Catalogue of coronal mass ejections and associated phenomena

Moreno, G.; Berhondo, A. Mendez; Taboada, Ramón E. Rodríguez

doi:10.1016/s1384-1076(98)00012-8

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2004

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“…Catalogues of recorded CMEs, some including associated phenomena, have already been compiled and published (cf. for example Yashiro et al 2001;Gil Moreno et al 1998).…”

Section: Introductionmentioning

confidence: 99%

Solar type II and type IV radio bursts observed during 1998–2000 with the ARTEMIS-IV radiospectrograph

Caroubalos

Hillaris

Bouratzis

et al. 2004

A&A

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-68% of the catalogue events were associated with CMEs. -67% of the type II events were associated with CMEs, in accordance with previous results. This percentage rises to 79% in the case of composite type II/IV events. -77% of the type IV continua were associated with CMEs, which is higher that the CME-type II association probability. -The type II associated CMEs had an average velocity of (835± 380) km s −1 , while the CMEs not associated with type IIs had an average velocity of (500 ± 150) km s −1 . -All events, but one, were well associated with Hα and/or SXR flares.-Most of the CME launch times precede by 5−60 min (30 min on average) the associated SXR flare peak; an important fraction (72%) precede the flare onset as well.

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“…Catalogues of recorded CMEs, some including associated phenomena, have already been compiled and published (cf. for example Yashiro et al 2001;Gil Moreno et al 1998).…”

Section: Introductionmentioning

confidence: 99%