Dear Collaborators,
Solar activity remains at an extremely low level. The target
region in the South East quadrant has emerged a small amount
of magnetic flux in the past 24 hours and has formed 2 pores
(1 in each of its polarities). No X-ray flares have occurred
since the last message, with no changes in flaring activity
expected in the following 24 hours.
The approximate position of this region on 25-Apr-2020 at 20:00 UT is:
S06E41 , ( -624", -41" )
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 Collaborators,
The level of solar activity continues to be extremely low, with the
visible solar disk remaining spotless. The small weak magnetic flux
region in the South East quadrant has lost its pore and produced a
few A-class events since the last message. No change is expected in
flaring activity over the next 24-hour period.
The approximate position of this region on 24-Apr-2020 at 17:00 UT is:
S06E57 , ( -798", -57" )
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 Collaborators,
Solar activity remains at an extremely low level. There are no
spot regions on the visible solar disk, but the target region
in the South East quadrant with compact bright EUV loops does
display a small pore. No change in flare activity is expected
in the following 24 hours.
The approximate position of this region on 23-Apr-2020 at 14:00 UT is:
S07E73 , ( -906", -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 Collaborators,
The level of solar activity continues to be extremely low, with no
spots on the solar disk. The target compact bright EUV-loop region
has now rotated over the South East limb, but no change in flaring
activity is expected over the next 24-hour period.
The approximate position of this region on 22-Apr-2020 at 14:00 UT is:
S08E90 , ( -945", -132" )
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 Collaborators,
Solar activity remains at an extremely low level, with no spots on the
solar disk. A set of compact, bright EUV loops are beginning to become
visible over the South East limb near to the location previously chosen
as the target region. No change in flaring activity is expected in the
following 24 hours.
The approximate position of this region on 21-Apr-2020 at 14:00 UT is:
S08E90 , ( -945", -132" )
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 Collaborators,
The level of solar activity continues to be extremely low. The visible
solar disk remains spotless, with no substantial prominences present at
either the East or West limb. The small, bright loop region visible in
STEREO-A images is still located 15-20 degrees beyond the Earth-viewed
East limb. The target remains as this region’s expected limb-crossing
location, but no change in flaring activity is expected over the next
24-hour period.
The approximate position of this region on 20-Apr-2020 at 14:00 UT is:
S10E90 , ( -940", -165" )
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 Collaborators,
Solar activity is still at an extremely low level. Solar minimum
conditions continue with the visible solar disk being spotless and
no substantial prominences present at either the East or West limb.
A small, bright loop region is visible in EUV images from STEREO-A,
at 20-25 degrees beyond the Earth-viewed East limb. The target will
become this region’s expected limb-crossing location, as high-lying
loops may become visible before the next email. No change in flare
activity is expected in the following 24 hours.
The approximate position of this region on 19-Apr-2020 at 14:00 UT is:
S10E90 , ( -940", -165" )
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 Collaborators,
The level of solar activity continues to be extremely low. The visible
solar disk remains spotless, with no substantial prominences at either
the East or West limbs. Once again, there is no default target region
today. No change is expected in flaring activity over the next 24-hour
period.
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 Collaborators,
Solar activity remains at an extremely low level, with no significant
flares (i.e., > B1.0) in the past 10 days. The visible solar disk is
devoid of spots, while there are no significant prominences at either
the East or West limb. There shall be no default target region again
today. No change in flaring activity is expected over the following
24 hours.
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 Collaborators,
The level of solar activity continues to be extremely low. Solar
minimum conditions persist, with no spots present on the visible
solar disk. There shall be no default target region again today,
with no change in flaring activity expected in the next 24-hour
period.
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)