
LASCO Activity Report for
September 11, 2006 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
KEYHOLE Operations:
-------------------
2006/08/21 - 2006/09/19 : 26 m Keyhole
2006/08/28 - 2006/09/13 : 34 m Keyhole
- LASCO safed for maneuvers (SK and MM) on 09/05 @ 18:00 UT.
LASCO recovery expected for late on 09/07; therefore,
observations started on 09/07 @ ~ 22:00 UT.
- Spacecraft Maneuvers (Station Keeping and Momentum Management,
not roll) on 09/06.
- 2006/08/19 - 2006/09/16 : EIT CCD Bakeout
- At least until next S/C maneuvers (scheduled for 09/06),
LASCO will NOT be recorded during DSN gaps (starting on 08/28,
until 09/16).
- 12 minutes cadence for C2 during Keyhole (only during contact
periods since 08/28, which are sparse...).
2006/09/08 (Friday)
00:12 UT WN West A bright loop front (development missed in the
next data gap). By 04:24 UT the loop front is close
to the outer edge of C2. It appears surrounded by a
fainter and much wider front spanning all across
the western hemisphere up to past the S Pole. Just
before the second data gap, the C2 occulter seems
to be surrounded, though the signal on E is barely
discernible and only very close to the occulting
disk. More faint wide loop fronts continue appearing
on W. Only one C3 frame (05:18 UT) shows something
of the event. Though the event covers a big angle
in the western hemisphere, the S Pole is not crossed
by that time. Afterwards, there is another data gap,
so nothing else can be said. After this second gap,
C2 shows a loop front already developing on WSW.
Very faint and diffuse loop-like extensions seems
to be developing above the S Pole. C3 shows no
remnant signatures of any Halo event. No EIT images
are available due to EIT CCD bakeout (the bakeout
will last until 09/16). GOES recorded a couple of
short duration B-class X-ray flares on NOAA AR 10909
during the time of the first LASCO data gap: i) a
B4.4 on S07E06 between 01:30 UT - 01:47 UT with peak
emission at 01:39 UT, and ii) a B3.3 on S07E05
between 02:34 - 02:45 UT with peak emission at
02:39 UT. And then during the second data gap, it
recorded a B5.6 on the same AR (S06E01) between
10:13 - 11:46 UT with peak emission at 10:58 UT. In
summary, an apparently faint and asymmetric Halo
Event was observed by LASCO C2. It is hard to say
whether the different structures mentioned above
belong to a unique event. It seems to exist a
temporal correlation between the activity on AR
10909 and the faint and diffuse wide loop-like
extensions aforementioned.
LASCO data gap between 00:12 - 04:12 UT.
LASCO data gap between 05:14 - 14:24 UT.
LASCO data gap between 16:36 - 23:36 UT.
23:36 UT S East System of faint loops already under development after
data gap.
2006/09/09 (Saturday)
LASCO data gap between 00:00 - 07:24 UT.
07:24 UT S East Development of faint system of loops continues (LE
already past the outer edge of C2). A faint twisted
structure develops behind.
LASCO data gap between 13:00 - 20:57 UT.
2006/09/10 (Sunday)
LASCO data gap between 00:24 - 07:12 UT.
LASCO data gap between 10:12 - 23:12 UT.
23:12 UT E Limb Faint ragged front already under development after
data gap.
2006/09/11 (Monday)
See Report named "obs20060915.html".
Web curator:
K.M.Schenk
NASA Goddard Space Flight Center
Solar Physics Branch / Code 682
Greenbelt, MD 20771