Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...265l..19k&link_type=abstract
Astrophysical Journal, Part 2 - Letters to the Editor, vol. 265, Feb. 1, 1983, p. L19-L21. Research supported by the Centre Nati
Astronomy and Astrophysics
Astrophysics
37
Solar Corona, Solar Radio Emission, Solar Storms, Electromagnetic Noise, Spectroheliographs, Type 4 Bursts
Scientific paper
Visible light observations of the corona have been combined with radioheliograph observations at metric wavelengths to examine the dynamic behavior of the corona during and after noise storm onsets and enhancements. For the period studied, the occurrence of such radio events is systematically associated with the addition of coronal material in the vicinity of the radio source. Some of the events correspond to mass ejection transients, but they more frequently represent merely a brightening, which grows in 1 hour or less with the coronal region and remains dense and stable for several hours.
House Leanna L.
Illing R.
Kerdraon Alain
Pick Monique
Sawyer Constance
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