Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..104...33r&link_type=abstract
(CNR, Workshop on Radio Continua during Solar Flares, Duino, Italy, May 27-31, 1985) Solar Physics (ISSN 0038-0938), vol. 104, M
Astronomy and Astrophysics
Astronomy
3
Solar Corona, Solar Flares, Solar Radio Bursts, Stellar Mass Ejection, Solar Wind Velocity, Spaceborne Astronomy, Spectroheliographs, Temporal Distribution, Visible Spectrum
Scientific paper
The results of a study are presented to determine the relationship between flare-related meter wavelength continuum outbursts and coronal mass ejection events. Using radio data obtained with the Culgoora radioheliograph and optical data from the SOLWIND experiment aboard the P-78 satellite a good temporal and positional overlap is found between the two types of events. In most cases the radio bursts could be classed as either a type-II-related Flare Continuum or a Slow Drift Continuum. Comparing properties for the events it was found that the continuum radio bursts were preferentially associated with the broader, more rapidly moving CME transients.
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