The small bipolar group was noticed at the 24th parallel of the Northern hemisphere since 18.09 to 22.09 near the Western limb. The head sunspot had a symmetrycal penumbra.
The big multipolar group crossed the Sun disc since 22.09 to 5.10 along the middle latitudes of the Northern hemisphere. The multipole consisted of big head sunspots with a large extended penumbra, tail sunspots with a common big penumbra and developed sunspots since a common penumbra in a middle part of the group which were gradually merging the head sunspots. As approaching the Western limb the head group's part had again forked and the tail sunspots had gradually decayed. Neighboring the central meridian the total region's area exceeded 1000 m.h.s., it was counted about forty sunspots in the group.
The stable sunspot with a symmetrycal penumbra crossed the Sun disc since 25.09 to 7.10 along the 12th parallel of the Northern hemisphere. Pores and fine sunspots were observed neighboring the sunspot. Before the Western limb the sunspot began grow, the total region's area reached 250 m.h.s.
The small bipolar group crossed the Sun disc since 2.10 to 14.10 along the high latitudes of the Northern hemisphere. The head sunspot had a noticeable symmetrycal penumbra.
The small bipolar sunspots were observed at the 11th parallel of the Southern hemisphere since 4.10 to 12.10 in the Western part of the Sun disc. The head sunspot had a stable symmetrycal penumbra.
The noticeable sunspot with a stable symmetrycal penumbra crossed the Sun disc since 4.10 to 17.10 along the 22nd parallel of the Northern hemisphere. Time to time the sunspot's area exceeded 250 m.h.s.
The big sunspot with a stable symmetrycal penumbra crossed the Sun disc since 9.10 to 22.10 along the 27th parallel of the Northern hemisphere. Time to time the total region's area reached 300 m.h.s., and pores and fine sunspots of an opposite magnetic polarity appeared neighboring the sunspot.
The big bipolar group crossed the Sun disc since 11.10 to 22.10 along the 12th parallel of the Southern hemisphere. The head sunspot had a developed symmertycal penumbra which was gradually extended lengthways a parallel owing to umbra's bifurcation. The tail group's part consisted of three umbraes with a common triangle penumbra. Then this construction was scattered on spots with separated penumbraes. Neighboring the central meridian the total bipole's area had exceeded 300 m.h.s. As approaching the Western limb the group's sunspots were gradually decreased.
The growing sunspot's shain was observed since 12.10 to 22.10 at the tenth parallel of the Northern hemisphere. In the evolution's peak the total bipole's area reached 400 m.h.s., and in the group it was counted more thirty sunspots.
The big bipolar group crossed the Sun disc since 17.10 to 31.10 along 12th parallel of the Northern hemisphere. The multipole represented a solid chain of small sunspots with developed penumbraes. As approaching the central meridian this construction began collapse, and few sunspot reached the Western limb. In the evolution's peak the total region's area exceeded 350 m.h.s., and it was counted about thirty sunspots in the group.
The collapsing bipolar group was observed since 20.10 to 20.10 at the middle latitudes of the Northern hemisphere. In the first days the head bipole's part consisted of two closer sunspots with symmetrycal penumbraes. Then the spots began disperse from each other and decrease in sizes. The maximal total region's area exceeded 250 m.h.s.
The undistinguished bipolar sunspots were observed at the middle latitudes of tne Northern hemisphere since 20.10 to 22.10, not far from the Western limb.
The small bipolar group was marked at the high latitudes of the Southern hemisphere since 20.10 to 28.10, in the Western part of the Sun disc. The tail sunspot had a stable penumbra. Time to time the total bipole's area reached 200 m.h.s.
The short-time bipolar sunspots were noticed at the middle latitudes of the Northern hemisphere since 20.10 to 23.10, neighboring the central meridian.
The opened bipolar group crossed the Sun disc since 22.10 to 4.11 along the low latitudes of the Northern hemisphere. The head sunspot represented a big umbra with a stable penumbra. In the first days the tail saunspots had a common curved penumbra, then this group's part returned in slow desintegration. Neighboring the central meridian the total bipole's area reached 500 m.h.s., and it was counted ten-twenty sunspots in the group.
The opened bipolar group crossed the Sun disc since 1.11 to 13.11 along the middle latitudes of the Southern hemisphere. The head and tail sunspots had stable symmetrycal penumbraes. The group's axis had a considerable inclination to the parallel. The total bipole's area exceeded 200 m.h.s.
The big multipolar group crossed the Sun disc since 2.11 to 15.11 along the 20th parallel of the Northern hemisphere. The head sunspot had a large stable penumbra and the group had a closed configuration. Time to time the total region's area 1500 m.h.s. and it was to fifty sunspots in the group.
