A computer simulation study of type III radio burst propagation through the solar corona

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Computerized Simulation, Solar Corona, Type 3 Bursts, Radio Emission, Radio Waves, Solar Radio Bursts

Scientific paper

Type III solar radio burst propagation through large-scale coronal structure is numerically simulated. It is shown that radio wave refraction in an overdense streamer results in an increase of the apparent radial distance of the type III fundamental source and produces a broadening of the radiation polar diagram in agreement with the observations. It is also verified that the well-known fine frequency structure of type IIIb emission can be due to the fibrous character of the streamer.

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