All Figures

$\begin{figure} \par\includegraphics[width=8cm,clip]{1319fig1.eps} \end{figure}$ Figure 1: The coordinate system in which the particle motion is considered. The curve BQ represents the particle trajectory in the x-y plane.
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In the text

$\begin{figure} \par\includegraphics[width=6cm,clip]{1319fig2.eps} \end{figure}$ Figure 2: Radial position of the particle as a function of time. Used $\gamma _0=100,$ d₀=10⁶ cm and $\theta _0 = 90^{\circ }$ .
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In the text

$\begin{figure} \par\includegraphics[width=5cm,clip]{1319fig3.eps} \end{figure}$ Figure 3: The geometry of motion of a particle along a rotating field line BQ. The angles are $\angle {\rm XOM} = \Omega t,$ $\angle {\rm MBQ} = \phi _{\rm p}$ and $\angle {\rm MOQ}=\phi ',$ and the radius ${\rm OA=OB}=d_0.$
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In the text

$\begin{figure} \par\includegraphics[width=6cm,clip]{1319fig4.eps} \end{figure}$ Figure 4: Particle trajectories during the time interval $0 \leq t \leq 0.02$ s in laboratory frame. We considered the field lines which lie in the range of $-15\hbox {$^\circ $ }\leq \phi _{\rm p} \leq 15\hbox {$^\circ $ }$ with an interval of $5\hbox {$^\circ $ }.$ Assumed neutron star radius $R_{\rm n} \approx 10$ Km.
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In the text

$\begin{figure} \par\includegraphics[width=6cm,clip]{1319fig5.eps} \end{figure}$ Figure 5: The power emitted by a particle as a function of $\phi _{\rm p}.$ Theparameter $W_0 = 25.6 q^2 \Omega ^2/(3c {k_0}^4),$ and k₀=k at D=0.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1319fig6.eps} \end{figure}$ Figure 6: The simulated profiles: panel a) for $\theta = \rm {0^{\circ }}$ and panel b) for $\theta =-0.05^{\circ }.$ The parameter $\phi$ is the rotation phase. Used $\gamma _0 = 100$ and d₀ = 10 Km.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{1319fig1.eps} \end{figure}$	Figure 1: The coordinate system in which the particle motion is considered. The curve BQ represents the particle trajectory in the x-y plane.
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$\begin{figure} \par\includegraphics[width=6cm,clip]{1319fig2.eps} \end{figure}$	Figure 2: Radial position of the particle as a function of time. Used $\gamma _0=100,$ d₀=10⁶ cm and $\theta _0 = 90^{\circ }$ .
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$\begin{figure} \par\includegraphics[width=5cm,clip]{1319fig3.eps} \end{figure}$	Figure 3: The geometry of motion of a particle along a rotating field line BQ. The angles are $\angle {\rm XOM} = \Omega t,$ $\angle {\rm MBQ} = \phi _{\rm p}$ and $\angle {\rm MOQ}=\phi ',$ and the radius ${\rm OA=OB}=d_0.$
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$\begin{figure} \par\includegraphics[width=6cm,clip]{1319fig4.eps} \end{figure}$	Figure 4: Particle trajectories during the time interval $0 \leq t \leq 0.02$ s in laboratory frame. We considered the field lines which lie in the range of $-15\hbox {$^\circ $ }\leq \phi _{\rm p} \leq 15\hbox {$^\circ $ }$ with an interval of $5\hbox {$^\circ $ }.$ Assumed neutron star radius $R_{\rm n} \approx 10$ Km.
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$\begin{figure} \par\includegraphics[width=6cm,clip]{1319fig5.eps} \end{figure}$	Figure 5: The power emitted by a particle as a function of $\phi _{\rm p}.$ Theparameter $W_0 = 25.6 q^2 \Omega ^2/(3c {k_0}^4),$ and k₀=k at D=0.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1319fig6.eps} \end{figure}$	Figure 6: The simulated profiles: panel a) for $\theta = \rm {0^{\circ }}$ and panel b) for $\theta =-0.05^{\circ }.$ The parameter $\phi$ is the rotation phase. Used $\gamma _0 = 100$ and d₀ = 10 Km.
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