Each
month a summary of sunspot activity is written and forms part of a
report sent to the Solar Section of the British Astronomical
Association (BAA)
and to The
Astronomer. Follow the links below to read a
page summary of
sunspot activity. The McIntosh Sunspot Group Classification is used for
sunspot group descriptions.
January
2012
The largest of
the five groups seen on the 2nd was AR 1389 at 19°S/84°
–
this was of type Ekc
with an area of 350 millionths. It consisted of a slightly asymmetrical
leading
penumbral sunspot and a collection of smaller following sunspots. All
of the followers had disappeared by the
6th to leave an Hkx sunspot. Close to the eastern limb on the 2nd was
an Hsx
sunspot (AR 1391) – by the 6th it was seen as a Dkc group at
11°N/11° where the
leading sunspot contained most of the area of the group of 320
millionths. When
next seen on the 11th AR 1391 was much smaller at 170 millionths
despite the
group becoming type Eac. Between the 6th and 11th AR 1393 at
19°N/52° changed
from type Bxo to a Eac group near the western limb. On the 13th and
14th AR
1391 continued to decay to become type Dso when last seen on the limb
on the
14th.
Two
of the 9
groups seen on the 15th were close to the eastern limb: AR 1401 and AR
1402.
AR 1401 was first seen
as type Hsx
on the 14th before becoming type Cso on the 15th and then type Eac on
the 16th
at 17°N/214°.
By the 19th it was
seen
approaching the central meridian when it has an area of 420 millionths
– it
consisted as a string of three cluster of almost equally sized
penumbral
sunspots. Further development had taken placed by the 21st when the
main
sunspot was towards the middle of the group. AR 1402 some 10°
to
the north of AR
1401 was a Hax sunspot when first seen on the 15th and type Hkx on the
16th. By
the 19th it was seen as Dko at 30°N/211° with an area
of 370
millionths: it
consisted of a small leading penumbral sunspot with a much larger
irregular
follower. This follower had changed shape slightly by the 21st and the
total
area was almost unchanged. AR 1402 was last seen on the western limb as
on
27th. The last observation of the month on the 28th showed just three
small
groups.
Hydrogen
Alpha:
On the 2nd a tall
prominence of an inverted V shape was seen on the NW limb while several
long
sinuous filaments were also seen in the northern hemisphere. There
was also a region of plage in the
northern hemisphere possibly associated with AR 1390. A flame type
prominence
was seen on the SW limb on the 14th – it had an estimated
height
of 110,000 km.
The majority of the filaments were still in the northern hemisphere
including a
broad filament in the NE quadrant. Plage was seen around AR 1396. On
the
following day, the 15th, all prominences were small – the
same
broad filament
was still present as was the plage around AR 1396 (although a filament
was now
also seen to its north). On the 21st a detached inverted V shaped
prominence
was seen above the NW limb where the height of the top of the
prominence was
about 120,000 km. Another detached prominence of a bush shape was seen
almost
exactly on the opposite limb. On the disk the same filament as seen on
the 14th
& 15th was seen nearing the W limb. Plage was seen near the
central
meridian and around AR 1401 and 1402. On the 28th the number of
prominences had
reduced to just three – all on the NE limb. A long thin
filament
was seen in
the north/south direction in the northern hemisphere while a much
broader
filament was seen in the southern hemisphere but lying east/west.
February
2012
Two of the four
northern groups from the 1st were AR 1413 and AR 1410. AR 1413 at
9°N/6° was a
small Dao group with an area of 40 millionths – it grew in
size
over the next
two days to 130 millionths but it had lost most of its pore sunspots.
Just to
its north was AR 1410 at 18°N/58° of type Hax with an
area of
150 millionths –
it became type Cao on the 2nd before reverting to type Hsx on the 3rd.
It was
last seen on the 7th close to western limb but now of type Dso (indeed
it was
the only group seen on the date).
The
next
observation on the 11th showed just two groups. AR 1416 at
18°S/287° was of
type Dkc with an area of 320 millionths which consisted of a bipolar
group
where the largest penumbral sunspot was the following one and with
several
small sunspots within the group. AR 1417 at 16°N/239°
was of
type Hsx with an
area of 50 millionths.
