Correlated type III burst emission from distant sources on the sun

Details Correlated type III burst emission from distant sources on the sun Correlated type III burst emission from distant sources on the sun

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..112..133k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 112, no. 1, 1987, p. 133-142.

Astronomy and Astrophysics

Astronomy

6

Emission Spectra, Radio Sources (Astronomy), Solar Spectra, Spectrum Analysis, Stellar Spectrophotometry, Type 3 Bursts, Solar Activity, Solar Flares, Solar Limb, Solar Magnetic Field

Scientific paper

The authors report the observation and interpretation of a correlated type III burst emitted from distant sources on the Sun. The angular separation between the distant sources is as large as 26arcmin or ≡106km. There was an active region ≡30° behind the limb, and it is believed that the type III burst emission originated from activity in this region. The implications of the locations of the correlated sources with regard to the geometry of the magnetic structures involved in the flare process are discussed.

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