
LASCO Activity Report for
December 31, 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
2004/12/29 (Wednesday)
NOTE: As on previous day, the multiple CMEs seen on WSW-SW along the day are
most probably associated with the X-ray activity, i.e. multiple C- and
B- class X-ray flares, reported by GOES during the day on NOAA AR
10713/10712 - by the time at around S10W90 - .
01:57 UT N Pole Very faint blob-like front preceded by a similar one
(which is already close to the end of the C2 FOV). A
couple more follow, developing toward NNW.
01:57 UT S West Elongated and initially bright feature. Asymmetric
and faint loop-like structure to N.
03:21 UT S West Another elongated and initially bright feature that
develops as an asymmetric loop front brighter to S.
06:21 UT S West Another elongated and initially bright feature that
develops as an asymmetric loop front brighter to S.
07:45 UT E Limb Initially bright ragged loop front that fades when
appearing the following event (*).
08:45 UT E Limb (*) Bright loop front with apparently twisted trailing
material developing toward ESE. A very faint and
diffuse loop-like feature (extensions?) moving toward
ENE follows its development.
10:45 UT S West Another elongated and initially bright feature that
develops as an asymmetric loop front (fainter than
the previous ones). Another one at 13:22 UT. At 16:21
UT, a spray-like front is immediately followed, a
little bit to N, by a ragged loop front developing
toward WSW. Another (smaller) spray front at 17:21 UT.
By 19:45 UT, an asymmetric loop front follows, much
brighter to S. Gusty outflow well into next day.
Signatures most likely related to B- and C-class X-ray
activity on NOAA AR 10713 (by the time at around S12W90).
Note that also an M1.4 X-ray flare from 10713 (S12W90)
was reported by GOES between 19:10 - 19:25 UT with
peak emission at 19:20 UT.
16:45 UT E Limb Big, wide, and very bright loop front followed by
gusty outflow at
roughly the PA of its southern leg (ESE), well into
next day. Some
infalling material by the end of the day on ENE.
Clear "pair formation" by ~ 00:21 UT on next day
at PA ~ 67 (separation point at ~ 4 solar radii).
GOES reported an M2.3 X-ray flare from NOAA AR 10715
(N04E62) between 15:57 - 16:38 with peak emission
at 16:27 UT.
2004/12/30 (Thursday)
00:45 UT S West Diffuse spray-like front. By the time, the slow
development of a faint system of loops along the
streamer starts to be discerned superposed in the LOS.
07:57 UT W Limb Faint elongated loop-like structure that fades very
close to the inner edge of the C3 FOV.
10:57 UT E Limb Wide, big and very bright loop front. By 11:45 UT,
extremely faint extensions can be seen surrounding
the C2 occulting disk. By 12:41 UT a new ragged front
seem to develop in the trailing material toward ENE.
The event is first seen in C3 at 11:33 UT above the
E Limb; by 12:33 UT extremely faint extensions seem
to surround the C3 occulting disk. The mean plane-of-
sky speed of the LE of the CME (based on C3 data)
at PA 90 was ~ 1132 km/sec (showing practically no
acceleration).
GOES reported high X-ray activity during the day
with a couple of M flares and multiple B- and C-
class X-ray flares from NOAA AR 10715. In particular,
it is worth to mention the following events, most
likely associated with the C2/C3 signatures
described above:
- a C1.3 (N04E52) between 10:10 - 10:19 UT, peak
emission at 10:17 UT,
- a M2.2 (N03E53) between 10:33 - 11:28 UT, peak
emission at 11:16 UT, and
- a C2.6 (N05E52) between 12:14 - 12:19 UT, peak
emission at 12:17 UT.
EIT 195 images show a strong brightening on the
aforementioned AR starting at 10:39 UT (clear
signature of the M2.2 flare). An intensity
disturbance (wave) is seen developing afterward
mainly toward W and SW of the AR.
In summary, the event has therefore been determined
as an extremely faint and asymmetric 'full' halo
event, frontsided.
17:45 UT E Limb Loop front that fades and gives place to another loop
(bubble-like) structure. By 23:30 is surpassed in the
C2 FOV by following event.
22:30 UT E Limb Another wide, big, and very bright loop front. By 23:30
UT, faint extensions can be seen surrounding the C2
occulting disk. By 00:54 UT on next day, a ragged
(faint) front can be seen developing above the W Limb,
with ragged extensions up to the S Pole, though it is
difficult to establish its association with the event
developing toward E. The event is first seen in C3 at
23:18 UT above the E Limb; by 23:42 UT faint extensions
surround the C3 occulting disk. The mean plane-of-sky
speed of the LE (based on C3 data) at PA 90 was ~ 1150
km/sec (showing practically no acceleration).
As mentioned in previous event, GOES reported high
X-ray activity during the day with a couple of M flares
and multiple B- and C- class X-ray flares from NOAA AR
10715. In particular, it is worth to mention the
following events, very likely associated with the C2/C3
signatures described above:
- a C4.1 (N03E46) between 21:41 - 21:56 UT, peak emission
at 21:52 UT,
- a M4.2 (N04E46) between 22:02 - 22:28 UT, peak emission
at 22:18 UT, and
- a C1.2 (N03E47) between 00:30 - 00:54 UT (on 12/31),
peak emission at 00:43 UT (on 12/31).
EIT 195 images show a brightening on the aforementioned
AR starting at 21:49 UT followed by a much stronger one
at 22.12 UT. An intensity disturbance (wave) is seen
developing by the time mainly toward N, S, and W of the
AR. The ejection of a filament to NE, N, S, and W of the
AR can be seen between ~ 22:24 - 22:36 UT.
In summary, the event has therefore been determined as
an asymmetric 'full' halo event, frontsided.
2004/12/31 (Friday)
07:31 UT E Limb Diffuse loop front discernible in the aftermath of
halo event reported to start at 22:30 UT on previous
day. Much outflow all across the eastern limb.
15:30 UT E Limb Big CME spanning in C2 all above the E Limb (as
projected on the plane of the sky) without clear
extensions. By 16:54 UT, C2 shows a ragged front just
appearing above the N Pole that spans later all above
the W Limb (it is difficult to say whether it is
related to the huge CME on E mentioned above). As for
C3, this latter front fades close to the inner edge.
On 2004/12/31, among multiple B- and C-class X-ray
flares, GOES reported an M1.2 X-ray flare (N04E38)
between 14:38 - 14:48 UT, with peak emission at 14:45
UT, followed by a C6.8 (N03E38) between 14:52 and 15:04
UT with peak emission at 14:59 UT. EIT 195 images show
a brightening on the aforementioned AR starting at
14:48 UT, clear signature of the M 1.2 X-ray flare. An
intensity disturbance (wave) can be seen developing
afterward mainly toward NW, W, S, and SE of the AR,
and by ~ 15:00 UT, a dimming region mainly to SW and S
of the AR.
21:54 UT S West Ragged loop front.
Web curator:
K.M.Schenk
NASA Goddard Space Flight Center
Solar Physics Branch / Code 682
Greenbelt, MD 20771