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$\begin{figure} \par\includegraphics[width=6.5cm,clip]{1944fig1.eps} \end{figure}$ Figure 1: An example of RS blips (narrow-band type III bursts) on 2002 April 14, around 0536 UT observed by PMO, without any flare detected by H $\alpha$ and X-ray (from SGD). Top panel: time profile at a fixed frequency of 5.5 GHz. The flux is given in arbitrary units. Middle panel: 36 RS blips identified by vertical lines on the time profile at a fixed frequency of 5.5 GHz. The mean quasi-period of bursts is about $0.4 \pm 0.2$ s. $\sigma$ gives the standard deviation of the noise level before or after solar radio bursts. Bottom panel: dynamic spectra of RS blips groups over the of 4.5-7.5 GHz frequency band.
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{1944fig2.eps} \end{figure}$ Figure 2: A unique example has RS type III groups preceding microwave type V continuum for the flare of 1999 August 25. 26 individual RS type III bursts are identified by solid lines with a mean quasi-period of $2.0 \pm 0.6$ s. The illustration is similar to Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{1944fig3.eps} \end{figure}$ Figure 3: An example of two RS type III groups in the impulsive phase of microwave type IV bursts for the flare of 2002 September 11. Two groups of four individual RS type III bursts each are identified by solid lines with a mean quasi-period of $1.4 \pm 0.6$ s. This illustration is similar to Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{1944fig4.eps} \end{figure}$ Figure 4: An example of RS type III group in the decay phase of microwave type IV bursts for the flare of 2000 April 8. 37 individual RS type III bursts are identified by solid lines with a mean quasi-period of $1.5 \pm 0.5$ s. The illustration is similar to Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{1944fig5.eps} \end{figure}$ Figure 5: An example of an RS type III group without any other microwave emission for the flare of 1999 October 27. 5 individual RS type III bursts take place and the last 3 identified by solid lines have a mean quasi-period of $1.0 \pm 0.3$ s. The illustration is similar to Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{1944fig6.eps} \end{figure}$ Figure 6: An example of microwave pulsation group in the impulsive phase of microwave type IV bursts for the flare of 1999 December 16. 8 individual pulses occur and the last 6 identified by solid lines have a mean quasi-period of $3.0 \pm 0.5$ s. The illustration is similar to Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{1944fig7.eps} \end{figure}$ Figure 7: An example of a microwave pulsation group in the decay phase of microwave type IV bursts for the flare of 2002 June 1. 19 individual pulses are identified by solid lines with a mean quasi-period of $3.0 \pm 0.6$ s. The illustration is similar to Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{1944fig8.eps} \end{figure}$ Figure 8: A special microwave type III group mixed RS type III burst (solid lines) preceding the upward type III bursts (dashed lines) for the flare of 2002 March 18. Both RS and upward type III bursts have a very short quasi-period of 0.05 s. The 7.3 Ghz profile is overplotted after subtracting 700 flux units. One RS type III and two upward type III bursts are shown with dotted lines. The illustration is similar to Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{1944fig2.eps} \end{figure}$	Figure 2: A unique example has RS type III groups preceding microwave type V continuum for the flare of 1999 August 25. 26 individual RS type III bursts are identified by solid lines with a mean quasi-period of $2.0 \pm 0.6$ s. The illustration is similar to Fig. 1.
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$\begin{figure} \par\includegraphics[width=6.5cm,clip]{1944fig3.eps} \end{figure}$	Figure 3: An example of two RS type III groups in the impulsive phase of microwave type IV bursts for the flare of 2002 September 11. Two groups of four individual RS type III bursts each are identified by solid lines with a mean quasi-period of $1.4 \pm 0.6$ s. This illustration is similar to Fig. 1.
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$\begin{figure} \par\includegraphics[width=6.5cm,clip]{1944fig4.eps} \end{figure}$	Figure 4: An example of RS type III group in the decay phase of microwave type IV bursts for the flare of 2000 April 8. 37 individual RS type III bursts are identified by solid lines with a mean quasi-period of $1.5 \pm 0.5$ s. The illustration is similar to Fig. 1.
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$\begin{figure} \par\includegraphics[width=6.5cm,clip]{1944fig5.eps} \end{figure}$	Figure 5: An example of an RS type III group without any other microwave emission for the flare of 1999 October 27. 5 individual RS type III bursts take place and the last 3 identified by solid lines have a mean quasi-period of $1.0 \pm 0.3$ s. The illustration is similar to Fig. 1.
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$\begin{figure} \par\includegraphics[width=6.5cm,clip]{1944fig6.eps} \end{figure}$	Figure 6: An example of microwave pulsation group in the impulsive phase of microwave type IV bursts for the flare of 1999 December 16. 8 individual pulses occur and the last 6 identified by solid lines have a mean quasi-period of $3.0 \pm 0.5$ s. The illustration is similar to Fig. 1.
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$\begin{figure} \par\includegraphics[width=6.5cm,clip]{1944fig7.eps} \end{figure}$	Figure 7: An example of a microwave pulsation group in the decay phase of microwave type IV bursts for the flare of 2002 June 1. 19 individual pulses are identified by solid lines with a mean quasi-period of $3.0 \pm 0.6$ s. The illustration is similar to Fig. 1.
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