
LASCO Activity Report for
November 17, 2005 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
2005/11/16 (Wednesday)
13:31 UT S Pole Very faint loop front.
16:30 UT W Limb Partial Halo Event associated to filament eruption on
NW quadrant. Likely signatures of the event were first
seen in C2 at 16:30 UT on the W Limb, developing
as a relatively bright loop front with faint and
diffuse extensions to N. By 18:06 UT, a faint, diffuse,
and ragged loop front develops toward SW, spanning all
the way from the W limb up to past the S Pole,
apparently disturbing the southern leg of the loop
first mentioned. The loop front is first seen in C3
above at 18:18 UT just appearing above the W Limb.
Clear signatures of the second front can be seen above
the SW limb by 20:18 UT. By this time, it becomes
difficult to disentangle both features. The whole event
spans ~ 190 deg (from PA 155 - 345) in the C3 FOV at
23:42 UT. The mean plane-of-sky speed of the outermost
edge of the event at PA 261 was ~ 314 km/sec, showing
a slight acceleration. GOES recorded multiple B-class
X-ray flares during the day, all from NOAA AR 10822 in
addition to a C5.9 X-ray flare at S07E36 (AR 10822)
between 11:41 - 12:48 UT with peak emission at 12:13 UT.
EIT 195 images show a brightening on AR 10822 peaking
at 12:12 UT. No dimming can be discerned. There is then
a gradual brightening on the same AR starting at around
14:24 UT and peaking at 14:36 UT, not correlated with
any peak in X-rays. This second brightening seems to
happen a little bit after the beginning of the eruption
of an apparently small filament located close to the
equator in the NW quadrant (eruption that is then seen
developing mainly toward W). A dimming region develops
to the NE and W of the original filament location. It
is the filament eruption (which apparently started at
around 13:48 UT) the most likely EIT counterpart of
the LASCO event. The event has therefore been
determined as a Partial Halo Event, frontsided, most
likely associated with a filament eruption.
2005/11/17 (Thursday)
02:30 UT S West Small and elongated loop front that quickly fades.
06:30 UT E Limb Fan-like front.
Last C2 image available by the time of writing: 09:06 UT.
Web curator:
K.M.Schenk
NASA Goddard Space Flight Center
Solar Physics Branch / Code 682
Greenbelt, MD 20771