from Djenize et al. (1991). SCPF (full line) represents our calculations using the semiclassical perturbation formalism. G (dashed line), denotes calculations of Griem (1974). $\langle\lambda\rangle$ is the mean wavelength of the multiplet.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{0728Fig7.eps}\end{figure}$ Figure 7: F III electron Stark FWHM vs. electron temperature at 10²³ m^-3 electron density. G represents (dashed line) results from Dimitrijevic & Konjevic (1981) based on Griem's semiclassical method (see Griem 1974, Eq. (526)). GM denotes its modification by Dimitrijevic & Konjevic (1980). SEM denotes the modified semiempirical method (Dimitrijevic & Konjevic 1980). SE denotes the result from Griem's semiempirical calculation (Griem 1968). SCPF denotes our electron Stark width values calculated on the basis of the semiclassical perturbation formalism. $\bullet$ denotes our new experimental data and $\oslash$ denotes results from Puric et al. (1988).
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{0728Fig8.eps}\end{figure}$ Figure 8: F III electron Stark shift (d) vs. electron temperature at 10²³ m^-3 electron density. $\bullet$ denotes our experimental data. SCPF (full line) represents our electron Stark shift values calculated on the basis of the semiclassical perturbation formalism.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{0728Fig1.eps}\end{figure}$	Figure 1: Recorded spectrum with several investigated F III spectral line profiles.
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$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0728Fig2.eps}\end{figure}$	Figure 2: The dependence of the position of the observed line center ( $X_{\rm C}$ ) as a function of the electron density (N) during the plasma decay.
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$\begin{figure} \par\includegraphics[width=7.3cm,clip]{0728F5.eps}\end{figure}$	Figure 5: F II Stark shifts (d in pm) as a function of the electron temperature (T) at 10²³ m^-3 electron density. $\bullet ,$ our experimental results and $\circ ,$ results from Djenize et al. (1991). SCPF (full line) represents our calculations using the semiclassical perturbation formalism. $\langle\lambda\rangle$ is the mean wavelength of the multiplet.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{0728Fig8.eps}\end{figure}$	Figure 8: F III electron Stark shift (d) vs. electron temperature at 10²³ m^-3 electron density. $\bullet$ denotes our experimental data. SCPF (full line) represents our electron Stark shift values calculated on the basis of the semiclassical perturbation formalism.
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