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

Figure 9a(above)

Fig.9a (~0.03Mb), Fig.9b (~0.03Mb): CDS observations between 07:07 and 07:58 UT for He I (a) and O IV (b) lines. Top panels, intensity; middle panels, Dopplerhift; low panels, line width. The redshifted part corresponds to the SUMER bubble A, the blueshifted one to the SUMER structure B.