MM#009 Default HESSI Target
Dear RHESSI Collaborators,
The level of solar flare activity has been very low since
the last message. The only reportable event was a B2.9
event at 11/27/11:17 UT produced by target region
NOAA 2689 (C-type sunspot group with a beta magnetic
configuration). 2689 has decayed within its trailing
portion. B-class events possible in the next 24 hour period.
The position of NOAA 2689 on November 27 at 16:30 UT is:
N13W31 (Solar X = 489", Solar Y = 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,
Bill Marquette (Helio Research)
Dear RHESSI Collaborators,
Solar activity remains at a very low level. The target region
has been designated as NOAA 12689 with a beta/C-type
configuration. 12689 is displaying dynamic surges in H-alpha
images. B-class activities are expected in the next 24 hours.
The position of NOAA 12689 on November 26 at 08:30 UT is:
N13W13 (213", 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,
Ying Li (Purple Mountain Observatory / Montana State University)
Dear RHESSI Collaborators,
Solar activity has been at very low levels. A new region is emerging
and forming spots. It produced a long-duration B1 flare just two hours
ago. This event is due to a filament eruption and accompanied by a
weak CME. Today we will watch this new region. B-class flares are
expected with a chance of low C-class events.
The approximate position of the target on November 25 at 08:30 UT is:
N13E03 (-50", 120")
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 / Montana State University)
Dear RHESSI Collaborators,
Solar activity continues at extremely low levels. The solar disk
remains spotless and no flares occurred in the past 24 hours.
There are several filaments distributed in the northern and also
southern hemispheres, which appear to be oscillating. The target
plage NOAA 12687 is mostly unchanged. It is rotating to the west
limb. We will watch this plage region for one more day. Only very
low activities are likely in the next 24 hours.
The position of NOAA 12687 on November 24 at 12:30 UT is:
S09W59 (824", -166")
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 / Montana State University)
Dear RHESSI Collaborators,
The solar disk remains spotless. The target plage NOAA 12687
was the source of a B1.7 at 09:06 UT today. 12687 is showing
surges. Minor activities are expected in the following 24 hours.
The position of NOAA 12687 on November 23 at 8:30 UT is:
S09W45 (680", -173")
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 / Montana State University)
Dear RHESSI Collaborators,
The solar disk remains spotless and no flares occurred again
in the past 24 hours. The target plage NOAA 12687 is creating
a filament. Very minor activities are likely in the next 24 hours.
The position of NOAA 12687 on November 22 at 12:30 UT is:
S09W31 (495", -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 / Montana State University)
Dear RHESSI Collaborators,
The solar disk remains spotless and no flares occurred in the
past 24 hours. The target plage NOAA 12687 is mostly unchanged.
Quiet conditions should continue in the next 24 hours.
The position of NOAA 12687 on November 21 at 08:30 UT is:
S09W15 (249", -186")
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 / Montana State University)
Dear RHESSI Collaborators,
Solar activity continues at an extremely low level with the
GOES soft X-ray flux flat at ~A5. The solar disk is spotless
now. The target plage region NOAA 12687 continues to decay.
No noteworthy events are likely in the following 24 hours.
The position of NOAA 12687 on November 20 at 08:30 UT is:
S09W01 (16", -189")
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 / Montana State University)
Dear RHESSI Collaborators,
The level of solar activity is extremely low. NOAA region 12687
has now decayed to plage. No flares have occurred since the last
message. Low B-class flares may be possible in the next 24 hours.
The position of the now decayed NOAA 12687 on 19-Nov-2017 at 23:00 UT is:
S09E05, ( -88",-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,
Shaun Bloomfield (Northumbria University)
Dear RHESSI Collaborators,
Solar activity is at a very low level. The region that was emerging
in the North West quadrant was initially numbered as NOAA 12688, but
already lost its spots. NOAA 12687 decayed since the last message,
losing a significant amount of area coverage in its trailing spot.
B-class activity is possible in the following 24-hour period.
The position of NOAA 12687 on 18-Nov-2017 at 20:30 UT is:
S08E19, ( -314",-173" )
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)