Dear Collaborators,
The level of solar activity continues to be extremely low. The spotless
plage that is the target region is now rotating over the South West limb.
No X-ray flares have occurred since the last message, with no in flaring
activity expected in the next 24-hour period.
The approximate position of this region on 17-Mar-2020 at 16:00 UT is:
S30W90 , ( 835", -478" )
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 (Northumbria University)
Dear Collaborators,
Solar activity remains at an extremely low level. The target
spotless plage region is rotating up to the South West limb.
No X-ray flares have occurred since the last message, and no
in flaring activity is expected over the following 24 hours.
The approximate position of this region on 16-Mar-2020 at 21:00 UT is:
S30W82 , ( 827", -464" )
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 (Northumbria University)
MM#009 Default Target
Dear Collaborators,
The visible solar disk is spotless. The target region
NOAA 2758 is a slowly decaying spotless Cycle 25
plage. No significant solar flare activity expected
in the next 24 hour period.
The position of NOAA 2758 on March 15 at 13:30 UT is:
S33W54 (Solar X = 656", Solar Y = -463")
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,
The visible solar disk is spotless. Target region NOAA 2758
is a stable spotless plage. 2758 is mostly unchanged
and quiescent in the past 24 hours. No change in solar
flare activity expected in the next 24 hour period.
The position of NOAA 2758 on March 14 at 13:30 UT is:
S33W42 (Solar X =543", Solar Y = -448")
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 continues at very low levels. NOAA 12758 has remained
quiescent and unchanged since the last message, but shall continue to
be the target region. No change in activity expected over the next 24
hours.
The position of NOAA 12758 on 3-Mar-2020 at 08:30 UT is:
S30W34, ( 468", -393" )
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 (Queen's University Belfast)
Dear Collaborators,
Solar X-ray flux remains at background levels. NOAA 12758 has remained
quiescent since the last message and continues to decay. It shall
continue to be the target region although no change in activity is
expected over the next 24 hours.
The position of NOAA 12758 on 12-Mar-2020 at 08:30 UT is:
S30W20, ( 287", -381" )
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 (Queen's University Belfast)
Dear Collaborators,
NOAA 12758 has continued to decay since the last message and is now
completely spotless. However it did produce a B2.3 flare at around
06:00 UT today. It shall remain the target region for another 24 hours
with a slight chance of an additional isolated, low-level event.
The position of NOAA 12758 on 11-Mar-2020 at 08:30 UT is:
S30W06, ( 87", -375" )
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 (Queen's University Belfast)
Dear Collaborators,
Quiet-Sun conditions continue. NOAA 12758 has remained quiescent since
the last message. It has decayed significantly over the past 24 hours
and is now classified as an alpha region with a single negative
polarity pore. The underlying plage region shall continue to be the
target with no change in activity expected.
The position of NOAA 12758 on 10-Mar-2020 at 08:30 UT is:
S30E07, ( -102", -376" )
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 (Queen's University Belfast)
Dear Collaborators,
Solar activity continues at extremely low levels. The target region in
the southeast quadrant is now designated as NOAA 12758. It is
classified as a beta/C-type active region, although its trailing spots
have decayed significantly since the last message. It will continue to
be the target region although no significant change in activity is
expected over the next 24 hours.
The position of NOAA 12758 on 9-Mar-2020 at 08:30 UT is:
S29E21, ( -303", -366" )
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 (Queen's University Belfast)
Dear Collaborators,
The level of solar activity continues to be extremely low. The newly
emerged magnetic flux region in the South East quadrant (that is the
current target) has grown in number of spots, spot area, and also now
developed a rudimentary penumbra on its leading spot. This region has
been the source of several A-class flares since the previous message.
An isolated B-class flare is possible in the following 24-hour period
if this region continues to emerge new flux.
The approximate position of this region on 8-Mar-2020 at 16:30 UT is:
S29E32 , ( -448", -376" )
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 (Northumbria University)