
LASCO Activity Report for
December 15, 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
2006/12/14 (Thursday)
NOTE 1:
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Proton storm slowly subsiding.
02:58 UT EN East Ragged (elongated) loop front developing gradually.
Some gusty outflow along the day.
20:30 UT WS West Diffuse ragged front later surpassed by the following
event.
22:30 UT WS West LASCO/EIT observed what would appear to be an
asymmetric Full Halo Event on 2006/12/14-15
(incomplete LASCO imagery by the time of writing).
The event was first seen in the LASCO C2 FOV on
12/14 at 22:30 UT as a very bright loop front on
the WSW Limb with diffuse extensions to N. By 23:30
UT, the bulk of the CME (which heads toward SW as
projected onto the plane of the sky) reached the outer
edge of the C2 FOV, while the diffuse extensions (on
W) are already well past the outer edge. An increase
of cosmic rays can be seen by this time. The event is
first seen in C3 on 12/14 at 23:42 UT, all above the
SW Limb with faint and diffuse extensions to the sides
of the bulk of the CME. The mean plane-of-sky speed
for the LE of the bulk of the CME at PA ~ 237 was
about 970 km/sec. On the other hand, if measured on
the LE of the extensions surrounding the bulk of the
CME at PA ~ 263, the plane-of-sky speed amount ~
1220 km/sec. Note that the measurements were based on
only a couple of C2 and C3 frames due to the no
availability of the "reformated" LASCO data at the
time of writing (we had yesterday a disk failure on
one of the LASCO operations machines and are right
now in the process of recovering). GOES recorded a
X1.5 X-ray flare on NOAA AR 10930 (S06W46) on 12/14
between 21:07 - 22:26 UT with peak emission at
22:15 UT. EIT 195 images show a brightness increase
on AR 10930 at 22:00 UT, the brightening becoming\
strongest at 22:12 UT. A rather circular wave (and
dimming) with epicenter on the AR mentioned can be
seen afterwards, developing almost all the way to the
far Limb (East). By 23:12 UT, a slight increase on
cosmic rays can be detected on EIT 195 images. In
summary, based on the few LASCO images available the
event has therefore been determined as a potentially
asymmetric full halo event, frontsided associated to
the X-class event that occurred late on 12/14 on AR
10930.
Last C2 image available by the time of writing: 23:30 UT
2006/12/15 (Friday)
No images available yet (computer maintenance).
Web curator:
K.M.Schenk
NASA Goddard Space Flight Center
Solar Physics Branch / Code 682
Greenbelt, MD 20771