
LASCO Activity Report for
May 4, 2006 SOHO Science Daily Meeting
Planner: K. Schenk, G. Stenborg
Event times are first frame seen in C2 camera unless otherwise noted.
These are preliminary observations for the daily SOHO science discussions.
Final analysis is reported on the Lasco CME list.
An archive of these reports is available.
Points Of Interest
2006/05/03 (Wednesday)
00:30 UT E Limb Diffuse and very faint front develops slowly, slightly
toward ENE. It fades throughout C3 (very faint). Some
gusty outflow along the day, especially on ENE.
23:30 UT S West Elongated and apparently twisted feature. Some
brightenings already seen since a little bit earlier.
EIt 1985 images show a prominence eruption to S
of NOAA AR 10875 between around 23:12 - 23:48 UT.
2006/05/04 (Thursday)
00:54 UT SS East Faint jet-like front that quickly fades.
01:31 UT S West Small brightening just appearing to S of event
reported to start at 23:30 UT, develops as a ragged
and expanding loop front [1]. It is followed by a
structured core (its inner front first seen in C2 at
02:54 UT) [2]. By 03:30 UT, a system of faint and
expanding loop fronts start to ve visible above the
S Pole [3]. By 06:54 UT this system of loops spans
~ 145 deg (from PA 110 - 255). Feature [1] is first
seen in C3 appearing above the SW Limb at 03:18 UT.
Feature [2] follows behind at 04:42 UT. Finally,
Feature [3] appears above the S Pole at 05:42 UT,
partly superposed in the LOS with [2]. The mean plane-
of-sky speed of the different features involved is
as follows (based on C3 data):
Feature [1] at PA 226: 520 km/sec (no acceleration)
Feature [2] at PA 225: 400 km/sec (no acceleration)
Feature [3] at PA 187: 300 km/sec (no acceleration).
The last measurement is not that reliable due to the
faintness of its LE (and superposition with Feature
[2]. GOES reported no significant X-ray activity by
the time prior to the LASCO C2 event, though it
recorded a B3.7 X-ray flare on NOAA AR 10876 (S17W41)
between 03:28 - 05:00 UT with peak emission at
04:35 UT. EIT 195 images shows between ~ 00:24 - 01:36
UT the eruption of the rest of the filament (see entry
at 22:30 UT on previous day), between AR 10876 and E05.
It is visible at least as far as skirt of the South
Polar Coronal Hole at ~ S60. EIT shows then, between
~ 01:13 - 06:48 UT, the slow evolution of post-CME
loops to SE of AR 10876. Given the observational
characteristics of the event C2 and C3 the event has
therefore been catalogued as a Partial Halo Event,
frontsided, associated to a filament eruption.
07:54 UT N West Faint and elongated front starts to be discernible.
Last C2 image available by the time of writing: 12:06 UT
Web curator:
K.M.Schenk
NASA Goddard Space Flight Center
Solar Physics Branch / Code 682
Greenbelt, MD 20771