Type IV bursts and coronal mass ejections

Details Type IV bursts and coronal mass ejections Type IV bursts and coronal mass ejections

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..104..175g&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

Physics

8

Solar Corona, Stellar Mass Ejection, Type 4 Bursts, Statistical Distributions, Type 2 Bursts, Velocity Distribution

Scientific paper

The relationship between moving type IV bursts and coronal mass ejections (CMEs) is of interest, because it may yield insights into the origin and the physics of the ejecta. The statistical association of moving type IV bursts with CMEs is discussed and it is found that about one-third to one-half of the IVs occur in association with CMEs, while only about 5 percent of the CMEs are accompanied by moving type IVs. It is also found that the mean speed of the moving IVs is smaller than the mean speed of CMEs, and it is concluded that the type IVs move out with the bulk of the ejecta.

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