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

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

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...253..521i&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 253, no. 2, Jan. 1992, p. 521-524.

Astronomy and Astrophysics

Astrophysics

7

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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