Dear RHESSI Collaborators,
The solar disk remains spotless and no flares have occurred
in the past 24 hours. The small North East quadrant bipolar
flux region has continued to display bright EUV emission. No
increase in flaring activity is expected over the following
24-hour perios.
The approximate position of the target region on 11-Nov-2017 at 22:30 UT is:
N13E50, ( -725", 184" )
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,
There continues to be no spots on the visible solar disk and the
previous 24 hours have had no flares. A small bipolar flux region
has emerged in the North East quadrant and developed reasonably
bright EUV emission. No significant increase in flaring activity
is likely in the next 24 hours.
The approximate position of the target region on 10-Nov-2017 at 19:30 UT is:
N13E65, ( -856", 195" )
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 spotless and the no flares have occurred in
the past 24 hours. The target East-limb prominence has been mildly
dynamic since the last message, producing some minor surges in its
southern portion. No change in flaring activity is expected in the
following 24 hours.
The approximate position of the target region on 9-Nov-2017 at 16:30 UT is:
S06E90, ( -963", -101" )
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,
There continues to be no spots on the solar disk and the previous
24 hours have produced no flares. The target will be an East-limb
prominence, with no change in flaring activity expected over the
next 24-hour period.
The approximate position of the target region on 8-Nov-2017 at 22:30 UT is:
S03E90, ( -967", -51" )
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 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)