
LASCO Activity Report for
August 17, 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
2006/08/16 (Wednesday)
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.
2006/08/17 (Thursday)
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).
Web curator:
K.M.Schenk
NASA Goddard Space Flight Center
Solar Physics Branch / Code 682
Greenbelt, MD 20771