On 2005/05/03 @ 19:06 UT SOHO Telemetry Submode changed to Submode 6. It will be in Submode 6 until 2005/05/16 @ 12:00 UT. During that time EIT CME watch at full resolution (1024x1024).
02:30 UT WN West Spray-like front surpassed by following event (03:30 UT) practically before reaching the end of the C2 FOV. 03:30 UT WN West Bright ragged loop front with faint and diffuse loop-like extensions all around the bright loop. Very bright in C3. GOES reported a C9.3 X-ray flare from NOAA AR 10756 (S04W71) between 03:05 - 03:21 UT with peak emission at 03:14 UT. 06:06 UT EN East Apparently, kind of reconexion event (very faint). Difficult to give an exact time of first appearance. 11:06 UT WS West Faint and diffuse ragged loop front. By 11:54 UT is already surpassed by following event (11:30 UT). 11:30 UT WN West Initially bright and small front just appearing. It develops as a bright ragged loop front with faint and diffuse loop-like extensions all around the bright loop. GOES reported a M1.3 X-ray flare from NOAA AR 10756 (S04W76) between 01:11 - 11:35 UT with peak emission at 11:28 UT. 17:28 UT S East Complex event. A Partial Halo event was first seen in C2 at 17:28 UT as a bright and wide loop front (hereafter Event #1) above the SE Limb. By 17:54 UT, faint and diffuse extensions can be seen above the W Limb and N Pole (Event #2). The Event #2 surrounds the C2 occulting disk by 18:06 UT. The Event #1 was first seen in C3 at 17:42 UT appearing above the SE Limb, while the Event #2 shows up at 18:18 UT just above the N Pole. The Event #2 surrounds the C3 occulting disk by 19:12 UT. The Event #1 spans ~ 185 deg by 21:18 UT (LE almost at the end of the C3 FOV), from PA 25 - 210. The mean plane-of-sky speed of the LE of Event #1 (based on C3 data) at PA 108 was ~ 1100 km/sec, showing an slight deceleration. As for the Event #2, the mean C3-plane-of-sky speed of the LE at PA 355 was about 675 km/sec, showing practically no acceleration. GOES reported a long duration C8.5 X-ray flare on NOAA AR 10758 (S09E29) between 16:03 - 18:09 UT with peak emission at 17:05 UT. EIT 195 images show a strong brightening on the aforementioned region starting at 16:12 UT. A big change in the magnetic field topology in and around the AR between the frames taken at 16:24 and 17:21 UT (no frames in between) can be observed. By 17:21 UT post-flares loop begin to appear as well as dimming regions to N and S of the AR. By that time, EIT 195 running difference images show a huge intensity disturbance all across the eastern hemisphere. The signatures observed in EIT clearly indicate the association of the X-ray event with the Event #1 observed by LASCO C2/C3. It is difficult to say whether the Event #2 is part of the Event #1 or signature of an apparently backsided CME with source region on the northern hemisphere. Observation of the evolution of the complex event in C3 seems to indicate that the latter does correspond to a different event. In summary, the Event #1 has therefore been determined as a Partial Halo CME, frontsided, associated with a long duration C-class X-ray flare on NOAA AR 10758. A faint full halo CME (Event #2), apparently backsided, developed by the time. 20:30 UT WS West Extremely faint and diffuse front develops in the aftermath of previous complex event. Slow development of a system of loops can be seen superposed in the LOS. 22:06 UT S Pole Extremely faint expanding loop front. It fades throughout C3. 23:30 UT W Limb Bright spray-like front with faint and diffuse extensions to S. It fades throughout C3.
01:31 UT WS West Bright narrow structure and diffuse brightening follows event reported to start at 23:30 UT on previous day. Most likely part of the same event. 03:54 UT N Pole Faint and wide expanding loop front. It fades throughout C3. 08:30 UT W Limb Two events partly superposed in the LOS: i) Very bright ragged loop front developing toward W. ii)A faint and diffuse front just appearing a little bit to S. By 09:06 UT, the first front already reached the C2 FOV, while the second one becomes clearer developing toward WSW. By 09:30 UT, bright material follows this second front (bright inner core). GOES recorded an M 1.4 X-ray flare on NOAA AR 10756 (S05W89) between 07:57 - 08:19 UT with peak emission at 08:13 UT. A B9.1 X-ray flare follows (S06W80) between 09:07 - 09:26 UT with peak emission at 09:16 UT. 14:06 UT N East Couple of extremely faint expanding fronts. Barely visible in C3. 20:06 UT S West Extremely faint blob-like front.
06:06 UT S Pole Very faint and ragged elongated loop front. It is followed by a similar one at around 12:06 UT. They both fade throughout C3. 06:30 UT S West Diffuse front superposed in the LOS with existing twisted structures. By 07:54 UT, a faint expanding loop front develops. 09:54 UT E Limb Faint fan-like front. It fades throughout C2. 15:54 UT W Limb Bright and ragged loop front. Excess brightness can already be seen by 15:30 UT. Extremely faint loop- like extensions to N. 17:06 UT S East Ragged and very elongated loop front. It fades throughout C3. 20:06 UT WN West Spray-like front. It fades throughout C3.
01:31 UT WN West Elongated and bright loop front. 02:30 UT WN West Bright and ragged loop front. Much brighter than the previous one. 05:30 UT WN West Faint and ragged (elongated) loop front. 09:54 UT WN West Ragged loop front.