- 2006/10/22: Venus started to be visible in the C2 FOV (upper right quadrant, moving from right to left).
04:30 UT N Pole Faint and diffuse front all above the N Pole extending up to the E limb (1). A brighter feature (ragged front) shows up on the W at 05:06 UT with some faint and diffuse extensions (2) to S up to the E Limb. All together, the event looks like a full halo event by this time ((elliptical shape), the signal being barely above the limb on the S Pole. Feature (1) is first seen in C3 at 05:18 UT, all above the E limb and N Pole. Feature (2) shows up on W at 06:42 UT, and at 08:18 UT the C3 occulting disk appears fully surrounded (difficult to establish the relationship between features (1) and (2)). The mean plane-of-sky speed of the outermost part of the LE of the complex event at different position angles is shown below (based on C3 data): - PA 085: ~ 450 km/sec (showing slight deceleration) - PA 310: ~ 670 km/sec (showing slight deceleration) - PA 204: ~ 210 km/sec (showing slight deceleration), most likely related to Feature (1). No frontsided signatures prior to the event on EIT 195 images, nor significant X-ray events were reported by the time. However, EIT 195 images seem to show the apparent slow lift-off of a prominence on NW between 03:48 - 11:12 UT, though it is really hard to say due to its faintness and size. In summary, the event has therefore been determined as a full Halo Event probably backsided based on the lack of significant frontsided activity. However please be aware that EIT 195 images did not show signatures of a backsided event either. 19:54 - 24:00 UT NO LASCO CME watch due to special observation program for Mars Express and Venus Express Campaign.
E Limb Slow development of a system of faint loop fronts since previous day. 05:54 UT N Pole Jet-like front. Last C2 image available by the time of writing: 12:06 UT.