
LASCO Activity Report for
November 05, 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
2004/11/04 (Thursday)
00:30 UT N Pole Faint and big expanding loop front.
04:06 UT S West Ragged loop front that fades in C3.
09:54 UT N East Bright loop front with a faint and diffuse extension
all above the NW, W, and NW Limbs. The event was first
seen on C3 at 10:42 UT above the NE Limb, developing
mainly toward NE. The extensions continue very clear
all around the N Pole, NW, W, and SW Limbs. Nothing
can be distinguished above the SE Limb. By 13:42 UT,
the event (excess brightness) spans in C3 ~ 280 deg
from PA 180 - 100. The mean plane-of-sky speed of the
LE of the front at PA 31 was ~ 635 km/sec (based on
C3 data) showing practically no acceleration.
GOES reported an C6.3 X-ray flare on NOAA AR 10696
(N09E28) between 08:45 - 10:04 with peak emission at
09:05 UT, most likely asssociated to the event described
above. On the other hand, EIT 195 images show a
brightening on the aforementioned AR at 09:00 UT, with
signatures of a CME developing mainly towards NE. But
please note that since around 07:13 UT excess activity
begins to be seen on that AR. GOES reported also a C1.0
X-ray flare on NOAA AR 10696 (N09E28) between 07:23 -
07:28 UT with peak emission at 07:26 UT.
In summary and based on its appearance in the C3 FOV,
the event has therefore been determined as a partial
halo CME, frontsided.
16:30 UT ES East Faint and elongated expanding loop front.
23:30 UT N East Extremely bright loop front spanning all above the
N Pole. By 00:30 UT on next day, fainter extensions can
be seen all around the western hemisphere. The event
was first seen on C3 at 23:42 UT just appearing above
the NE Limb, and developing mainly toward NE. The events
looks much brighter than the previous reported one.
Even though, nothing can be distinguished above the SE
Limb. Close inspection of C3 images show apparently
another front coming behind the first front. This first
front seems to develop mainly toward NE while the second
one seems to be the one that continues all around the
western hemisphere. The whole event spans in C3 about
290 deg (by 02:42 on 2004/11/05) from PA 180 - 110.
The mean plane-of-sky speed of the LE of the outermost
front at PA 27 was ~ 1053 km/sec (based on C3 data)
and showing practically no acceleration.
GOES reported an M2.5 X-ray flare on NOAA AR 10696
(N11E19) between 21:42 - 22:53 UT with peak emission at
22:29 UT, most likely associated to the first front;
and an M5.4 X-ray flare on the same AR (N08E18) between
22:53 - 23:26 UT with peak emission at 23:09 UT, most
likely asssociated to the second front. On the other
hand, EIT 195 images show a brightening on the
aforementioned AR at ~22:00 UT, with signatures of a
CME developing mainly towards NE. A strong wave-like
intensity disturbance can be distinguished developing
mainly toward N, NW, and W. By 23:12 UT another strong
brightening can be seen on the aforementioned AR
developing afterward with similar morphological
characteristics as before.
In summary, and from a global point of view, the event
as a whole has therefore been determined as a complex
partial halo CME, frontsided. But please keep in mind
that in fact two events close in space and time occurred.
2004/11/05 (Friday)
03:30 UT N Pole In the aftermath of previous halo event, several
faint and expanding loop fronts.
06:30 UT W Limb Jet-like front that quickly fade. It is followed at
07:54 UT by a bright and very narrow ragged loop front.
10:30 UT W Limb Similar event to the previous one. A jet-like front that
quickly fades preceding at 12:06 UT a brighter feature
resembling a very narrow loop front.
12:54 UT EN East Ragged and elongated front. It is preceded at 10:54 UT,
on W, by a very faint and diffuse loop front that fades
throughout C2. Apparent expanding outflow all around
the occulter. GOES reported an M4.0 X-ray flare on
NOAA AR 10696 (N08E15) between 11:23 - 11:33 UT with
peak emission at 11:30 UT.
14:54 UT W Limb Bright and narrow front.
Web curator:
K.M.Schenk
NASA Goddard Space Flight Center
Solar Physics Branch / Code 682
Greenbelt, MD 20771