Dear RHESSI Collaborators,
Solar conditions remain unchanged. The spotless region along the
western equator has remained quiescent since the last message. It
shall continue to be the target region for the next 24 hours although
no significant change in activity is expected at this time.
The approximate position of the target region on 17-Jul-2018 at 16:10 UT is:
N07W38, ( 583", 56" )
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 has remained at very low levels since the message, with
solar X-ray flux around the mid A-level. The plage region along the
western equator associated with an active region remnant shall
continue to be the target region, with only a slight change of an
isolated low-level event over the next 24 hours.
The approximate position of the target region on 16-Jul-2018 at 07:10 UT is:
N07W20, ( 329", 47" )
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 level of solar activity is extremely low. The visible solar disk
continues to be spotless. The target plage region was the source of
two B-class events since the last message, the largest being a B1.5
flare on 15-Jul-2018 at 08:39 UT. Low B-class flares are possible in
the following 24-hour period.
The approximate position of this region on 15-Jul-2018 at 14:00 UT is:
N05W10, ( 164", 12" )
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,
Solar activity is at an extremely low level. No spots are visible on
the solar disk and there have been no flares since the last message.
An isolated low B-class flare is a remote possibility from the target
plage region over the next 24 hours.
The approximate position of this region on 14-Jul-2018 at 12:00 UT is:
N05E04, ( -65", 13" )
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 level of solar activity is extremely low. Spotless conditions
continue on the visible disk. No flares have occurred in the past
24 hours. B-class flares might be possible from the target plage
region in the following 24-hour period.
The approximate position of this region on 13-Jul-2018 at 10:00 UT is:
N05E19, ( -307", 18" )
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,
Solar activity is at an extremely low level. The visible solar disk
remains devoid of spots. No flares have occurred in the previous 24
hours. Low B-class flares are possible from the target plage region
over the next 24 hours.
The approximate position of this region on 12-Jul-2018 at 12:00 UT is:
N05E31, ( -486", 25" )
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 level of solar activity is extremely low. Spotless conditions
continue on the visible solar disk. No flares have occurred since
the last message. Low B-class flares are possible from the target
plage region in the following 24-hour period.
The approximate position of this region on 11-Jul-2018 at 12:00 UT is:
N05E44, ( -654", 35" )
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,
Solar activity is at an extremely low level. The solar disk remains
spotless, so the target will continue to be the plage region in the
North East quadrant. No flares have occurred since the last message.
B-class flares are possible over the next 24 hours with a very small
chance of a low C-class flare.
The approximate position of this region on 10-Jul-2018 at 10:00 UT is:
N05E58, ( -799", 49" )
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 level of solar activity is extremely low. The target region has
rotated further onto the visible disk, revealing that this region
harbours no spots. No flares have occurred since the last message.
B-class flares are possible over the following 24-hour period with
a small chance of another low C-class flare.
The approximate position of this region on 9-Jul-2018 at 13:00 UT is:
N05E72, ( -895", 63" )
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 target region on the eastern limb has remained quiescent since the
last message, producing only a few B1 level events. The region remains
unnumbered and unclassified but may produce further low-level
activity, and possibly another isolated C-class flare, over the next
24 hours.
The approximate position of the target region on 8-Jul-2018 at 14:33 UT is:
N04E80, ( -926", 55" )
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)