$\begin{figure} \par\includegraphics[width=4cm,height=5cm,clip]{3750fig1.eps}\hsp... ...e*{4mm} \includegraphics[width=4cm,height=5cm,clip]{3750fig4.eps} \end{figure}$ Figure 1: Frequency dependence of the refractive index for $\omega _{\rm pe}/\omega _{\rm He} = 10$ , the angle between the wave vector and magnetic field $\theta = 0.0$ (panel a)), $\theta = 1.0$ (panel b)), and for $\omega _{\rm pe}/\omega _{\rm He} = 5$ , $\theta = 0.0$ (panel c)), $\theta = 1.0$ (panel d)). Branches 1, 2, and 3 correspond to the X (extraordinary), O (ordinary), and longitudinal modes, respectively. Branch 4 corresponds to the Z-mode, branch 5 corresponds to the waves with anomalous dispersion. $v_{\rm Te}^2/c^2 = 2\times 10^{-4}$ .
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In the text

$\begin{figure} \par\includegraphics[width=70mm,height=48mm,clip]{3750fig5.eps} \end{figure}$	Figure 2: Type II solar radio burst with harmonic-component splitting.
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