All
of the five
groups seen on the 19th were small – the largest was AR 1422
at
18°N/177° of
type Dac and an area of 80 millionths. By the 21st it grew to 320
millionths
where the leader was quite elongated and the largest sunspot in the
group. This
group reduced in size slightly by the 23rd and was last seen near the
limb as a
Hax sunspot on the 25th. The last observation of the month on the 26th
showed
four small groups in the north east quadrant of the Sun.
Hydrogen
Alpha:
On the 11th
filaments were the dominant Hα feature with a long string of
filaments in the
NW quadrant as well as near the South Pole. A similar number of
filaments were
seen on the 19th but these were quite short and spread throughout the
disk. A
moderately tall prominence was seen on the NE limb and plage was
visible around
AR 1422.
The same flame and
spike
prominence
was seen on the SW limb and SE limb respectively on the 25th and 26th.
Filaments were seen on both dates including a string a filaments
spanning the
meridian in the southern hemisphere. Plage was still seen around AR
1422 but
only on the 25th having rotated off the disk on the 26th.
March
2012
A medium sized
Hkx sunspot was seen close to the eastern limb on the 3rd at
17°N/299°.
By the 6th this group,
AR 1429 was now seen
as an irregular and elongated penumbral sunspot with many umbra and a
small
region of photosphere within it. A smaller penumbral sunspot was also
seen
towards the north east of the main sunspot – its total area
was
estimated to be
700 millionths. When next seen on the 8th it was close to the central
meridian
and slightly larger at 920 millionths – again many umbra were
seen. By the 11th
several penumbral sunspots were seen due to the splitting of the main
penumbral
sunspot - the total area was a reduced 500 millionths and it was of
type Ekc. A
single Hsx sunspot on the western limb was all that remained of AR 1429
on the
15th (the leading part of the group may have already rotated off the
disk).
On the 6th a small Csi
group,
AR
1430, was seen some 15° to the west of AR 1429 at
19°N/315°. By the 8th the
penumbral sunspot has become asymmetric to give a Cai group with an
area of 160
millionths. It had decayed to type Cso when last seen on the 11th. During
this period the other notable group
was in the southern hemisphere was AR 1428 at 16°S/319°
which
had a maximum
area of 170 millionths on the 8th when the group was bipolar and of
type Dao.
From
the 15th
onwards all the groups seen were small – the largest being an
Esc
group at 23°S/25°
on the 26th (AR 1445).
From the 20th
onwards, and unusually for this solar cycle, there were more groups in
the
southern hemisphere than in the northern hemisphere. For example on the
28th
there were five southern groups and one northern group.
Hydrogen
Alpha:
On the 3rd
several small prominences were seen together with a dark filament in
the NE and
plage around AR 1423. On the 11th a tall spike like prominence was seen
on the
SE limb while on the disk the majority of Hα activity was
confined to the
northern hemisphere with a long multi part filament in the NE quadrant.
Plage
was also seen around AR 1429, AR 1430 and AR 1432. Very little activity
was
seen on the 24th which improved slightly by the following day with
plage being
seen around AR 1440 and AR 1444. An active multiple arch prominence was
seen on
the NE limb on the 26th with an estimated height of 100,000 km. A few
filaments
were seen on the disk as well as plage AR 1444.
April
2012
White light
activity was quite low during the first half of the month before
becoming
moderately high for the third week before reducing slightly towards the
month’s
end. On the 1st four groups were seen where the largest was AR 1445 of
type Hax
at 21°S/31° with an area of 140 millionths. Another
group, AR
1450 at 16°N/323°,
was of type Bxo on the 1st before developing into type Csi on the 2nd
and then
into a small Eao group on the 4th having just passed the central
meridian and
then into a slightly larger Dai group on the 6th when it had an area of
150
millionths. This and AR 1452 were the only groups seen on the 6th. Even
lower activity was seen on the 11th when
there were only two Axx groups (AR 1455 and AR 1454). AR 1455 at
6°N/206° was
of type Dao on the 13th and 14th with an area of 130 millionths
–
it had
decayed when last seen approaching the western limb on the 16th now of
type
Csi.
