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  • Explore the type III radio bursts delays (Krucker et al., 1999; Haggerty and Roelof, 2002). Possible explanations:
    • Propagation effects in the interplanetary medium (Cane and Erickson, 2003).
    • Delayed acceleration by large-scale coronal transient (EIT or Moreton) waves or by shock waves associated with narrow CMEs (Simnett et al., 2002; Rouillard et al., 2012). Also for non-impulsive SEP events.
    • Coronal magnetic restructuring in the aftermath of CMEs (Maia and Pick, 2004; Klein et al. 2005; van Driel-Gesztelyi et al., 2014).

 

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