07:31 UT W Limb Ragged and diffuse front preceding the development toward SW of a system of wide and expanding (brighter) loop fronts. The outermost front seems to fully cover the C2 occulting disk by 09:08 UT. The signal on the eastern hemisphere is extremely faint and just above the occulting disk, while on W it is already past the outer edge of the C2 FOV. The event is first seen in C3 at 08:18 UT appearing above the SW limb as a diffuse loop front. The brighter system of loops shows up at 10:19 UT. By that time, the outer front fully surround the C3 occulting disk (signal on the eastern hemisphere just above the occulter). The mean plane-of-sky speed of the outermost front of the event (very faint and diffuse) at PA 230 was ~ 600 km/sec (based on C3 data), showing practically no acceleration. GOES reported prior and during the time of the LASCO event, a couple of impulsive B-class X-ray flares on NOAA AR 10904 on top of B-level X-ray activity: i) a B2.1 (at S11W09) between 04:54 - 05:00 UT with peak at 04:57 UT, and ii) a B3.4 (at S13W16) between 08:12 - 08:19 UT with peak at 08:15 UT. EIT 195 images show the formation of a dimming region to N of AR 10904 starting at 07:13 UT. Between 08:48 - 11:46 UT, formation of loops connecting from quiet Sun and AR 10904 to bright plasma NW of AR. At 10:14 UT, loops in center of AR open and appear to eject material. 16:30 UT S Pole Bright and wide loop front, the LE already half way to the end of the C2 FOV (note that there is a C2/C3/EIT 195 Full Field data gap between around 14:30 and 16:30 UT due to EIT/CDS ICAL01 -Intercalibration for EIT with CDS- between 15:00 - 16:20 UT). By 17:30 UT, the LE of the event is already past the outer edge of C2, and diffuse extensions all around the outer edge of the event fully cover the occulting disk. The event was first seen in C3 at 16:42 UT appearing about the S Pole. By 19:42 UT the C3 occulting disk is fully covered (signal on N just above the occulting disk). The mean plane-of-sky speed of the outermost front of the event (it becomes very diffuse by the end of the C3 FOV) at PA 175 was ~ 915 km/sec (based on C3 data), showing a slight acceleration. GOES reported a long duration C3.6 X-ray flare on NOAA AR 10904 (S16W08) between 14:37 - 19:22 UT with peak emission at 16:17 UT. EIT 195 images show a brightening on AR 10904 starting at 16:24 UT, peaking at around 17:12 UT. Nice post-flare loops. Formation of a dimming region all around the AR, most discernible to S of AR.
NO LASCO C2/C3 CME watch during 2006/08/17 and 08/18 due to a special Observation campaign with EIT (7 minute high cadence run in 304A until 08/18 22:00 UT, afterward CCD EIT Bakeout).