Dear Collaborators,
Solar activity continues at background levels. Yesterday's target
region has decayed completely, but a new bipolar region is currently
emerging at low latitudes that shall be the new target region. Low
probability of any increase in activity over the next 24 hours.
The position of the target region on 24-Mar-2020 at 14:30 UT is:
N08W39, ( 596", 223" )
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. Since the last
message, a small emerging flux region has appeared at high latitudes
but may already be beginning to decay. The region is spotless and
unnumbered but shall be the new target region for the next 24 hours.
No change in activity expected at this time.
The approximate position of the target region on 23-Mar-2020 at 08:30 UT is:
N26W21, ( 304", 518" )
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
target in the North East quadrant decayed further and has now
merged into the quiet Sun. The target becomes a new moderately
dynamic prominence on the North West limb. No X-ray flares have
occurred since the last message, and no change is expected in
flaring activity in the next 24-hour period.
The approximate position of this region on 22-Mar-2020 at 17:00 UT is:
N40W90 , ( 737", 614" )
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 region
in the North East quadrant has decayed to enhanced network over the
previous 24 hours. No significant X-ray flares have occurred and no
change in flaring activity is expected over the following 24 hours.
The approximate position of this region on 21-Mar-2020 at 18:00 UT is:
N26E02 , ( -30", 526" )
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,
The level of solar activity continues to be extremely low. The small
target magnetic flux region in the North East quadrant has lost its
pores in the past 24 hours. No significant X-ray flares have occurred
since the last message, and no change in flaring activity is expected
in the next 24-hour period.
The approximate position of this region on 19-Mar-2020 at 17:00 UT is:
N26E29 , ( -422", 514" )
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 previous target
has now fully rotated over the South West limb. A small magnetic flux
region with very small pores has emerged in the North East quadrant.
No X-ray flares have occurred since the last message, with no change
in flaring activity expected over the following 24 hours.
The approximate position of this region on 18-Mar-2020 at 17:00 UT is:
N26E42 , ( -581", 500" )
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,
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)