MM#009 Default Target
Dear Collaborators,
The current visible solar disk is spotless, plageless, and
does not have any noteworthy filaments or prominences.
Target region NOAA 2741 is now well beyond the
northwestern limb. There is no default target region
available. The quiet Sun conditions are expected to
continue for the next 24 hour period.
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,
Bill Marquette (Helio Research)
MM#009 Default Target
Dear Collaborators,
Solar flare activity is extremely low. The current
visible solar disk is spotless and plageless. Target
region NOAA 2741 is now located beyond the
northwestern limb where faint prominence material
associated with the region is still visible. No
significant solar flare activity expected anytime soon.
The position of NOAA 2741 on May 20 at 13:30 UT is:
N05W91 (Solar X = 944", Solar Y = 081")
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,
Bill Marquette (Helio Research)
Dear Collaborators,
Solar activity remains at very low levels. NOAA 12741 has been
quiescent since the last message and the ERF in the northwest quadrant
has already decayed. NOAA 12741 is now on the western limb and shall
remain the target region for a further 24 hours. No change in activity
expected at this time.
The position of NOAA 12741 on 19-May-2019 at 13:30 UT is:
N05W91, ( 944", 81" )
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 (University of Glasgow)
Dear Collaborators,
Quiet-Sun conditions continue. NOAA 12741 has been quiescent since the
last message despite producing a filament eruption from the western
limb. There is also a small, emerging flux region in the northwest
quadrant that might bring some low-level activity over the next few
days. However, NOAA 12741 shall remain the target region for a further
24 hours, and may produce an isolated low-level event before west limb
passage.
The position of NOAA 12741 on 8-May-2019 at 13:30 UT is:
N05W78, ( 924", 90" )
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 (University of Glasgow)
Dear Collaborators,
Solar X-ray flux has remained at background levels since the last
message. NOAA 12741 has remained quiescent and retains its alpha
configuration as it approaches the western limb. Slight possibility of
an isolated low-level event over the next 24 hours.
The position of NOAA 12741 on 17-May-2019 at 13:00 UT is:
N05W65, ( 857", 99" )
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 (University of Glasgow)
Dear Collaborators,
The target region NOAA 12741 has continued to produce B-level activity
since the last message, as well as a C2.0 flare at 19:15 UT yesterday.
The region itself remains unchanged in terms of size and complexity,
but may produce additional low-level events over the next 24 hours.
The position of NOAA 12741 on 6-May-2019 at 13:00 UT is:
N05W52, ( 746", 108" )
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 (University of Glasgow)
Dear Collaborators,
The target region NOAA 12741 remains unchanged since the last message,
and still maintains a large overarching filament. The region produced
a B3.5 flare at 08:32 UT today. Additional isolated low-levels events
still possible over the next 24 hours.
The position of NOAA 12741 on 15-May-2019 at 13:00 UT is:
N06W38, ( 582", 134" )
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 (University of Glasgow)
Dear Collaborators,
The target region NOAA 12741 was the source of another long-duration
B-class flare since the last message. The B3.5 flare was associated
with strong coronal dimming, indicating a possible CME eruption. The
region itself is showing signs of decay and retains its alpha
configuration. The chance persists for an additional isolated
low-level event over the next 24 hours.
The position of NOAA 12741 on 14-May-2019 at 07:30 UT is:
N05W20, ( 324", 126" )
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 (University of Glasgow)
Dear Collaborators,
NOAA 12741 was the source of a long duration B2.2/B3.7 flare at 19:15
UT yesterday, in association with a filament eruption to the
southwest. The region retains its alpha configuration and shall remain
the target region. Slight chance of an additional isolated B-class
flare over the next 24 hours.
The position of NOAA 12741 on 13-May-2019 at 13:00 UT is:
N06W10, ( 164", 146" )
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 (University of Glasgow)
MM#009 Default Target
Dear Collaborators,
Solar flare activity was very low during the past 24
hours. Target region NOAA 2740 continues to
decay and was quiescent. The target will switch
to NOAA 2741. The curved filament located south
and west of 2741 became active and the southern
portion erupted. B-class events possible in the next
24 hour period.
The position of NOAA 2741 on May 12 at 12:45 UT is:
N06E06 Solar X = -099", Solar Y = 149")
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,
Bill Marquette (Helio Research)