There
was quite
a contract in activity on the next observation on the 20th –
there were now
seven groups with several being moderately sized. The groups were also
spit
between the hemispheres, three in the north and four in the south. Although
AR 1459 at 14°S/91° was seen
close
to the eastern limb on the 16th it just comprised of four small
penumbral
sunspots; it now consisted of a small clump of many small penumbral and
other
sunspots. Two other southern groups had formed on the disk towards the
west of
AR 1459 – these were AR 1463 and AR 1462. The
main northern group on the 20th was the Dac AR 1460 at
16°N/108° and
near the central meridian which comprised a string of moderately size
penumbral
sunspots. By the 21st AR 1459 had become type Eac and where the size of
the
many penumbral sunspots had increased slightly. AR 1462 was still of
type Dao
but it had increased in size to 450 millionths. When
seen on the following day AR 1459 has lost some if its penumbral
sunspots but the leader had increased so that the group was now of type
Ekc
with an area of 350 millionths. AR 1462 was now approaching the western
limb
while the northern AR 1460 was of type Dao with an area of 320
millionths. The
five groups from the 22nd were of a similar appearance by the following
day.
On
the 27th the
largest of the five groups seen was AR 1466, a Fac group at
12°N/35° which had
an area of 160 millionths. By the 29th AR 1471 of type Cho had rotated
around
the eastern limb and when seen on the following day it became type Eho
– it had
a total area of 360 millionths due mainly to the moderately sized
leading
sunspot.
Hydrogen
Alpha:
Activity was
quite low on the 1st with just a few small prominences but quite a few
small
filaments. On the following day a small arch prominence was seen on the
NW limb
while a moderately long filament was seen to the north of AR 1452 in
the NE
quadrant where two small regions of plage were seen.
The
arch prominence was still visible on the
4th as was the filament which now appeared longer as it approached the
central
meridian. The plage region was also still visible.
The
same long filament was seen on the 6th as
was the plage – on this date all prominences were still small
but
there were
still several other filaments visible.
Hα
activity had
increased by mid-month as the height of prominence and the number of
filaments
had increased slightly. Plage was seen around AR 1455 and AR 1457 on
the 13th
and around AR 1455 and AR 1459 on the 16th. A bush type prominence was
seen on
the SE limb while slightly taller flame type prominences were seen on
the SW
limb, both on the 16th. On the same day another long filament was seen
spanning
the central meridian in the northern hemisphere.
On the 21st a fine
loose arch prominence was seen on the SW limb – by the
following
day this had
formed into two nearby pillar filaments with a thin string of filament
linking
the two pillars. The height was estimated to be 140,000 km. Many
regions of
plage were also seen, mirroring the increase in white light activity.
Several
small filaments were on both the 21st and 22nd.
May
2012
Activity during
the month was
dominated by one group – AR 1476. The
first observation of the month on the 7th showed AR 1476 near the
eastern limb at
11°N/181°
and of type Fkc: the largest sunspot was the leader which was quite
irregular
in shape and this was followed by a number of smaller penumbral
sunspots. When
next seen on the 11th AR 1476 was near the central meridian and the
leader
dominated the group and it had become quite irregular with many umbrae
within
it. A string of small penumbral sunspots had formed to the NE of the
main
sunspot. The group had an estimated area of 960 millionths. By the
following
day the leading sunspot had reduced in size but it now included two
area of
photosphere within it. There were some smaller penumbral sunspots to
the west
and south of this sunspot – the number of sunspots in the
following string had
reduced in number such that now the total area was 660 millionths. The
group
had decayed slightly when seen on the 13th but it was still of type
Fkc. It was
last seen on the 16th near the western limb as a single Hsx sunspot. AR
1476 was seen with the protected naked eye
on the 11th, 12th and 13th.
Together
with AR 1476 on the
16th, six other groups were seen but none were particularly large. For
the rest
of the month there were either four or five groups seen for each
observation –
the largest being AR 1492 at 230 millionths when seen on the 27th at
12°S/283°
and type Eao.
Hydrogen
Alpha:
A
striking arch prominence was seen on the SW
limb on the 11th, 12th and 13th. A quite active prominence was seen on
the NE
limb on the 11th and 12th – at a similar location on the 13th
a
detached
prominence was seen which comprised three separate pieces of hydrogen.
