- 2006/10/22: Venus starts to be visible in the C2 FOV (upper right quadrant, moving from right to left).
00:54 UT W Limb Very faint ragged front. 14:54 UT W Limb Ragged front starts to be discernible. It fades throughout C3. 20:06 - 24:00 UT NO LASCO CME watch due to special observation program for Mars Express and Venus Express Campaign.
12:06 UT S West Slow development of a system of extremley faint loop fronts. Difficult to give an exact time of first appearance. 20:06 - 24:00 UT NO LASCO CME watch due to special observation program for Mars Express and Venus Express Campaign.
19:31 UT E Limb Diffuse loop front (preceded by a very diffuse brightening at 18:54 UT). After the data gap it is seen developing as a very wide expanding ragged loop front, already covering all the eastern hemisphere, LE past the outer edge of the C2 FOV (the event extends up to past the poles, on NNW and SSW). It is first seen in C3 on 10/23 at 00:42 UT, covering al the eastern limb. The mean plane-of-sky speed of the LE at PA 87 is ~ 242 km/sec, showing practically no acceleration (based on C3 data). No X-ray events were recorded by GOES, nor significant X-ray activity could be observed on EIT 195 images prior to the time of first appearance of the event in C2. Therefore, the source of the event is most probably on the backside of the disk, somewhere close to the E limb.. 20:06 - 24:00 UT NO LASCO CME watch due to special observation program for Mars Express and Venus Express Campaign.
02:06 UT S West Brighty blob-like front. Gusty outflow. Last C2 image available by the time of writing: 05:06 UT.