02:54 UT ES East Ragged loop front. It fades close to the inner edge of C3 FOV. 03:30 UT EN East Very faint ragged and diffuse front that quickly fades. It is followed at 06:54 UT by a similar front above the E Limb that also quickly fades. 03:30 UT W Limb Ragged elongated loop front with fain loop-like extensions to S. It is preceded at 01:54 UT by a faint kind-of spray-like front. 06:30 UT E Limb Another very faint and ragged front that quickly fades. 12:55 UT N Pole Extremely faint and diffuse front. Difficult to give an exact time of first appearance. Its development seems to be affected by event at 15:38 UT. 14:00 - 16:40 UT EIT Shutterless Run #2 (no C3 images, ~1 C2 image/hour) 15:38 UT WS West Complex event that developed as a very asymmetric halo CME. The event was first observed in C2 at about 15:38 UT above the WSW Limb as, apparently, two loop fronts embedded in a diffuse structure. By 17:50 UT the event developed as a very asymmetric full halo CME in C2; the leading edge in the SW direction having already left the C2 FOV, while in the E direction the front is barely above the C2 occultor. The event was first seen in C3 at 16:38 UT above the WSW Limb. Please anote that by that time a feature brighter to N starts developing toward ENE in the C3 FOV, and seems to give a different appearance to our event. By ~ 00:18 UT on next day the event is practically no longer visible, apparently without having reached the end of the C3 FOV. The mean plane-of-sky speed for the LE of the outermost loop front at PA ~ 245 was ~ 442 km/sec. On the other hand, the inner front showed a plane-of-sky speed of about 400 km/sec at PA ~ 250 (in both cases based only on C3 data). GOES did not record any significant X-ray activity by the time. Likewise, the available EIT Fe XII images do not show any signature on the visible disk. Please note that by that time EIT was performing the Run #2 of the Shutterless Campaign. Inspection of the EIT movie made with the images of the Shutterless sequence do not show anything (in the restricted FOV) that could be related to our event. The event has therefore been determined as an asymmetric 'full' halo CME, most probably backsided. 23:06 UT WN West Elongated and diffuse loop front.
N West Gusty outflow. ES East Infalling material. 01:31 UT W Limb Blob-like front becomes discernible. 09:30 UT WN West Diffuse and elongated ragged loop front.