MM#009 Default Target
Dear Collaborators,
The target region now numbered NOAA 2743 is
mostly unchanged maintaining its tiny B-type/beta
sunspot group. 2743 has been quiescent since
it emerged yesterday. Only minor events possible
in the next 24 hour period.
The position of NOAA 2743 on June 25 at 06:00 UT is:
N04W56 (Solar X = 783", Solar Y = 046")
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)
MM#009 Default Target
Dear Collaborators,
The target region (N03W25, A-type/alpha) is now in decay
phase. We will switch to an emerging flux region located
in the northwestern quadrant. The EFR is currently displaying
a B-type/beta sunspot group. A-type events possible
with a slight chance of B-class activity if the region
continues in growth phase in the next 24 hour period.
The position of the target on June 24 at 11:00 UT is:
N03W45 (Solar X = 669", Solar Y = 025")
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 Collaborators,
Solar activity has been at an extremely low level with
the GOES soft X-ray flux flat at ~A6. Spotless conditions
continue. Yesterday's target filament remains weak.
Today the target will switch to a tiny new flux emerging
region in the northwest quadrant. No flaring activity is
expected in the next 24 hours.
The approximate position of the target on June 23 at 17:00 UT is:
N03W14 (220", 30")
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 GOES soft X-ray flux has been flat at an ~A7 level.
The visible solar disk is still quite clear for any spots. The
target filament becomes fainter, as shown in H-alpha images.
No flaring activity is expected in the next 24 hours.
The approximate position of the target on June 22 at 13:30 UT is:
N45E20 (-150", 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 Collaborators,
Solar activity continues at an extremely low level. No flares
occurred in the past 24 hours. Yesterday's target has decayed.
Today the target will switch to a small filament as shown in the
H-alpha image. No flaring activity is expected in the next 24 hours.
The approximate position of the target on June 21 at 07:30 UT is:
N43E40 (-480", 620")
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 with the
GOES soft X-ray flux flat at ~A6. The visible solar disk remains
spotless, without any features in H-alpha images. Yesterday's
target has significantly decayed. Today the target will switch to
another bright EUV point region in the northeast quadrant. No
flaring activity is expected in the next 24-hour period.
The approximate position of the target on June 20 at 07:30 UT is:
N33E18 (-190", 500")
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. The GOES
soft X-ray flux is flat at ~A6. The visible solar disk is spotless,
even without any features (plage, filament, surge, etc.) in the
H-alpha images. Yesterday's target has completely rotated over
the west limb. Today the target will switch to a bright EUV "point"
region in the southeast quadrant, where seems to be emerging
new flux. No flare activity is expected in the following 24 hours.
The approximate position of the target on June 19 at 07:30 UT is:
S04E70 (-890", -20")
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. The GOES soft
X-ray flux has been flat at ~A6. The target region is rotating over
the west limb. No flare activity is expected in the next 24 hours.
The approximate position of the target on June 18 at 07:30 UT is:
N23W90 (950", 325")
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
have occurred since the last message. The target region only
shows some small EUV jets. No noteworthy events are expected
in the following 24 hours.
The approximate position of the target on June 17 at 07:30 UT is:
N20W70 (890", 305")
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 remains at an extremely low level. The target EFR
has decayed slightly since the last message, and no flares have
occurred in the period. No change in flare activity is expected
over the following 24 hours.
The approximate position of this region on 16-Jun-2019 at 17:30 UT is:
N19W61, ( 782", 299" )
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)