On these
three days, several short filaments were present as was plage around AR
1476
was well as AR 1479 (an Esc group at 15°N/103°).
Several
prominences were seen
on the 16th which included another detached prominence on the NW limb -
several
filaments were also seen as was plage around ARs 1479, 1484 and 1485. On
the 27th several prominence and filaments
were seen as well as plage around ARs 1488, 1490 and 1492.
June
2012
Although 7
groups were seen on
the first observation on the month on the 4th, none were particularly
large –
there largest were AR 1497 at 20°S/223° of type Dac and
AR 1493
at 15°N/208° of
type Eac each with an estimated area of 150 millionths.
There
were an almost equal number of groups
in the northern and southern hemispheres. The largest group of the
month was
first seen on the 9th as a Dsc group near the eastern limb at
15°S/85° (AR
1504). It was of a similar appearance on the following day but by the
13th it
had developed into a bipolar group where the main sunspots were the
leader and
follower with an arc of smaller sunspots between. It
was now of type Ekc with a total area of
450 millionths. On the 14th some of the smaller sunspots had developed
into a
penumbral sunspot.
When next seen on the
16th, there were now three penumbral sunspots where the leader and
followers
were of almost equal size while the other sunspot to the north of the
follower
– the total area was now 610 millionths. It
was of a similar size on the 17th although it had
become type
Eac.
By the 19th, with the
group nearing
the western limb it had reduced to 430 millionths and it was finally
seen on
the 20th as a Dac group.
It was also the
only group seen on the 20th and it was seen with the protected naked
eye on the
13th, 14th and 16th.
Activity
on the 23rd, 24th and
25th was limited to one different group per day (AR 1511, 1510 and 1512
respectively).
On the 26th AR 1512, a
Dsc group at 15°S/262° was joined by AR 1513 at
12°N/213° on the eastern limb
as an Hsx sunspot.
Other groups has
appear by the 29th and 30th (five on each day) where the largest was AR
1515 at
16°S/206° of type Dac and area 330 millionths on the
30th.
Hydrogen
Alpha:
Generally
the prominences seen from 6
observations were fairly small but reasonably numerous on each day. Of
particular note was a bright and active
prominence seen on the SW limb on the 20th and a combined arch
&
cloud
prominence seen on the SE limb on the 30th. Filaments
were also reasonably numerous on each
observation but most
were short – an exception was a curved filament seen on the
SW
quadrant on the
30th.
Plage was seen around
AR 1499 on
the 9th, around AR 1504 & 1507 on the 13th, AR 1510 on the
24th, AR
1512 on
the 25th and around AR 1513 and 1516 on the 30th. Two flares were seen
during
the month:
on the 4th a flare were
briefly
seen in a gap in the clouds around AR 1494 at 15h 40m UT (type B9.9)
while on
the 30th a flare was seen near the NE limb between 16h 10m and 16h 20m
UT (type
C1.3).
July
2012
Activity was
dominated by three moderately
sized groups, all in the southern hemisphere.
The
first of these was AR 1515
which developed from a D type group at the end of June into an Eac
group at 16°S/206°
with an area of 450 millionths when seen on the 1st.
It
was a particularly complex group with an
asymmetrical leader and a set of complex following penumbral spots. This
group still retained its complex form
when next seen on the 7th when it had an area of 690 millionths
–
now the
largest sunspot was the follower. This
group was last seen on the 8th when it was close to the western limb.
The
second group, AR 1520, was
seen close to the eastern limb on the 7th. On
the following day, this group at 16°S/86°, was
of type Fkc with an
area of 1190 millionths – the largest penumbral sunspot was
near
the centre
with thin following extension and other surrounding sunspots. Several
umbrae were seen within the main
sunspot as well as a region of photosphere. This
group was of a similar size when next seen a few days
later on the
14th. The largest sunspot was now toward the following part of the
group but
there were still other penumbral sunspot leading and following the main
sunspot. The appearance of the main sunspot changed appearance by the
following
day and it the total area of the group was slightly smaller at 1000
millionths.
AR 1520 was last seen
close
to the western limb on the 17th when it was still of type Fkc. It
was seen with the protected naked eye on
the 13th and 14th.
