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$\begin{figure} \par\includegraphics[width=6cm,clip]{8481fig1.eps}\end{figure}$ Figure 1: Model of thread in cylindrical geometry. The plot shows the profile for the Alfvén velocity: constant until R=10, then slowly increasing as 1.1r/(r+1). The Alfvén velocity is made dimensionless by the Alfvén velocity in the interior and the radius is expressed in gyroradii, $\sqrt {\rho _{\rm i}^2+\rho _{\rm s}^2}$ . The dots show the Alfvén resonance points in ideal MHDs.
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In the text

$\begin{figure} \par\includegraphics[width=7cm,clip]{8481fig2.eps}\end{figure}$ Figure 2: Wave profile for the first mode. The plot shows the current in the z direction, j_z (dashed line), and the magnetic field in the $\protect\varphi$ direction, $B_{\protect\varphi}$ (full line), as a function of the distance from the centre of the cylinder. The current is normalised by the current at r=0 and the magnetic field by $(\!\sqrt{\rho_{\rm i}^2+\rho_{\rm s}^2}/v_{\rm A})j_z$ at r=0.
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In the text

$\begin{figure} \par\includegraphics[width=7cm,clip]{8481fig3.eps}\end{figure}$ Figure 3: Damping distance as a function of the inner radius of the density tube. The damping distance is normalised by the average length of a coronal loop, $L=5 \times 10^7$ m, and R is expressed in gyroradii.
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In the text

$\begin{figure} \par\includegraphics[width=7cm,clip]{8481fig4.eps}\end{figure}$ Figure 4: Heating function in r, made dimensionless by $10^{-9}\sqrt {(\rho _{\rm i}^2+\rho _{\rm s}^2)}/v_{\rm A} \cdot j_z^2$ at r=0.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{8481fig5.eps}\end{figure}$ Figure 5: Sketch of the physical mechanism responsible for the maintenance of density threads.
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In the text

$\begin{figure} \par\includegraphics[width=6cm,clip]{8481fig1.eps}\end{figure}$	Figure 1: Model of thread in cylindrical geometry. The plot shows the profile for the Alfvén velocity: constant until R=10, then slowly increasing as 1.1r/(r+1). The Alfvén velocity is made dimensionless by the Alfvén velocity in the interior and the radius is expressed in gyroradii, $\sqrt {\rho _{\rm i}^2+\rho _{\rm s}^2}$ . The dots show the Alfvén resonance points in ideal MHDs.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7cm,clip]{8481fig3.eps}\end{figure}$	Figure 3: Damping distance as a function of the inner radius of the density tube. The damping distance is normalised by the average length of a coronal loop, $L=5 \times 10^7$ m, and R is expressed in gyroradii.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7cm,clip]{8481fig4.eps}\end{figure}$	Figure 4: Heating function in r, made dimensionless by $10^{-9}\sqrt {(\rho _{\rm i}^2+\rho _{\rm s}^2)}/v_{\rm A} \cdot j_z^2$ at r=0.
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$\begin{figure} \par\includegraphics[width=9cm,clip]{8481fig5.eps}\end{figure}$	Figure 5: Sketch of the physical mechanism responsible for the maintenance of density threads.
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