LASCO images severely degraded following the X18 proton flare from AR 0486 2003/10/28 and X11 proton flare from AR 0486 2003/10/29. LASCO images are at irregular times and cadences due to the impact of the proton levels on the instrument's telemetry buffer
20:54 UT HALO Bright front in S is fast bright full halo CME by 21:08. X11 X-ray flare AR 0486 S18W06. Proton levels raised again
01:51 UT E Limb Bright spray-like front, quite wide 10:23 UT S East Narrow loop front with some gusty outflow