Dear Collaborators,
Solar activity continues at an extremely low level with
no sunspots on the visible solar disk at present. The
target region still shows some overlying loops above the
limb. We will watch this region for a further 24 hours.
No significant activities are likely in the following
24-hour period.
The approximate position of the target on February 10 at 20:30 UT is:
S35W90 (890", -520")
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,
Ying Li (Purple Mountain Observatory)
Dear Collaborators,
The level of solar activity is extremely low. The target region
is rotating up to the South West limb, so foreshortening effects
prevent us knowing if it still has some pores or immature spots.
No flares have occurred since the last message, but this region
will remain the target until its compact EUV loop structure has
fully rotated over the limb. An isolated low B-class flare is
possible over the following 24 hours.
The approximate position of this region on 9-Feb-2020 at 17:00 UT is:
S32W86, ( 823", -506" )
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 is at a very low level. The unnumbered target region
appears to have ceased emerging and has lost some of its small spots
since the last message, but retains at least one pore in its trailing
flux portion. An isolated low B-class flare is possible in the next
24-hour period.
The approximate position of this region on 8-Feb-2020 at 14:00 UT is:
S32W72, ( 786", -484" )
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 is very low. A new magnetic flux region is
in the process of emerging in the South West quadrant. This region has
already developed small sunspots and was the source of a B1.0 flare on
7-Feb-2020 at 18:22 UT. Additional B-class flares are possible over the
following 24 hours.
The approximate position of this region on 7-Feb-2020 at 20:30 UT is:
S32W63, ( 737", -471" )
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 is at an extremely low level. The visible disk remains
spotless, with no X-ray flares having occurred since the last message.
The target switches to a dynamic prominence on the North West limb. No
change in flare activity is expected in the next 24-hour period.
The approximate position of this region on 6-Feb-2020 at 22:00 UT is:
N30W90, ( 842", 483" )
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 is extremely low. The solar disk
continues to be devoid of spots, while no significant X-ray
flares have occurred since the last message. The target small
coronal loop system has rotated onto the disk and appears to
be rooted in an enhanced network region. This will remain the
target for another 24 hours, with no change in flare activity
expected.
The approximate position of this region on 5-Feb-2020 at 23:00 UT is:
N12E70, ( -895", 237" )
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 is at an extremely low level. The visible disk
remains spotless and no X-ray flares have occurred in the past
24 hours. A small, EUV-bright coronal loop system is currently
rotating over the North East limb and becomes the new target.
No change in flaring activity is expected over the following
24-hour period.
The approximate position of this region on 4-Feb-2020 at 18:00 UT is:
N12E90, ( -951", 201" )
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 is extremely low. There are no sunspots
on the visible disk now that NOAA 12757 has completed its West-limb
transit. No X-ray flares have occurred since the last message. The
target region for the next 24 hours becomes a dynamic prominence on
the North West limb. No change in flare activity is expected during
the next 24 hours.
The approximate position of this region on 3-Feb-2020 at 16:30 UT is:
N45W90, ( 688", 684" )
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 single alpha sunspot in the leading portion
of target region NOAA 2757 has completed west
limb passage. The visible solar disk is now spotless.
2757 was the source of a limb occulted A9.6 event
at 02/02/05:44 UT. 2757 will continue to be the
default target today. No significant solar flare events
expected in the next 24 hour period.
The position of NOAA 2757 on February 02 at 14:30 UT is:
N03W91 (Solar X = 971", Solar Y = 048")
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,
Target region NOAA 2757 continues to slowly decay.
2757 was the source of a minor B1.4 event at
01/31/15:01 UT. The short active filament located
just south and east of the leading sunspot has
disappeared since the last message. No significant
solar flare activity expected in the next 24 hour period.
The position of NOAA 2757 on February 01 at 13:30 UT is:
N03W74 (Solar X = 936", Solar Y = 079")
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)