VENUS reappeared in the C3 FOV at around 07:00 UT on 2004/06/09 (Wednesday). VENUS reappeared in the C2 FOV at around 20:00 UT on 2004/06/08 (Tuesday). VENUS entered the EIT FOV at 08:21 UT on 2004/06/08 (Tuesday). However, the signal was too faint at that part of the FOV. It can be discerned by around 12:00 UT on 2004/06/08. VENUS entered the C2 FOV from the left on 2004/06/07 (Monday) at around 13:20 UT. VENUS entered (from the left) the C3 field of view on 2004/06/03 (Thursday) at around 16:00 UT. SOHO Telemetry Submode changed to Submode 5 on 2004/04/13 at 16:00 UT (SUMER began observing on 2004/04/14). SUMER campaign runs until 2004/06/17. In other words, LASCO synoptic observation plan cadence remains the same but the EIT CME watch images will be reduced to half-resolution (512x512) during that period.
05:26 UT N East Diffuse faint and ragged loop front. Faint extensions above N Pole and on SE quadrant. Related to the event?? 06:06 UT E Limb Bright loop front. 06:36 UT Last C2 image before EIT Venus Observation Program. 07:45 - 19:15 UT LASCO C2/C3 Data Gap because of EIT Venus Observation Program. 19:36 UT First C2 image after EIT Venus Observation Program. 21:41 UT E Limb Blob-like front.
01:15 - 04:40 UT Temporary DSN Data Gap.