
LASCO Activity Report for
July 11, 2005 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
On 2005/07/06, SOHO Telemetry Submode was changed to Submode 5 (support for
VAULT -Sounding Rocket Launch on 2005/07/07). Telemetry Submode will be
changed back to Submode 6 on 2005/07/08 at 15:00 UT.
During TM Submode 5, EIT 195 CME watch in half-res (512x512).
2005/07/08 (Friday)
07:27 UT N East Elongated loop front developing toward ENE.
07:27 UT ES East Slow development of a system of faint loops. Difficult
to give an exact time of first appearance.
12:26 UT E Limb Faint front developing slightly toward ESE (partly
superposed with the development of the system of faint
loops). It fades close to the inner edge of C3.
17:31 UT N Pole Extremely faint and diffuse front. Next C2 image
available (19:22 UT) shows a very faint expanding
system of loop-like fronts developing mainly toward N.
A bright ragged front is also developing toward W,
which does not form part of the partial halo under
analysis (se below). The partial halo event was first
seen in C3 at 19:42 UT above the N Pole. By 00:18 UT
(on 07/09) the event spans ~ 150 deg, from around PA
280 - 070. It is difficult to precise the limit on W,
as the faint halo event superposes there in the LOS
with the brighter limb event described above (see
also below). The mean plane-of-sky speed of the LE of
the partial halo event at PA ~ 3 was ~ 461 km/sec
(based only on the first four C3 frames, as the LE
becomes then barely discernible). GOES reported a long
duration C1.6 X-ray event on NOAA AR 10786 (N13W11)
between 15:40 - 17:19 UT with peak emission at 16:18 UT.
EIT 195 images show the development of a dimming region
to N of the AR 10786, starting at around 16:12 UT.
Please note that the Telemetry Submode changed from
Submode 5 to 6 by 15:00 UT and therefore the EIT 195
CME watch changed from half-res (512x512) to full-res
(1024x1024) by that time. Note that by 17:15 UT, a
barely backsided CME starts to be seen developing above
the WSW Limb. This signature likely corresponds to the
EIT counterpart of the ragged front seen in C2/C3 images
developing toward W mentioned above. In summary, the
event has therefore been determined as a very faint
partial halo CME, frontsided, associated with a long
duration C1.6 X-ray flare on NOAA AR 10786.
19:22 UT W Limb Bright ragged loop front. Some infalling material (see
previous event for some other details).
2005/07/09 (Saturday)
02:30 UT NN East Extremely faint expanding loop front. It fades close
to the inner edge of C3.
09:06 UT E Limb Small front.
13:31 UT S East Expanding 'half' loop fronts. They fade throughout C3.
13:31 UT W Limb Narrow and elongated front. It fades throughout C3.
21:54 UT EN East Bright loop-like front followed by a cavity and bright
inner core. See next event for some other details on
this event.
22:30 UT N West Wide and ragged loop front front. Faint and diffuse
extensions all above both poles can also be discerned.
By 23:06 UT, the C2 occulting disk is already completely
covered. Note that the development of a typical 3-part
structure CME can be seen on ENE since 21:54 UT
(previous entry). Signatures of the halo event were
first seen in C3 at 23:18 UT all above the W Limb. A
very faint and diffuse front can be seen ahead (shock?)
spanning all above the N Pole. The C3 occulting disk is
completely covered by 23:42 UT. The mean plane-of-sky
speed of the LE of the halo CME (where the intensity
gradient is maximum) at PA ~ 306 is around 1140 km/sec,
showing practically no acceleration (based on C3 data).
GOES reported an M2.8 X-ray flare on NOAA AR 10786
(N12W28) between 21:47 - 22:19 UT with peak emission
at 22:06 UT. Note also the occurrence of a C1.5 X-ray
flare on NOAA AR 10789 (N17E15) between 20:23 - 21:01
UT with peak emission at 20:45 UT preceded by a B5.8
X-ray flare on the same AR 10789 that peaked at 19:38
UT. EIT 195 images show a small brightening on AR 10789
starting at 20:36 UT with the formation of a dimming
region toward NE of the AR afterward. The eruption of
at least part of a filament on NE can be seen more or
less coincident with the development of the dimming.
The EIT events just described are most likely related
to the X-ray activity reported by GOES on NOAA AR 10789
(and seem to be the EIT counterpart of the 3-part
structure CME seen by the LASCO coronagraphs). Later,
at 22:00 UT, a strong brightening can be seen on AR
10786 followed by the formation of a dimming toward NW,
N, and NE of the AR. Corresponding running difference
EIT 195 images show a strong intensity disturbance
developing radially away of the AR, mainly toward N.
The bulk of the material ejected seems to develop mainly
toward NW. These EIT events are related to the M2.8
X-ray flare on AR 10786. In summary, the event has
therefore been determined as an asymmetric full halo
event, frontsided, associated with an M2.8 X-ray flare
on NOAA AR 10786.
2005/07/10 (Sunday)
06:06 UT W Limb Diffuse front. Developing missed in following data gap.
06:54 - 20:58 UT Temporary Data Gap.
NOTE:
GOES reported a C9.9 X-ray flare on NOAA AR 10783 (N00W90) between 15:08 -
15:20 UT with peak emission at 15:16 UT.
23:06 UT W Limb Bright loop front with twisted inner structure. Much
gusty outflow afterward.
2005/07/11 (Monday)
00:30 UT W Limb Just after the event reported to start at 23:06 UT,
an apparently new bright and ragged front appears.
05:30 UT WN West Initially bright and relatively small loop front.
06:54 UT W Limb Initially bright and relatively small loop front that
quickly fades. Gusty outflow continues on W.
13:54 UT WN West Another initially bright and relatively small loop
front.
Time of the last C2 image analyzed: 16:30 UT.
Web curator:
K.M.Schenk
NASA Goddard Space Flight Center
Solar Physics Branch / Code 682
Greenbelt, MD 20771