Dear RHESSI Collaborators,
Solar activity continues at very low levels. Yesterday's target
region has now designated as NOAA 12723 with a beta/B-type
sunspot group. This region is emerging magnetic flux. Minor
activity is likely in the following 24 hours.
The position of NOAA 12723 on September 30 at 07:10 UT is:
S08W05 (83", -244")
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 RHESSI Collaborators,
The level of solar activity is extremely low. The visible solar disk remains
spotless. Only some very small scale EUV brightenings show up. Today
we will watch one of the brightenings close to the central meridian. small
EUV jets are possible in the next 24 hours.
The approximate position of the target on September 29 at 07:10 UT is:
S10E10 (-120", -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 RHESSI Collaborators,
Solar activity continues at a background level and the visible solar disk
remains spotless. There show up some small brightenings within the
target coronal hole. No flaring activity is expected in the next 24 hours.
The approximate position of the target on September 28 at 07:10 UT is:
S01E41 (-600", -95")
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 RHESSI Collaborators,
Solar activity remains at a background level. No noteworthy events
occurred on the spotless disk. Yesterday's target prominence/filament
seems to disappear. Today we will watch a small "coronal hole" in the
southeastern quadrant that is close to the equator. Some bright emissions
(especially in AIA 193) show up. No flaring activity is likely in the following
24 hours.
The approximate position of the target on September 27 at 07:10 UT is:
S02E58 (-760", -90”)
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 RHESSI Collaborators,
Solar activity continues at extremely low levels. The visible solar disk
remains spotless. The target prominence/filament shows some swirling
motions and appears to erupt some plasma. Today we will continue to
watch this target. No significant activity is expected in the next 24 hours.
The approximate position of the target on September 26 at 07:10 UT is:
N44E80 (-600", 650")
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 RHESSI Collaborators,
Solar activity remains at an extremely low level. The visible solar disk is
very clean. Yesterday's target (a plage region) has rotated beyond the
west limb. Today we will switch to a limb prominence/filament, which is
rotating onto the disk. A cavity appears to form at the limb. No significant
activity is expected in the next 24 hours.
The approximate position of the target on September 25 at 07:10 UT is:
N44E90 (-650", 650")
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 RHESSI Collaborators,
Solar activity continues at extremely low levels with the GOES soft
X-ray flux being flat at ~A3. The visible solar disk is featureless, no
spots or filaments. The decaying plage region shall remain the target
for a further 24 hours although no flaring activity is expected.
The approximate position of the target region on September 24 at 07:10 UT is:
N08W75 (910", 90")
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 RHESSI Collaborators,
Solar activity remains at very low levels. The decaying plage region
has remained quiescent as it approaches the western limb. It shall
remain the target region for a further 24 hours although no change in
activity is expected.
The approximate position of the target region on 23-Sep-2018 at 07:10 UT is:
N08W60, ( 825", 75" )
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 visible solar disk remains spotless. The decaying plage region
along the western equator continues to exhibit UV and EUV
brightenings, and has developed a mini-filament along its polarity
inversion line. It shall continue to be the target region although no
significant change in activity is expected over the next 24 hours.
The approximate position of the target region on 22-Sep-2018 at 16:10 UT is:
N07W54, ( 765", 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 visible solar hemisphere is almost featureless. The new target
region shall be a weak, decaying plage region along the western
equator, which contains a few bright H-alpha kernels. No change in
activity is expected over the next 24 hours.
The approximate position of the target region on 21-Sep-2018 at 16:10 UT is:
N06W41, ( 620", 10" )
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)