$\begin{figure} \par\hspace*{1mm}\includegraphics[width=7.35cm,clip]{5691f1a.ps}\vspace*{2mm} \includegraphics[width=7.5cm,clip]{5691f1b.ps}\end{figure}$ Figure 1: Temperature and density profiles from the footpoint (s=0 cm) to the apex (s=1.5 $\times$ 10⁹ cm) of the loop during explosive heating. Times: 5 s (solid); 10 s (dot); 15 s (dash); 20 s (dot-dash); 25 s (triple dot-dash); and 30 s (long dash).
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{5691f3.ps}\end{figure}$ Figure 3: The ratio of thermal flux ( $F_{\rm c}$ ) to saturated thermal flux ( $F_{\rm s}$ ) from the footpoint to the apex of the loop during explosive heating. Times: 1 s (solid); 5 s (dot); 10 s (dash); 20 s (dot-dash); and 30 s (triple dot-dash).
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In the text

$\begin{figure} \par\includegraphics[width=7.55cm,clip]{5691f5.ps}\end{figure}$ Figure 5: The ratio of total energy (thermal + kinetic) to total heat input during explosive heating.
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In the text

$\begin{figure} \par\hspace*{-1mm}\includegraphics[width=7.55cm,clip]{5691f6a.ps}\vspace*{2mm} \includegraphics[width=7.65cm,clip]{5691f6b.ps}\end{figure}$ Figure 6: The predicted counts (as functions of temperature and spatial location) at 2 s intervals, between 4 s and 20 s, for the Fe VIII emission in the SolarB-EIS short wavelength (170-210 Å) range during explosive heating. Times: 4 s (solid); 6 s (dot); 8 s (dash); 10 s (dot-dash); 12 s (triple dot-dash); 14 s (long dash); 16 s (cross); 18 s (asterisk); and 20 s (diamond).
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In the text

$\begin{figure} \par\includegraphics[width=6.85cm,clip]{5691f7a.ps}\vspace*{2mm} ... ...f7c.ps}\vspace*{2mm} \includegraphics[width=6.85cm,clip]{5691f7e.ps}\end{figure}$ Figure 7: The predicted counts (as a function of temperature) for the emission from higher charge states of iron in the SolarB-EIS short wavelength (170-210 Å) range during explosive heating. Charge states: Fe VIII (solid); Fe IX (dot); Fe X (dash); Fe XI (dot-dash); Fe XII (triple dot-dash); and Fe XIII (long dash).
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In the text

$\begin{figure} \par\includegraphics[width=7cm,clip]{5691f7b.ps}\vspace*{2mm} \in... ...691f7d.ps}\vspace*{2mm} \includegraphics[width=7cm,clip]{5691f7f.ps}\end{figure}$ Figure 8: The predicted counts (as a function of spatial location) for the emission from higher charge states of iron in the SolarB-EIS short wavelength (170-210 Å) range during explosive heating. Charge states: Fe VIII (solid); Fe IX (dot); Fe X (dash); Fe XI (dot-dash); Fe XII (triple dot-dash); and Fe XIII (long dash).
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In the text

$\begin{figure} \par\hspace{1mm}\includegraphics[width=7.35cm,clip]{5691f1a.ps}\vspace{2mm} \includegraphics[width=7.5cm,clip]{5691f1b.ps}\end{figure}$	Figure 1: Temperature and density profiles from the footpoint (s=0 cm) to the apex (s=1.5 $\times$ 10⁹ cm) of the loop during explosive heating. Times: 5 s (solid); 10 s (dot); 15 s (dash); 20 s (dot-dash); 25 s (triple dot-dash); and 30 s (long dash).
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$\begin{figure} \par\includegraphics[width=7.25cm,clip]{5691f2a.ps}\par\includegraphics[width=7.25cm,clip]{5691f2b.ps}\end{figure}$	Figure 2: The time-evolution of the apex temperature and density during and following explosive heating.
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$\begin{figure} \par\includegraphics[width=7.6cm,clip]{5691f3.ps}\end{figure}$	Figure 3: The ratio of thermal flux ( $F_{\rm c}$ ) to saturated thermal flux ( $F_{\rm s}$ ) from the footpoint to the apex of the loop during explosive heating. Times: 1 s (solid); 5 s (dot); 10 s (dash); 20 s (dot-dash); and 30 s (triple dot-dash).
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$\begin{figure} \par\includegraphics[width=6.8cm,clip]{5691f4a.ps}\vspace{2mm} \... ...1f4c.ps}\vspace{2mm} \includegraphics[width=6.8cm,clip]{5691f4d.ps}\end{figure}$	Figure 4: The ionisation balance of several ions of iron during explosive heating. The ion populations are far from equilibrium.
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$\begin{figure} \par\includegraphics[width=7.55cm,clip]{5691f5.ps}\end{figure}$	Figure 5: The ratio of total energy (thermal + kinetic) to total heat input during explosive heating.
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$\begin{figure} \par\hspace{-1mm}\includegraphics[width=7.55cm,clip]{5691f6a.ps}\vspace{2mm} \includegraphics[width=7.65cm,clip]{5691f6b.ps}\end{figure}$	Figure 6: The predicted counts (as functions of temperature and spatial location) at 2 s intervals, between 4 s and 20 s, for the Fe VIII emission in the SolarB-EIS short wavelength (170-210 Å) range during explosive heating. Times: 4 s (solid); 6 s (dot); 8 s (dash); 10 s (dot-dash); 12 s (triple dot-dash); 14 s (long dash); 16 s (cross); 18 s (asterisk); and 20 s (diamond).
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$\begin{figure} \par\includegraphics[width=6.85cm,clip]{5691f7a.ps}\vspace{2mm} ... ...f7c.ps}\vspace{2mm} \includegraphics[width=6.85cm,clip]{5691f7e.ps}\end{figure}$	Figure 7: The predicted counts (as a function of temperature) for the emission from higher charge states of iron in the SolarB-EIS short wavelength (170-210 Å) range during explosive heating. Charge states: Fe VIII (solid); Fe IX (dot); Fe X (dash); Fe XI (dot-dash); Fe XII (triple dot-dash); and Fe XIII (long dash).
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$\begin{figure} \par\includegraphics[width=7cm,clip]{5691f7b.ps}\vspace{2mm} \in... ...691f7d.ps}\vspace{2mm} \includegraphics[width=7cm,clip]{5691f7f.ps}\end{figure}$	Figure 8: The predicted counts (as a function of spatial location) for the emission from higher charge states of iron in the SolarB-EIS short wavelength (170-210 Å) range during explosive heating. Charge states: Fe VIII (solid); Fe IX (dot); Fe X (dash); Fe XI (dot-dash); Fe XII (triple dot-dash); and Fe XIII (long dash).
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