A linearly unstable, time-of-flight-truncated electron distribution in a randomly inhomogeneous plasma produces Langmuir wave intensity profiles with the same asymmetric shape as Type III solar radio bursts.
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Plasma instability in the front of ejected energetic electrons and Type III solar radiobursts
A linearly unstable, time-of-flight-truncated electron distribution in a randomly inhomogeneous plasma produces Langmuir wave intensity profiles with the same asymmetric shape as Type III solar radio bursts.