Eruptive Prominence and Associated CME Observed with SUMER, CDS, and LASCO

by J.E. Wiik, B. Schmieder, T. Kucera, A.I. Poland, P. Brekke, and G.M. Simnett

Fig.7 (~0.05Mb): CDS observations of the prominences as seen in 6 lines (He I, O III, O IV, O V, Ne VI, and Mg X). The time indicate the mean of the rasters. The prominence is in emission for lines formed at T < 5 10⁵ K (until Ne VI). In Mg X we observe a lack of emission due to absorption of chromospheric continua.