The relationship between prominence eruptions and coronal mass ejections

Journal of Atmospheric and Solar-Terrestrial Physics

Volumn 62, Issue 16, 2000, Pages 1479-1487

  Simnett, G M ^a  

^a UNIVERSITY OF BIRMINGHAM   (United Kingdom)

Author keywords

Corona; Prominence; Sun

Indexed keywords

EID: 0040016230     PISSN: 13646826     EISSN: None     Source Type: Journal    
DOI: 10.1016/S1364-6826(00)00088-2     Document Type: Article

References (6)

1. Brueckner G.E.et al. The large angle spectrometric coronagraph (LASCO). Sol. Phys. 162:1995;357.
2. Delaboudiniere J.-P.et al. EIT, extreme ultraviolet telescope for the SOHO mission. Sol. Phys. 162:1995;291.
3. Dere K.P.et al. EIT and LASCO observations of the initiation of a coronal mass ejection. Sol. Phys. 175:1997;602.
4. Hundhausen A.J. Sizes and locations of coronal mass ejections: SMM observations from 1980 and 1984-1989. J. Geophys. Res. 98:1993;13,177.
5. Simnett, G.M., Hudson, H.S., 1997. In: Wilson, A. (Ed.), The evolution of a rapidly-expanding active region loop into a trans-equatorial coronal mass ejection, ESA Publications Division, ESTEC, Noordwijk, The Netherlands, ESA SP-415, p. 437.
6. Wiik J.E., Schmeider B., Kucera T., Poland A., Brekke P., Simnett G. Eruptive prominence and associated CME observed with SUMER, CDS and LASCO (SOHO). Sol. Phys. 175:1997;411.