The
final moderately sized group,
AR 1532, was initially seen as a single Hsx sunspot on the eastern limb
on the
26th.
By the 28th, further
following
sunspots had rotated on to the disk to make the group, at
21°S/177°, of type
Fko. By the 29th a penumbral sunspot had appeared between the leader
and
follower to make the group of type Fkc while by the 30th the
irregularly shaped
leader in increased to give the group a total size of 620 millionths.
Hydrogen
Alpha:
The
most notable prominences from 6 observations
were seen towards the end of the month. On the 26th a fine windsock
shaped
prominence was seen on the NE limb with a maximum height estimated to
be about
110,000 km (a smaller more complex prominence was seen at a similar
location on
the 24th).
On the 28th two nearby
cloud
prominence were seen on the SE limb – the northern most being
completely
detached from the limb.
There were many
filaments on the disk on the 1st and 15th, very few on the 21st before
increasing again for observations on the 24th, 26th and 28th. Some
of the longest prominences were seen on
the 26th and 28th.
Plage was seen around
AR 1515 on the 1st, AR 1520 on the 15th, ARs 1531 and 1533 on the 26th
and
around ARs 1533, 1530 and AR 1532 on the 28th. Two
flares were seen during the month: on
the
1st a flare was seen near AR 1515 between 15h 50m
and 16h 25m UT
(type C8.2) while on the 28th a C1 flare was seen near AR 1530 between
16h 30m
and 17h 00m UT.
August
2012
Overall
activity was high at the
start of the month before reducing towards the middle of the month and
then
becoming high again at the month’s end. Also
activity was slightly higher in the southern hemisphere. None of the
groups
seen during the month were particularly large.
The
Fkc group AR 1532 at
21°S/176° from July was seen straddling the central
meridian on
the 1st but
with a reduced size of 320 millionths – the leader was still
the
largest sunspot
in the group.
AR 1532 was also the
largest of the seven groups seen on the 1st. On the 2nd AR 1532 has
become type
Fac through a further reducing in the size of the leader.
It
was of similar appearance on the 3rd
before on the 4th all but one of the following sunspots remained to
make the
group type Cao.
This group was last
seen
on the 5th as it neared the western limb. On
the 3rd and 4th ten groups were seen with a sunspot
number of just
over 120.
On
the 8th a Dho group was seen
close to the eastern limb at 20°N/20° - AR 1543. It was
of the
same type on the
9th before the leader became asymmetric to make the Dko when seen on
the 10th.
Several other sunspots were seen within the group on the 12th while on
the 14th
the group, now just past the central meridian, was of type Hkx with an
area of
320 millionths.
Only two groups were
seen on the 14th, the lowest number during the month.
AR
1543 was seen of type Hax on the 17th and
18th before being seen as type Dao as it approached the western limb on
the
19th.
Observations
on the 23rd and 25th
to 28th showed either four or five small groups. Although the number of
groups
had increased by the 31st, the largest of the eight groups were AR 1553
at 20°S/182°
of type Dac at 200 millionths and AR 1560 at 4°N/127°
also of
type Dac at 180
millionths.
Hydrogen
Alpha:
An unusual
prominence seen from 11
observations was on the 27th and 28th – on the 27th an almost
rectangular block
of hydrogen was seen on the NE limb. The
top of the prominence was quite flat and parallel to the limb; there
was also a
slight extension from the middle of the northern side of the prominence. On
the 28th, this extension could be seen
extending onto the limb as a short filament. Also on this date, the
height of
the prominence had reduced slightly.
Many
filaments were seen at the
start of the month, especially on the 1st and 2nd.
These
were of various lengths with the
longest being near the equator in the eastern hemisphere.
This
was still seen on the 4th when this was
the main filament seen.
A multi-segment
semi-circular filament was seen on the southern hemisphere on the 17th,
18th
and 19th.
The number of filaments
increased again towards the end of the month as seen on the 27th and
28th.
Plage
was seen around AR 1538 & 1539 on the
3rd and 4th, AR 1543 on the 8th & 10th, around AR 1546 on the
19th
and
around AR 1555 on the 28th.
