
LASCO Activity Report for
December 02, 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
SOHO Telemetry Submode changed back to Submode 5 on 2004/12/01 @ ~ 19:00 UT.
EIT 195 CME watch at half resolution (512x512) since then.
After the EIT Shutterles Campaign and while in Submode 6, EIT 195 CME
watch at full resolution (1024x1024).
SOHO Telemetry Submode changed to Submode 6 at 14:00 UT on 2004/11/30
(EIT Shutterless Campaign between 17:00 - 19:40 UT). It will be back
to Submode 5 on 2004/12/01 at 19:00 UT.
SOHO is in Telemetry Submode 5 since 2004/11/08 @ 22:15 UT. While in
Submode 5, half resolution EIT 195 CME watch (512x512).
2004/12/01 (Wednesday)
02:29 UT S West Faint asymmetric front.
04:53 UT NN East Jet-like front.
07:53 UT NN East At least three different features can be guessed at this
time: i) a diffuse ragged front that will develop mainly
toward NE-NNE, ii) a wide and ragged loop front that
extends up to above the N Pole, (just appearing at this
time), and iii) a bright front also just appearing on
ENE that will develop as a relative narrow loop (as
compared to the other two features). Both, the feature
described in i) and the one in iii) are first seen in
the C3 FOV at 08:18 UT, while the wide loop in ii) is
first seen in C3, all above the N Pole, by 09:18 UT.
The total angular spans by 10:42 UT is about 180 deg
(C3), form PA ~ 270 - 090, and it matches apparently
the angular span of the wide loop front [ii)]. The mean
plane-of-sky speed of the LE of the different features
observed is given below (based on C3 data):
Feature i) : PA 036 --> 742 km/sec
Feature ii) : PA 342 --> 326 km/sec
Feature iii): PA 073 --> 731 km/sec
GOES recorded an M1.1 X-ray flare from NOAA AR 10708
(N09E19) between 07:00 - 07:41 UT with peak emission at
07:20 UT, most likely associated to at least one of the
features described above. EIT 195 images show a strong
brightening on NOAA AR 10708 at 07:13 UT, followed by a
rather circular intensity disturbance traveling away
from the AR. In summary, the event has therefore been
determined as a complex partial halo event, frontsided.
But keep in mind that several features contribute to
the overall morphology of the event.
18:29 UT NN West Faint loop front preceded by the development of an
apparent system of faint loops. By 19:27 UT, an elongated
feature develops at roughly the central PA of the loop
front. As it develops it shows up as a blob-like front.
A similar one at 22:06 UT (a little bit fainter).
2004/12/02 (Thursday)
01:27 UT EN West Faint ragged front accompanied to N by a narrow front
moving apparently a little bit faster. By 02:50 UT, on
NNW, a couple of blob-like fronts start to be discerned.
They all fade throughout C3. Gusty outflow follows on
NNW in the form of small blobs.
07:50 UT N Pole Very faint and raged front developing slightly toward
NNE. It fades throughout C3. By 08:50 UT a very narrow
loop-like feature (jet-like) is seen at roughly the PA
of its southern leg. And by 09:26 UT another faint and
ragged loop front can be seen above the N Pole.
Web curator:
K.M.Schenk
NASA Goddard Space Flight Center
Solar Physics Branch / Code 682
Greenbelt, MD 20771