All Figures

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{9043fig1.eps}\end{figure}$ Figure 1: The function R₀(z)=A₀zj₁(z) of the homogeneous solution is plotted as a function of $z=a\eta$ to show the radial domains of the axisymmetric plasma structures.
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{9043fig2.eps}\end{figure}$ Figure 2: The power series solution R₁₍₁₂₎(z) of the particular solution, with $A=1\times 10^{-7}$ , is plotted as a function of z to show the plasma pressure effect on the radial domains of the axisymmetric plasma structures.
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{9043fig3.eps}\end{figure}$ Figure 3: The power series solution R₁₍₉₎(z) of the particular solution, with $A=1\times 10^{-7}$ and $\kappa ^{3}=16$ , is plotted as a function of z to show the plasma pressure effect on the radial domains of the axisymmetric plasma structures.
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{9043fig4.eps}\end{figure}$ Figure 4: The power series solution R₁₍₆₎(z) of the particular solution, with $A=1\times 10^{-7}$ and $\kappa ^{3}=16$ , is plotted as a function of z to show the plasma pressure effect on the radial domains of the axisymmetric plasma structures.
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In the text

$\begin{figure} \par\includegraphics[width=6.8cm,clip]{9043fig5.eps}\end{figure}$ Figure 5: The power series solution R₁₍₃₎(z) of the particular solution, with $A=1\times 10^{-7}$ and $\kappa ^{3}=16$ , is plotted as a function of z to show the plasma pressure effect on the radial domains of the axisymmetric plasma structures.
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In the text

$\begin{figure} \par\includegraphics[width=6.8cm,clip]{9043fig6.eps}\end{figure}$ Figure 6: The power series solution R₁₍₀₎(z) of the particular solution, with $A=1\times 10^{-7}$ and $\kappa ^{3}=16$ , is plotted as a function of z to show the plasma pressure effect on the radial domains of the axisymmetric plasma structures.
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In the text

$\begin{figure} \par\includegraphics[width=6.4cm,clip]{9043fig7.eps}\end{figure}$ Figure 7: The magnetic field lines using the homogeneous solution R₀(z) are shown with C=+0.05, C=+0.20, C=+0.40, C=+0.60, C=+0.80, and C=+1.00 from the outer to inner contours respectively. The axes are labelled in $x=\cos\theta$ , and the contribution of the plasma pressure represented by R₁(z) is neglected here.
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In the text

$\begin{figure} \par\includegraphics[width=6.4cm,clip]{9043fig8.eps}\end{figure}$ Figure 8: The asymptotically bounded evolution function, the lower curve, is plotted as a function of the normalized time $\tau$ with $\vert H\vert/\alpha =0.5$ , whereas the unbounded evolution function, the upper curve, is plotted with $H/\alpha =0.1$ .
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In the text

$\begin{figure} \par\includegraphics[width=6.7cm,clip]{9043fig9.eps}\end{figure}$ Figure 9: The explicit radial dependence of pressure profile $\bar p_{1}(\eta)$ is shown as a function of the normalized radial label $\eta /\eta _{*}$ through the thick line. The explicit radial dependence of mass density profile $\bar\rho_{1}(\eta)$ is also shown through the thin line for comparisons.
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In the text

$\begin{figure} \par\includegraphics[width=6.1cm,clip]{9043fig10.eps}\end{figure}$ Figure 10: The full, explicit and implicit, radial mass density profile $\bar\rho(\eta,\bar P)$ using the homogeneous solution R₀(z) is shown as a function of z.
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In the text

$\begin{figure} \par\includegraphics[width=6.4cm,clip]{9043fig11.eps}\end{figure}$ Figure 11: The mass density contours $\bar\rho(\eta,\bar P)$ with $\bar C=0$ are shown with C=+200, C=+300, C=+400, and C=+500 from the outer to inner contours respectively.
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In the text

$\begin{figure} \par\includegraphics[width=5.8cm,clip]{9043fig12.eps}\end{figure}$ Figure 12: The general solution of the radial function R(z) is shown as a function of z.
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In the text

$\begin{figure} \par\includegraphics[width=6.1cm,clip]{9043fig13.eps}\end{figure}$ Figure 13: The full, explicit and implicit, radial mass density profile $\bar\rho(\eta,\bar P)$ is shown as a function of z.
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In the text