On the 18th
between
14h 25m and 14h 40m UT a type C7.3 flare was seen near AR 1548 which
was also close
to the eastern limb.
September
2012
The
highest number of group
seen
during the month, eight, was on the 3rd. The
most prominence of these groups was AR 1560 and AR
1564.
AR 1560 was of type Eac
at
4°N/129° which
comprised of a collection of small penumbral and other sunspots where
the total
area was 190 millionths.
On subsequent
days the number and size of sunspots within this group reduced such
that by the
6th when the group was nearing the western limb it was just a Bxo
group. AR
1564 was slightly larger than AR 1560 on the 3rd at 250 millionths and
of type
Eac at 13°S/69° – it too was a collection of
penumbral
and other sunspots. As
this group progressed towards the central meridian the number of
penumbral
sunspots reduced while the number of pores increased. On the 7th, with
the
group just past the central meridian, just two penumbral sunspots were
seen –
however by the following day there were more penumbral sunspots. AR
1564 was
last seen on the western limb on the 11th as a Bxo group.
By
the 13th there were three
groups on the disk – the largest being AR 1569 at
11°S/297° and of type Eac
with an area of 220 millionths through the presence of three penumbral
sunspots. As this group progressed towards the central meridian, it
lost its
following sunspots such that by the 18th it was of type Hax. AR 1571
was seen
at almost the same latitude as AR 1569 but following by almost
20°
- for
example on the 18th it was at 12°S/280° of type Hsx
with an
area of 60 millionths.
No sunspots were
seen in the northern
hemisphere on the 16th and 17th.
The
next observation on the 22nd
showed AR 1575 at 9°N/181°and of type Eao to be the
largest of
three groups at
270 millionths. When next seen on the 29th it was of type Hsx close to
the
western limb. Also on the 29th Hhx and Hkx sunspots were seen in the
southern
hemisphere at 9°S/108° and 11°S/85°
with areas of 120
and 260 millionths
respectively (ARs 1579 and 1582).
Hydrogen Alpha:
There were
numerous prominences
seen on 3rd including a pair of nearby flame type on the NW limb with a
maximum
height of about 100,000 km, an arch type on the W limb and a tower type
on the
SE limb. A slightly reduced number of prominences were seen on the 7th
and
14th.
Only three prominences
were seen
on the 16th and 29th but one of those on the 29th was as a complex
structure on
the SE limb with a maximum height of 100,000 km.
Filaments
were seen on all five
observations – of particular note was a semi-circular
filament
seen in the SW
quadrant on the 16th and a pair of nearby filaments on the NW quadrant
on the
29th.
Plage
was seen around AR 1560 & 1564 on the
3rd, around AR 1569 on the 14th, around AR 1574 on the 16th and around
AR 1577
and AR 1583 on the 29th.
October
2012
Although only seven observations
were made, it appears that activity was reduced compared to recent
month.
Also the majority of
the activity
seen was in
the southern hemisphere.
The largest of
the four groups
seen on the 4th was an Hkx sunspot AR 1582 at 10°S/83°
which
had an area of 270
millionths.
This sunspot was
located
mid-way between the central meridian and the western limb. It was seen
having
the same form on the 6th and 7th when it was near the western limb.
Another of
the groups from the 4th was AR 1585 at 20°S/6° of type
Dao
– this comprised of
an irregularly shaped leader penumbral sunspot and a smaller follower
penumbral
sunspot. By the 6th the follower sunspot had disappeared to make the
group Cao
as there were also a few pores within the group. On the 7th this group
was near
the central meridian with an area of 120 millionths. It changed little
by the
10th but it decayed into a single Axx sunspot when seen on the 13th
close to
the western limb.
A
complex group, AR 1589, was
seen near the eastern limb on the 10th as type Dko at
14°N/266°. It comprised
of two irregular penumbral sunspots and it was surrounded by an
extensive area
of faculae. By the 13th one of the penumbral sunspots had decayed to
leave a
compact collection of several smaller penumbral sunspots –
the
total area was
estimated to be 160 millionths. By the 16th this group had decayed
further to
become a single small penumbral sunspot surrounded by many pores.
The
final observation of the
month, on the 30th, showed three southern groups, the largest being AR
1598 at
9°S/115° with an area of 240 millionths.
