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A three-dimensional reconstruction of the 2002 April 21 partial halo Coronal Mass Ejection (CME) has been made based on the O vi 1032 8 and [ Fe xviii] 974 8 lines observed by the Ultraviolet Coronagraph Spectrometer ( UVCS) on board the Solar and Heliospheric Observatory (SOHO). We use the Doppler velocities to derive the CME structure along the line of sight. UVCS observed the O vi line profiles split into strongly Doppler red-and blueshifted components, and the region of split profiles grewdoi:10.1086/506981 fatcat:74zp6imtfvbvbbirozfcx7r5ba