Fast CMEs with filaments are more often produced by active-region and intermediate filaments, active-region eruptions are usually reconnection-triggered, quiet-Sun eruptions usually ideal-MHD-triggered, and the trigger type barely changes the final CME speed.
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A Statistical Study of Solar Filament Eruptions That Forms High-Speed Coronal Mass Ejections
Fast CMEs with filaments are more often produced by active-region and intermediate filaments, active-region eruptions are usually reconnection-triggered, quiet-Sun eruptions usually ideal-MHD-triggered, and the trigger type barely changes the final CME speed.