An association between coronal structures and type III burst sources

Details An association between coronal structures and type III burst sources An association between coronal structures and type III burst sources

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...111..306t&link_type=abstract

Astronomy and Astrophysics, vol. 111, no. 2, July 1982, p. 306-311. Research supported by the Centre National d'Etudes Spatiale

Astronomy and Astrophysics

Astrophysics

36

Solar Corona, Solar Maximum Mission, Stellar Structure, Type 3 Bursts, Coronagraphs, Data Reduction, Wave Propagation

Scientific paper

Observations of the coronal structures overlying type III radio burst producing regions, obtained with the HAO Coronograph/Polarimeter on board the Solar Maximum Mission, have been combined with observations of the type III bursts from the Mark III Nancay Radioheliograph at 169 MHz. A first qualitative comparison of the data, performed for two periods, indicates that the corona overlying type III producing sites is composed of small, discrete, over-dense structures, which are sometimes diverging and short-lived. The type III burst sources are complex, exhibiting elementary components. It is suggested that the type III burst structure follows that of the corona and that discrete structures may play a fundamental role for type III production.

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