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Fig. 11


Left: velocities as a function of distance from the Sun for all the type III bursts using the Parker model (top) and the Dulk altitudes (bottom) after t = 5 s. The red line is a linear fit to the log of the velocity such that log10 (v) = ar + c. Right: Frequency and density profiles as a function of altitude for the Parker model (top) and Dulk model (bottom).

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