Dear RHESSI Collaborators,
The level of solar activity remains extremely low. Yesterday's target
region has been designated as NOAA 12702, a beta/B-type sunspot group.
Over the past 24 hours, 12702 has stopped emerging flux and started
to decay. No flaring above the A-class level is expected in the next
24 hours.
The position of NOAA 12702 on 18-Mar-2018 at 20:00 UT is:
N21W58, ( 763", 402" )
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 continues at an extremely low level. A new flux region
has emerged in the North West quadrant in the past 24 hours. Although
small, it has already developed spots and is continuing to emerge new
flux. A-class flares may be possible over the following 24-hour period.
The approximate position of the target region on 17-Mar-2018 at 19:00 UT is:
N20W43, ( 618", 410" )
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 remains extremely low. Yesterday's target
region was designated by NOAA as 12701, but has since decayed into an
unspotted plage region. No flares above A-class are expected in the
next 24 hours.
The approximate position of the target region on 16-Mar-2018 at 20:00 UT is:
S12W19, ( 309", -89" )
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 continues at an extremely low level. A new, very small
spotted region has emerged close to solar disk centre. This currently
unnumbered region has a beta/B-type configuration. A-class flaring may
be possible in the following 24-hour period.
The approximate position of the target region on 15-Mar-2018 at 22:00 UT is:
S13W06, ( 102", -99" )
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 remains extremely low. Spotless conditions
continue on the visible solar disk. The target decaying plage region
has evolved little over the past 24 hours. No flaring activity above
A-class is expected in the next 24 hours.
The approximate position of the target region on 14-Mar-2018 at 14:30 UT is:
S10W60, ( 826", -107" )
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 continues at an extremely low level. The visible solar
disk is devoid of spots. The decaying plage region in the South West
quadrant remains the target. No flares above A-class are expected in
the following 24-hour period.
The approximate position of the target region on 13-Mar-2018 at 22:00 UT is:
S10W51, ( 742", -92" )
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 remains extremely low. Spotless conditions
continue on the visible solar disk. A weak filament may still exist in
the target decaying plage region. No flaring activity above A-class is
expected within the next 24 hours.
The approximate position of the target region on 12-Mar-2018 at 15:00 UT is:
S10W34, ( 534", -68" )
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)
MM#009 Default HESSI Target
Dear RHESSI Collaborators,
Solar flare activity is at an extremely low level.
The visible solar disk is spotless. The plage
target continues to slowly decay. Its main filament
located along the region's magnetic inversion line has
almost completely disappeared. No significant solar
flare activity is expected anytime soon.
The position of the target on March 11 at 13:30 UT is:
S10W20 (X = 327", Solar Y = -054")
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 HESSI Target
Dear RHESSI Collaborators,
Solar flare activity continues at an extremely low
level. The visible solar disk remains spotless.
The decaying spotless target region (return of old
NOAA 2699) is mostly unchanged but its main
filament located along its magnetic inversion line
is currently somewhat activated. No significant
solar flare activity expected anytime soon.
The position of the target on March 10 at 15:30 UT is:
S09W09 (Solar X = 150", Solar Y = -031")
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 HESSI Target
Dear RHESSI Collaborators,
Solar flare activity continues at an extremely
low level. The visible solar disk is spotless.
The spotless target region (return of old NOAA 2699)
is mostly unchanged. No significant solar flare activity
expected anytime soon.
The position of the target on March 09 at 15:30 UT is:
S08E04 (Solar X = -067", Solar Y = -013")
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)