Dear RHESSI Collaborators,
Solar activity remains low with no activity above C-level over the
past 24 hours. The target region NOAA 11183 has undergone some minor
flux emergence but retains its beta configuration. Slight chance of an
isolated C-class flare.
The position of NOAA 11183Â on 2-Apr-2011 at 04:30 UT is:
N17W02, ( 32", 384" )
See http://www.SolarMonitor.org for images and
http://solar.physics.montana.edu/max_millennium/ops/observing.shtml
for a description of the current Max Millennium Observing Plan.
Regards,
Ryan Milligan (QUB)
Dear RHESSI Collaborators,
There have been several low C-class flares over the past 24 hours,
some from NOAA 11176, but the largest was a C3.4 flare from the target
region NOAA 11183 at 01:46 UT. We shall continue to monitor NOAA 11183
as it crosses the central meridian. Although the region has diminished
in size there is still a chance of one or two isolated low-level
events.
The position of NOAA 11183Â on 1-Apr-2011 at 04:30 UT is:
N15E11, ( -177", 352" )
See http://www.SolarMonitor.org for images and
http://solar.physics.montana.edu/max_millennium/ops/observing.shtml
for a description of the current Max Millennium Observing Plan.
Regards,
Ryan Milligan (QUB)
Dear RHESSI Collaborators,
Solar activity remains low. The target region NOAA 11183 was the
source of two C1 flares since the last message. The region retains its
beta configuration but has increased in size over the past 24 hours.
Chance for further isolated C-level events.
The position of NOAA 11183Â on 31-Mar-2011 at 04:30 UT is:
N15E24, ( -378", 345" )
See http://www.SolarMonitor.org for images and
http://solar.physics.montana.edu/max_millennium/ops/observing.shtml
for a description of the current Max Millennium Observing Plan.
Regards,
Ryan Milligan (QUB)
Dear RHESSI Collaborators,
The target region NOAA 11183 has remained quiescent over the past 24
hours, producing only a C1.2 flare at 21:21 UT on 29-Mar-2011. The
region has been down graded from a beta-gamma region to a beta region
but may still produce isolated low-level events.
The position of NOAA 11183Â on 30-Mar-2011 at 04:30 UT is:
N15E36, ( -547", 335" )
See http://www.SolarMonitor.org for images and
http://solar.physics.montana.edu/max_millennium/ops/observing.shtml
for a description of the current Max Millennium Observing Plan.
Regards,
Ryan Milligan (QUB)
Dear RHESSI Collaborators,
Solar activity remains low with NOAA 11176 continuing to decay. At
this time we shall switch the target region to NOAA 11183 in the
northeast quadrant. This region is now classified as a beta-gamma
region and has significantly increased in size over the past 24 hours,
producing a C1.1 flare at 05:11 UT in the process. Further C-level
activity expected if the region continues to develop.
The position of NOAA 11183Â on 29-Mar-2011 at 10:30 UT is:
N15E48, ( -691", 320" )
See http://www.SolarMonitor.org for images and
http://solar.physics.montana.edu/max_millennium/ops/observing.shtml
for a description of the current Max Millennium Observing Plan.
Regards,
Ryan Milligan (QUB)
Dear RHESSI Collaborators,
Solar activity remains low with NOAA 11176 continuing to decay. The
region comprises two positive polarity spots with trailing negative
polarity plage. Chance for an isolated low-level event as the region
crosses the central meridian.
The position of NOAA 11176Â on 28-Mar-2011 at 04:30 UT is:
S15W01, (16", -138" )
See http://www.SolarMonitor.org for images and
http://solar.physics.montana.edu/max_millennium/ops/observing.shtml
for a description of the current Max Millennium Observing Plan.
Regards,
Ryan Milligan (QUB)
Dear RHESSI Collaborators,
Solar activity has diminished as NOAA 11176 continues to decay. The
region was the source of a C3.1 flare since the last message. Chance
of an additional isolated C-class event over the next 24 hours.
The position of NOAA 11176Â on 27-Mar-2011 at 10:30 UTÂ is:
S16E10, ( -161", -156" )
See http://www.SolarMonitor.org for images and
http://solar.physics.montana.edu/max_millennium/ops/observing.shtml
for a description of the current Max Millennium Observing Plan.
Regards,
Ryan Milligan (QUB)
Dear RHESSI Collaborators,
Solar activity is at moderate levels. The target region NOAA 11176
retains its beta-gamma configuration and was the source of an isolated
M1.0 event at 23:08 UT on 25-Mar-2011. Further C-level activity
expected with chance for another isolated M-class flare.
The position of NOAA 11176Â on 26-Mar-2011 at 05:30 UT is:
S16E27, ( -421", -165" )
See http://www.SolarMonitor.org for images and
http://solar.physics.montana.edu/max_millennium/ops/observing.shtml
for a description of the current Max Millennium Observing Plan.
Regards,
Ryan Milligan (QUB)
Dear RHESSI Collaborators,
The level of solar activity is now medium. NOAA 11176 has decreased in
area but increased in number of spots while maintaining its beta-gamma
magnetic classification. This region has continued to produce several
C-class events and an M1.0 flare at 12:01 UT on 24-Mar-2011. Further
C-class activity is expected, with a chance of another M-class event.
The position of NOAA 11176 on 25-Mar-2011 at 11:30 UT is:
S16E38, ( -567", -176" )
See http://www.SolarMonitor.org for images and
http://solar.physics.montana.edu/max_millennium/ops/observing.shtml
for a description of the current Max Millennium Observing Plan.
Regards,
Shaun Bloomfield (Trinity College Dublin)
Dear RHESSI Collaborators,
Solar activity is at a low level. NOAA region 11176 has increased in area and
number of spots as it rotates further on-disk, being designated a beta-gamma
magnetic classification. This region has slowed in terms of numbers of flares,
producing only three B-class and a C1.1 flare since yesterday's M1.4 event at
02:03 UT. Further C-class activity is likely, with a small chance for
an M-class
event if the region undergoes a period of growth or fragmentation.
The position of NOAA 11176 on 24-Mar-2011 at 10:30 UT is:
S15E52, ( -737", -179" )
See http://www.SolarMonitor.org for images and
http://solar.physics.montana.edu/max_millennium/ops/observing.shtml
for a description of the current Max Millennium Observing Plan.
Regards,
Shaun Bloomfield (Trinity College Dublin)