$\begin{figure} \par\includegraphics[width=6.4cm,clip]{9043fig14.eps}\end{figure}$ Figure 14: The magnetic field lines are shown with C=+0.0, C=+0.1, C=+0.3, C=+0.5, and C=+0.7 from the outer to inner contours respectively.
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{9043fig1.eps}\end{figure}$	Figure 1: The function R₀(z)=A₀zj₁(z) of the homogeneous solution is plotted as a function of $z=a\eta$ to show the radial domains of the axisymmetric plasma structures.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{9043fig2.eps}\end{figure}$	Figure 2: The power series solution R₁₍₁₂₎(z) of the particular solution, with $A=1\times 10^{-7}$ , is plotted as a function of z to show the plasma pressure effect on the radial domains of the axisymmetric plasma structures.
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$\begin{figure} \par\includegraphics[width=6.5cm,clip]{9043fig3.eps}\end{figure}$	Figure 3: The power series solution R₁₍₉₎(z) of the particular solution, with $A=1\times 10^{-7}$ and $\kappa ^{3}=16$ , is plotted as a function of z to show the plasma pressure effect on the radial domains of the axisymmetric plasma structures.
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$\begin{figure} \par\includegraphics[width=6.5cm,clip]{9043fig4.eps}\end{figure}$	Figure 4: The power series solution R₁₍₆₎(z) of the particular solution, with $A=1\times 10^{-7}$ and $\kappa ^{3}=16$ , is plotted as a function of z to show the plasma pressure effect on the radial domains of the axisymmetric plasma structures.
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$\begin{figure} \par\includegraphics[width=6.8cm,clip]{9043fig5.eps}\end{figure}$	Figure 5: The power series solution R₁₍₃₎(z) of the particular solution, with $A=1\times 10^{-7}$ and $\kappa ^{3}=16$ , is plotted as a function of z to show the plasma pressure effect on the radial domains of the axisymmetric plasma structures.
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$\begin{figure} \par\includegraphics[width=6.8cm,clip]{9043fig6.eps}\end{figure}$	Figure 6: The power series solution R₁₍₀₎(z) of the particular solution, with $A=1\times 10^{-7}$ and $\kappa ^{3}=16$ , is plotted as a function of z to show the plasma pressure effect on the radial domains of the axisymmetric plasma structures.
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$\begin{figure} \par\includegraphics[width=6.4cm,clip]{9043fig7.eps}\end{figure}$	Figure 7: The magnetic field lines using the homogeneous solution R₀(z) are shown with C=+0.05, C=+0.20, C=+0.40, C=+0.60, C=+0.80, and C=+1.00 from the outer to inner contours respectively. The axes are labelled in $x=\cos\theta$ , and the contribution of the plasma pressure represented by R₁(z) is neglected here.
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$\begin{figure} \par\includegraphics[width=6.4cm,clip]{9043fig8.eps}\end{figure}$	Figure 8: The asymptotically bounded evolution function, the lower curve, is plotted as a function of the normalized time $\tau$ with $\vert H\vert/\alpha =0.5$ , whereas the unbounded evolution function, the upper curve, is plotted with $H/\alpha =0.1$ .
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$\begin{figure} \par\includegraphics[width=6.7cm,clip]{9043fig9.eps}\end{figure}$	Figure 9: The explicit radial dependence of pressure profile $\bar p_{1}(\eta)$ is shown as a function of the normalized radial label $\eta /\eta _{*}$ through the thick line. The explicit radial dependence of mass density profile $\bar\rho_{1}(\eta)$ is also shown through the thin line for comparisons.
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$\begin{figure} \par\includegraphics[width=6.1cm,clip]{9043fig10.eps}\end{figure}$	Figure 10: The full, explicit and implicit, radial mass density profile $\bar\rho(\eta,\bar P)$ using the homogeneous solution R₀(z) is shown as a function of z.
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$\begin{figure} \par\includegraphics[width=6.4cm,clip]{9043fig11.eps}\end{figure}$	Figure 11: The mass density contours $\bar\rho(\eta,\bar P)$ with $\bar C=0$ are shown with C=+200, C=+300, C=+400, and C=+500 from the outer to inner contours respectively.
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$\begin{figure} \par\includegraphics[width=5.8cm,clip]{9043fig12.eps}\end{figure}$	Figure 12: The general solution of the radial function R(z) is shown as a function of z.
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$\begin{figure} \par\includegraphics[width=6.1cm,clip]{9043fig13.eps}\end{figure}$	Figure 13: The full, explicit and implicit, radial mass density profile $\bar\rho(\eta,\bar P)$ is shown as a function of z.
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$\begin{figure} \par\includegraphics[width=6.4cm,clip]{9043fig14.eps}\end{figure}$	Figure 14: The magnetic field lines are shown with C=+0.0, C=+0.1, C=+0.3, C=+0.5, and C=+0.7 from the outer to inner contours respectively.
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