
LASCO Activity Report for
April 05, 2004 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
SOHO is back now from the telemetry keyhole, again with high rate
telemetry.
After bakeout, EIT synoptic observation program resumed on 04/05/2004
at 00:24 UT.
2004/04/02
03:00 UT S East Ragged front slightly to N of slow-development-of-
faint-system-of-loops event reported to start at
21:40 UT on previous day, and much faster.
04:40 UT N East Small ragged front in the trailing material of the
'flux-rope' event reported to start at 23:05 UT on
previous day. Another one at 07:20 UT.
10:41 UT N East Faint ragged loop front. Development missed because
of following data gap.
13:20 - 22:20 UT Data Gap
23:40 UT S West Ragged front already in progress after data gap.
2004/04/03
00:40 - 07:20 UT Data Gap
07:20 UT N East Ragged front already in progress after data gap.
11:00 UT S East Bright ragged front.
16:00 - 24:00 UT Data Gap
2004/04/04
00:40 UT S East Ragged front already in progress after data gap, close
to the edge of C2 FOV.
01:20 UT S East Ragged front preceded at 00:40 UT by a brighter (and
apparently slower) front slightly to S.
04:00 - 07:00 UT Data Gap
08:00 UT W Limb Small ragged front. It fades throughout C3.
12:20 UT S East Faint ragged loop front.
16:20 UT S West Couple of fairly faint ragged fronts. They fade
throughout C3.
16:40 UT S East Bright loop front and apparently twisted trailing
material.
2004/04/05
01:31 UT W Limb Spray-like front follwed at 03:54 UT by another
spray-like front.
02:54 UT S East Ragged loop front slightly to N of previous events. At
~04:06 UT it is followed by a brighter loop front at PA
that matches that of its southern leg. At ~01:13 UT a
CME is seen in EIT Fe XII running difference images
coming out from just behind the SE limb.
06:06 UT S East Bright loop front, strong cavity, and trailing material.
It surpasses previous event by the end of C2 FOV.
By the time, faint extensions (shock signatures) can be
seen to NE and SW giving the appearance of a partial
halo CME. NOAA AR 0588 (located S18E35) produced an
M1.7 X-ray flare starting at ~05:37 UT with peak
emission at 05:55 UT. The flare could be most likely
related to the event.
12:45 - 18:00 UT Temporary DSN Data Gap
Web curator:
K.M.Schenk
NASA Goddard Space Flight Center
Solar Physics Branch / Code 682
Greenbelt, MD 20771