All Figures

$\begin{figure} \par\includegraphics[width=8cm,clip]{1596fig1.eps} \end{figure}$ Figure 1: The geometry used for the inclination, $\chi$ , and the arc angle, $\theta$ . Refer to Eq. (8) for how these parameters can be applied to coronal loop code.
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In the text

$\begin{figure} \par\includegraphics[height=6.4cm,width=8.3cm,clip]{1596fig2.eps} \end{figure}$ Figure 2: $\xi =10$ km s^-1; a) Maximum proton temperature (MK); b) maximum proton velocity (km s^-1), c) minimum proton density ( ${\times }10^{8}$ cm^-3); d) minimum pressure (dyne cm^-2).
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In the text

$\begin{figure} \par\includegraphics[height=6.4cm,width=8.1cm,clip]{1596fig3.eps} \end{figure}$ Figure 3: $\xi =14$ km s^-1. a) Maximum proton temperature (MK), b) maximum proton velocity (km s^-1); c) minimum proton density ( ${\times }10^{8}$ cm^-3); d) minimum pressure (dyne cm^-2).
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1596fig4.eps} \end{figure}$ Figure 4: The regions of loop heating (based on Fig. 2).
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In the text

$\begin{figure} \par\includegraphics[height=6.7cm,width=8.6cm,clip]{1596fig5.eps} \end{figure}$ Figure 5: L=40 Mm. a) Maximum proton temperature (MK); b) maximum proton velocity (km s^-1); c) minimum proton density ( ${\times }10^{8}$ cm^-3); d) minimum pressure (dyne cm^-2). No data is plotted in the top left hand corner of each plot as these would be hydrostatic solutions and cannot be evaluated by our dynamic code.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{1596fig6.eps} \end{figure}$ Figure 6: L=10 Mm, "cool'' coronal loop heated by Alfvénic turbulence. Top left: proton (solid line) and electron (dashed line) temperature along the loop semi-circular length; top right: proton velocity (solid), is near-zero and wave amplitude (dashed) appears to remain constant (i.e. little dissipation); bottom left: electron density; bottom right: wave pressure (top plot) and combined electron and proton pressure (bottom plot). In this simulation, wave amplitude $\xi =10$ km s^-1, and turbulent driving scale l=280 km.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1596fig7.eps} \end{figure}$ Figure 7: The temperature ( top), heating rate ( middle) and density ( bottom) progression of a L=600 Mm loop through the driving scales of l=60 (solid line), 200 (dotted), 500 (dashed), 2000 (dot-dash) and 8000 km (triple-dot-dash). The solid line represents the start of the simulation. Temperature inversion, footpoint, non-uniform, maximum temperature and quasi-uniform heating profiles are all evident.
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In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{1596fig8.eps} \end{figure}$ Figure 8: a) Temperature, velocity and pressure profiles for a 600 Mm (long) loop. $\xi =6$ km s^-1 and l=40 km. b) Corresponding energy fluxes can be directly compared with the profiles in the top frame. Kinetic energy flux (thin solid line), gravitational flux (dotted), radiative flux (long-dash), conductive flux (short-dash), enthalpy flux (dot-dash) and wave flux (triple-dot-dash) from Eq. (9) will all contribute toward the total flux (thick solid line). The total flux must remain constant to confirm steady state.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{1596fig1.eps} \end{figure}$	Figure 1: The geometry used for the inclination, $\chi$ , and the arc angle, $\theta$ . Refer to Eq. (8) for how these parameters can be applied to coronal loop code.
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$\begin{figure} \par\includegraphics[height=6.4cm,width=8.3cm,clip]{1596fig2.eps} \end{figure}$	Figure 2: $\xi =10$ km s^-1; a) Maximum proton temperature (MK); b) maximum proton velocity (km s^-1), c) minimum proton density ( ${\times }10^{8}$ cm^-3); d) minimum pressure (dyne cm^-2).
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$\begin{figure} \par\includegraphics[height=6.4cm,width=8.1cm,clip]{1596fig3.eps} \end{figure}$	Figure 3: $\xi =14$ km s^-1. a) Maximum proton temperature (MK), b) maximum proton velocity (km s^-1); c) minimum proton density ( ${\times }10^{8}$ cm^-3); d) minimum pressure (dyne cm^-2).
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1596fig4.eps} \end{figure}$	Figure 4: The regions of loop heating (based on Fig. 2).
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$\begin{figure} \par\includegraphics[height=6.7cm,width=8.6cm,clip]{1596fig5.eps} \end{figure}$	Figure 5: L=40 Mm. a) Maximum proton temperature (MK); b) maximum proton velocity (km s^-1); c) minimum proton density ( ${\times }10^{8}$ cm^-3); d) minimum pressure (dyne cm^-2). No data is plotted in the top left hand corner of each plot as these would be hydrostatic solutions and cannot be evaluated by our dynamic code.
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