
LASCO Activity Report for
July 18, 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
2005/07/15 (Friday)
00:54 UT ES East Faint jet-like front preceding an elongated loop-like
front at 02:30 UT. The loop front fades throughout C3.
02:30 UT W Limb Bright loop front developing slightly toward WSW. Much
gusty outflow continues all above the W Limb.
08:30 UT ES East Very diffuse and elongated loop-like front.
09:06 UT WN West Diffuse brightening just appearing, develops as a
not-well-defined front. It is followed at 09:54 by a
ragged loop front developing toward W.
11:54 UT WN West Bright and ragged loop front developing as a nice
balloon-type CME (with twisted inner structure).
Gusty outflow continues.
16:06 UT W Limb Elongated and bright front developing slightly toward
WSW. Gusty outflow continues.
20:06 UT WN West Faint front just appearing. It develops as a bright
loop front, followed (at 20:54 UT) by a wider and
bright loop front which in turn is followed by a bright
inner structure. By 22:30 UT, faint extensions
(apparently deflected structures) can be seen above the
S Pole. The event is seen in C3 at 21:18 UT above the
WNW Limb with faint extensions developing then above
the S Pole (they do not seem to surround the occulter).
EIT 195 images show, starting at around 19:13 UT, the
slow expansion of a system of loops on WNW (apparently
anchored barely behind the limb on NOAA AR 10786). By
20:48 UT, the expansion accelerates. GOES reported a
long duration C6.5 X-ray flare above NOAA AR 10786
(almost behind the limb) starting at 20:08 UT (Source:
BBSO Active Region Monitor). In brief, the event is
clearly a limb event. Its associated shock gives the
appearance to the event of, at least, a faint partial
halo.
2005/07/16 (Saturday)
00:06 UT W Limb Small front develops as a relatively bright and ragged
loop front slightly toward WSW. Gusty outflow continues.
EIT show a strong CME signature with source region
nearby AR 10790 by the end of previous day.
01:32 UT EN East Slow development of a faint system of loops along
streamer. Pseudo-continues outflow superposed in the
LOS.
13:54 UT WN West Initially bright ragged front that quickly fades in
the gusty outflow.
19:31 UT E Limb Extremely faint front starts to be discernible above
the E Limb in C2 (though it is difficult to precise the
exact time) partly superpose with the pre-existent
development of a faint system of loops on ENE. Our front
develops then in C2 as a very faint (and slow) full halo
CME (though extremely faint on W). It is first seen in
C3 just appearing above the E Limb at 23:18 UT (the
part of the event on W, if any, is not discernible in
C3). By 06:42 UT, the event is already barely discernible
(the LE on W just by 11.5 solar radii). No clear
signatures of any frontsided event can be seen on EIT
195 images by the time.
2005/07/17 (Sunday)
00:06 UT S East Slow development of a faint system of wide and
expanding loops. Difficult to give an exact time of
first appearance.
00:54 UT W Limb Fan-like front immediately followed a little bit to N
by a diffuse and elongated loop-like front. They fade
throughout C3.
04:06 UT W Limb Ragged loop front that fades throughout C3.
07:32 UT W Limb Bright and narrow front followed at 09:54 UT by a
bright and ragged front. By 10:34 UT, an initially
bright ragged loop front follows, developing slightly
toward WNW. The three fronts are then quickly surpassed
by the following halo event.
11:30 UT N west Very strong loop-like front partly superposed with
previous event (see entry at 07:32 UT). By 11:54 UT,
faint loop-like extensions can be seen all above the
S Pole, the C2 occulting disk being completely covered
by 12:06 UT. By that time, the LE of the event on W is
already past the outer edge of the C2 FOV, while the
halo extensions on E are just above the limb. Much
gusty outflow then on the W-WNW Limb. The event is
first seen in C3 at 12:18 UT, as a very bright loop
front on NW surrounded by faint and diffuse extensions
that almost cover completely the C3 occulting disk
(which is then fully surrounded by 12:42 UT). The mean
plane-of-sky speed of the LE of the event (outermost
front) at several PA is given below (based on C3 data):
. PA 049: 1060 km/sec
. PA 232: 1340 km/sec
. PA 304: 1453 km/sec
. PA 350: 1364 km/sec
showing practically no acceleration (in all four cases).
GOES reported multiple B-class activity during the day
on NOAA ARs 10790 (in average at S10W90) and 10789 (in
average at N13W90) plus an impulsive C4.3 X-ray flare
on AR 10790 (S10W90) that peaked at 06:29 UT. They do
not seem to be directly associated with the big halo
under analysis, as observed in the EIT 195 images. EIT
195 running difference images show signatures of a big
CME with source region behind the limb (most likely
nearby the actual location behind the disk of the
already gone 10786). It starts to be clearly seen by
10:50 UT as the expansion of a loop front above the WNW
limb, which seems to break up by 11:36 UT. A big
intensity disturbance to N and S above the limb (as
well as partly on the most western part of the disk)
can be seen afterward. In summary, the event has
therefore been classified as a strong and asymmetric
full halo event, backsided. Note that after ~14:00 UT,
a slight and gradual increase of energetic particles
hitting the CCD can be seen in C2 images.
13:54 UT W Limb In the aftermath of the Halo CME, the slow development
of a faint system of loops can be seen. Difficult to
give an exact time of first appearance.
2005/07/18 (Monday)
Much gusty outflow on ENE and ESE since late on previous day.
00:30 UT WN West Faint loop front in the gusty outflow.
Time of the last C2 image under analysis: 12:06 UT.
Web curator:
K.M.Schenk
NASA Goddard Space Flight Center
Solar Physics Branch / Code 682
Greenbelt, MD 20771