Dear RHESSI Collaborators,
The visible solar disk continues to show no spots, with no flaring
activity having occurred in the past 24-hour period. The North East
quadrant's decaying plage region remains the target. No changes are
expected in flaring activity over the following 24 hours.
The approximate position of the target region on 7-Nov-2017 at 16:00 UT is:
N09E16, ( -264", 93" )
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 RHESSI Collaborators,
The solar disk remains devoid of spots. No significant activity has
occurred since the last message, with the background soft X-ray flux
remaining below the A5 level. The decaying plage region in the North
East quadrant continues to be the target region. There is no expected
increase in flaring activity over the next 24 hours.
The approximate position of the target region on 6-Nov-2017 at 16:30 UT is:
N09E29, ( -465", 96" )
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 RHESSI Collaborators,
The visible solar disk is now spotless. The decaying plage region in
the northeast quadrant has remained quiescent but shall continue to be
the target region for a further 24 hours. No increase in activity is
expected.
The approximate position of the target region on 5-Nov-2017 at 12:30 UT is:
N09E45, (-683", 106")
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 RHESSI Collaborators,
Solar activity remains at background levels. The bright, compact
region close to the eastern limb appears spotless, and therefore
unnumbered. The underlying plage shall continue to be the target
region although it shows little sign of producing any activity over
the next 24 hours.
The approximate position of NOAA 12685 on 4-Nov-2017 at 12:30 UT is:
N09E59, ( -819", 117" )
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 RHESSI Collaborators,
Solar activity remains at very low levels with NOAA 12685 now behind
the western limb. The associated filament erupted without any
significant flaring. The new target region shall be the compact,
dynamic region near the eastern equatorial limb. Slight chance for an
isolated low-level event.
The approximate position of the target region on 3-Nov-2017 at 14:30 UT is:
N10E79, (-936", 155")
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 RHESSI Collaborators,
The remnants of NOAA 12685 are now on the western limb. The region
remains quiescent but is still flanked by a long filament channel. Any
additional activity before west limb passage is highly unlikely but it
shall remain the target region for a further 24 hours.
The position of NOAA 12685 on 2-Nov-2017 at 08:30 UT is:
S09W82, ( 945", -160" )
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 RHESSI Collaborators,
Solar activity remains at very low levels. The sunspot associated with
NOAA 12685 has decayed completely as the region as approaches the
western limb. The filament channel remains visible between the
positive and negative plage regions, and shall continue to be the
target region for a further 24 hours. No increase in activity expected
unless the filament erupts.
The position of NOAA 12685 on 1-Nov-2017 at 12:30 UT is:
S09W70, ( 898", -175" )
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 RHESSI Collaborators,
Solar activity remains unchanged since the last message, with X-ray
flux still below the B1 level. NOAA 12685 has all but decayed, and the
remaining plage shall be the target region for a further 24 hours. No
increase in activity expected at this time.
The position of NOAA 12685 on 31-Oct-2017 at 14:30 UT is:
S09W58, ( 811", -190" )
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 RHESSI Collaborators,
Solar X-ray flux remains constant below the B1 level. There has been
no activity since the last message. Both active regions retain their
alpha configuration and NOAA 12685 shall continue to be the target
region. No increase in activity is expected over the next 24 hours.
The position of NOAA 12685 on 30-Oct-2017 at 12:30 UT is:
S09W41, ( 627", -208" )
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 RHESSI Collaborators,
Solar activity remains at very low levels. The two alpha regions on
the visible disk have areas of just 10uh each. NOAA 12685 shall
continue to be the target region although no change in activity is
expected at this time.
The position of NOAA 12685 on 29-Oct-2017 at 08:30 UT is:
S08W27, ( 435", -203" )
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)