
LASCO Activity Report for
November 04, 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
2004/11/03 (Wednesday)
02:06 UT W Limb Kind of 'explosive' (and initially bright) ragged loop
front. Infalling material afterward. Pushed material
superposed in the LOS on NW with the slow development
of the system of loops reported in previous day. The
event fades throughout C2. GOES reported an M2.8 X-ray
flare from NOAA AR 0691 (N12W75) between 01:23 - 01:37
UT with peak emission at 01:33 UT. EIT 195 images show
a strong brightening on NOAA AR 0691 at -1:36 UT and
a big CME signature afterward, all above the western
Limb.
03:54 UT EN East Bright loop front with a very faint and diffuse
extension all above the SE Limb and S Pole. It develops
toward NE as a bright loop front, the southern leg much
fainter than the rest. By 04:30 UT, a ragged front
begins to be seen above the S Pole. Its evolution show
that this front seems to extend all above the W Limb,
N Pole, and NE Limb, looking like a second front in
the C2 FOV (just behind the original one at 03:54 UT)
on NE. The event was first seen on C3 above the E Limb,
developing afterward mainly toward NE as an asymmetric
loop front. The event looks pretty faint on SE, S, SW,
and W. By the time the LE on NE reaches the outer edge
of C3 (about 10:42 UT), the event looks like a partial
halo, spanning ~ 135 deg from PA 330 - 105. However,
in C2 one could say that the event (bulk of the mass
plus eventual shock) covers completely the occultor.
The mean plane-of-sky speed of the LE of the front at
PA 49 was ~ 750 km/sec (based on C3 data) showing
practically no acceleration.
GOES reported an M1.6 X-ray flare on NOAA AR 10696
(N09E45) between 03:23 - 03:57 with peak emission at
03:35 UT, most likely associated to the event described
above. On the other hand, EIT 195 images show a strong
brightening on the aforementioned AR at 03:36 UT,
followed by an intensity disturbance travelling mainly
toward NE, jointly with a wave-like disturbance
travelling partially across the disk with apparent
epicenter on AR 10696.
In summary and based on its appearance in the C3 FOV,
the event has therefore been determined as a partial
halo CME, frontsided.
16:06 UT EN East Bright loop front with a faint and diffuse extension
all above the SE Limb and S Pole. It's morphology is
pretty similar in appearance to that of the event at
03:54 UT. The difference is basically that i) it moves
apparently faster, ii) the faint extensions on SE and
S look a little bit brighter, and iii) the C3 occultor
seems to be completely covered (by 18:42 UT). The event
is first seen in C3 at 16:42 UT. The mean plane-of-sky
speed of the LE of the front at PA 43 was ~ 1016 km/sec
(based on C3 data) showing practically no acceleration.
GOES reported an M5.0 X-ray flare on NOAA AR 10696
(N09E38) between 15:35 - 15:55 with peak emission at
15:47 UT, most likely associated to the event described
above. On the other hand, EIT 195 images show a strong
brightening on the aforementioned AR at 15:48 UT,
followed as in the previous reported event by an
intensity disturbance travelling mainly toward NE,
jointly with a wave-like disturbance travelling
partially across the disk with apparent epicenter on
AR 10696. In summary, the event has therefore been
determined as an asymmetric 'full' halo CME, frontsided.
18:54 UT EN East Ragged expanding front with a bright inner part.
Please also note that GOES reported an M1.0 X-ray flare
again from NOAA AR 10696 between 18:03 - 18:35 UT with
peak emission at 18:26 UT.
EIT 195 images show a brightening on the aforementioned
AR starting at ~ 18:00 - 18:12 UT and an intensity
disturbance shortly afterward travelling mainly toward
W. By 22:08 UT, the event spans only about 70 deg in C3,
from PA 20 - 90.
2004/11/04 (Thursday)
Last C2 image analyzed at 00:54 UT.
Web curator:
K.M.Schenk
NASA Goddard Space Flight Center
Solar Physics Branch / Code 682
Greenbelt, MD 20771