Hydrogen Alpha:
The only
Hα observation of the
month was on the 5th. Although several filaments were seen, none were
particularly
large.
Several small filaments
were also
seen as was plage around AR 1585.
November
2012
The first
observation of the
month, on the 3rd, shows only three small groups. By the 11th the
number of
groups had increased to seven which were all with the south-east
quadrant.
The group nearest the
central
meridian was AR
1610 at 22°S/263° which was of type Dac and it had an
estimated
area of 190
millionths. Another moderately sized group was AR 1611 at
12°N/240° – it was
also of type Dac with an area of 240 millionths. AR
1614 was seen close to the eastern limb at
14°N/193° and of type Dsc. On
the
13th
and 14th, AR 1610 had increased in size slightly to 230 millionths and
had
become type Eac. Meanwhile AR 1611 reduced in size to become an Hsx
sunspot
when seen on the 18th. AR 1614 because a complex Dac group by the 14th
with an
area of 220 millionths – it had become type Csi by the 18th.
Between
the 14th and 18th, the
largest group seen during the month, had appeared on the disk. This
was AR 1618 which was of type Cai at
9°N/134°
with an area of 90 millionth – it was seen as an asymmetric
leading penumbral
sunspot followed by several pores. When seen on the 22nd the group was
far more
complex with irregular penumbral sunspots in the middle and following
parts of
the group – it was of type Ekc with an area of 430
millionths. It
was also near
the central meridian and seen with the protected naked eye. By the 25th
it had
decayed to a size of 250 millionths and of type Eac although the
largest
sunspot was at the following part of the group.
The
final observation of the
month, on the 30th, showed four groups which included two D type groups
at a
similar longitude and separated by a few degrees in latitude
– AR
1625 at
14°N/341° and AR 1623 at 9°N/340°.
These
two groups gave the appearance of a square of four penumbral sunspots.
Hydrogen Alpha:
Although
prominences were seen on
each of the four observing days on the 3rd, 11th, 18th and 25th, the
most
striking prominences were seen on the 18th – a tree shaped
prominence was seen
on the SE limb with the main “branches” being
vertically
and two horizontal
either side of the prominence.
Close by
and slightly towards to the equator a combined prominence/filament we
also
seen, although the prominence part was not as tall as the tree
prominence. Many
other filaments were seen for each of the four observations, especially
again
on the 18th when filaments were seen in both hemispheres and over all
longitudes.
The
observation on the
3rd showed
plage near to AR 1604.
On the 11th plage
was seen around AR 1610 and around AR 1614 which was near the eastern
limb. On
the 18th plage was seen around ARs 1612, 1614, 1619 and 1618 while on
the 25th
plage was still visible around AR1618, although the group had decayed
since the
18th, but also around AR 1620 and 1622.
December
2012
Based on seven
observations throughout
the month, activity was quite low with all the groups seen being quite
small.
On the 2nd the two
nearby groups
of AR 1625 and 1623 were seen of a similar appearance as at the end of
November
although the following sunspot of AR 1623 had almost disappeared to
remove the
square appearance of these two groups. These groups had disappeared by
the time
of the next observation on the 10th when just two groups were seen
nearing the
central meridian – AR 1630 of type Bxo at
18°N/253° and
AR 1629 of type Dso at
12°N/239° and size 90 millionths. By the 12th AR 1630
had
become type Dso with
an area of 70 millionths. When last seen on the 17th AR 1629 a single
Hsx sunspot
close to the western limb.
The
largest of five groups seen
on the 17th was AR 1633 at 5°S/111° of type Eao and
area 200
millionths. It was
next seen on the 26th as an Hsx sunspot near the western limb. Also on
the 26th
AR 1635 was seen at 14°N/62° of type Dsc and area 200
millionths – this was the
largest of the four groups seen on the 26th.
Hydrogen
Alpha:
Observations
on the 2nd and 16th
showed several small prominences with the largest being on the SE limb
on the
2nd as two nearby curved pieces of hydrogen. Similarly many small
filaments
were seen on both dates. Plage was seen around each the three groups
seen on
the 2nd (ARs 1621, 1625 & 1623).
Page
created on 30 December 2011.
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