Dear Collaborators,
Solar activity continues at a very low level. The visible solar
disk remains spotless. It is worth mentioning that the filament
in the target plage region erupted around 00:30 UT today,
producing a very weak two-ribbon flare and being associated
with a weak CME. The target plage is rotating to the west limb.
No significant activities are likely in the next 24 hours.
The approximate position of the target on February 24 at 14:30 UT is:
N09W58 (780", 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,
Ying Li (Purple Mountain Observatory)
Dear Collaborators,
Solar activity continues at extremely low levels. The visible solar disk remain
spotless. No flares occurred in the past 24 hours. The filament rooted in the
target plage region has gradually disappeared. Quiet-Sun conditions should
continue in the following 24 hours.
The approximate position of the target region on February 23 at 14:30 UT is:
N07W46 (640", 180")
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,
Solar activity continues at a very low level with no flares occurring on the
spotless solar disk in the past 24 hours. The target plage region retains its
filament channel and the filament shows some oscillations. Only very minor
activities are likely in the next 24 hours.
The approximate position of the target region on February 22 at 14:30 UT is:
N07W32 (500", 200")
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,
Solar activity continues at an extremely low level. No flares occurred on
the spotless solar disk in the past 24 hours. The target plage region retains
its filament channel. The filament shows some oscillations. Only very minor
activities are possible in the next 24 hours.
The approximate position of the target region on February 21 at 14:30 UT is:
N07W18 (290", 210")
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 visible solar disk remains spotless. Only an A9.7 occurred in
the past 24 hours, which was produced by the target plage region.
The target plage region retains its filament channel. Only very minor
activities are likely in the following 24 hours.
The approximate position of the target region on February 20 at 20:30 UT is:
N07W09 (100", 200”)
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,
Solar activity continues at a very low level. Only an A1.4 event
occurred in the past 24 hours, which was produced by the target
plage region. The target plage region retains its filament channel.
Only very minor activities are possible in the following 24 hours.
The approximate position of the target region on February 19 at 14:30 UT is:
N07E09 (-100", 200”)
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,
Solar activity has been at extremely low levels with the solar disk
remaining spotless. No noteworthy events occurred in the past 24
hours. The target plage region retains its filament channel and some
parts of the filament are oscillating. Only very minor activities are
possible in the next 24 hours.
The approximate position of the target region on February 18 at 14:30 UT is:
N05E20 (-290", 210")
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,
Quiet-Sun conditions continue. The target plage region has remained
quiescent and unchanged since the last message and retains its
filament channel. Slight chance for an isolated low-level event over
the next 24 hours.
The approximate position of the target region on 17-Feb-2019 at 14:30 UT is:
N05E35, ( -554", 180" )
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 Collaborators,
Solar activity remains at very low levels. The target plage region in
the northeast quadrant remains unchanged since the last message, and
it retains a filament channel along its magnetic neutral line. Chance
for some isolated activity over the next 24 hours if the filament
erupts.
The approximate position of the target region on 16-Feb-2019 at 14:30 UT is:
N05E47, ( -707", 164" )
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 Collaborators,
The visible solar disk remains spotless. The bipolar plage region in
the northeast quadrant has remained quiescent since the last message.
The region appears to have a low-lying filament along its magnetic
neutral line, which may produce some isolated activity if it erupts.
The approximate position of the target region on 15-Feb-2019 at 14:30 UT is:
N05E60, ( -839", 142" )
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)