The small bipolar group crossed the Sun disc since 5.11 to 18.11 along the tenth parallel of the Northern hemisphere. The head sunspot had a stable symmetrycal penumbra and the tail group's part consisted of recurrent sunspots.
The opened bipolar group was observed since 5.11 to 18.11 to the North-West from the group 11341. The head sunspot had a stable symmetrycal penumbra and the tail group's part consisted of recurrent sunspots. Time to time the total bipole's area reached 300 m.h.s.
The growing bipolar group was observed at the 20th parallel of the Southern hemishere since 7.11 to 15.11 in the Western part of the Sun disc. Before the Western limb the total bipole's area reached 200 m.h.s.
The fine bipolar group crossed the Sun disc since 12.11 to 24.11 along the middle latitudes of the Southern hemisphere. The head sunspot had a stable symmetrycal penumbra.
The small bipolar group crossed the Sun disc since 16.11 to 28.11 along the high latitudes of the Southern hemisphere. The head sunspot had a stable symmetrycal penumbra. The tail pores were gradually collapsed.
The fine sunspot with an unstable symmetrycal penumbra was observed since 17.11 to 28.11 at the low latitudes of the Northern hemisphere. Time to time pores of an opposite magnetic polarity appeared neighboring the sunspot.
The small bipolar group crossed the Sun disc since 17.11 to 27.11 along the middle latitudes of the Southern hemisphere. In the first days the bipole presented as a rhombus made from small sunspots with developed penumbraes, the total area reached 200 m.h.s. The group was slowly collapsing.
The small stable sunspot with a symmetrycal penumbra crossed the Sun disc since 18.11 to 1.12 along the 14th parallel of the Northern hemisphere. Time to time pores and fine sunspots appeared neighboring the sunspot.
The big bipolar group crossed the Sun disc since 19.11 to 2.12 along the middle latitudes of the Northern hemisphere. The head and the tail sunspots had stable symmetrycal penumbraes. The tail sunspot was gradually bifurcaing. In the evolution's peak the total bipole's area reached 400 m.h.s.
The small bipolar group crossed the Sun disc since 22.11 to 5.12 along the 20th parallel of the Northern hemisphere. The head sunspot had a stable symmetrycal penumbra. The tail sunspots were gradually collapsing.
The opened bipolar group crossed the Sun disc since 27.11 to 10.12 along the low latitudes of the Northern hemisphere. The head and the tail sunspots had stable symmetrycal penumbraes. The head sunspot was gradually bifurcating.
The big bipolar group crossed the Sun disc since 29.11 to 10.12 along the 20th parallel of the Southern hemisphere. The isolated sunspot with a stable symmetrycal penumbra was feature of the group which was situated to the North from the head group's part. This sunspot was gradually decreasing. The head group's part consisted of two closely located sunspot with a common oblong penumbra. The tail sunspots were gradually collapsing. Neighboring the central meridian the total region's area reached 600 m.h.s., and it was counted more thirty sunspots in the group.
The small sunspot with a stable symmetrycal penumbra crossed the Sun disc since 29.11 to 11.12 along the 18th parallel of the Northern hemisphere. Time to time pores and fine sunspots of an opposite magnetic polarity appeared neighboring the sunspot.
The fine sunspots crossed the Sun disc since 3.12 to 14.12 along the 18th parallel of the Northern hemisphere. The main sunspot had a stable symmetrycal penumbra.
The short-time bipolar sunspots were noticed at the middle latitudes of the Southern hemisphere since 5.12 to 7.12, in the Eastern part of the Sun disc.
The double sunspot with common penumbra crossed the Sun disc since 8.12 to 20.12 along the middle latitudes of the Southern hemisphere. Neighboring the central meridian the total bipole's area reached 200 m.h.s.
The small sunspots crossed the Sun disc since 8.12 to 20.12 along the eighth parallel of the Northern hemisphere. In the first days the group had a bipolar configuration. The head sunspot had a stable symmetrycal penumbra. The tail pores had quickly collapsed.
The small bipolar group was observed since 18.12 to 27.12 to the East from the group 11381. The head sunspot had a stable penumbra, and tail sunspots were gradually collapsing.
The opened bipolar group crossed the Sun disc since 20.12 to 31.12 along the middle latitudes of the Northern hemisphere. The bipole consisted of a large head sunspot with a penumbra and fine tail sunspots which were gradually collapsing. Neighboring the central meridian the total region's area reached 500 m.h.s.
The small bipolar group crossed the Sun disc since 23.12.11 to 5.01.12 along the 18th parallel of the Southern hemisphere. The bipole changed a configuration, but the sunspot in the middle group's part had a stable penumbra. Neighboring the central meridian the total region's area reached 200 m.h.s.
The growing bipolar group was observed at the 20th parallel of the Southern hemisphere since 25.12 to 30.12, in the Western part of the Sun disc. Before the Western part the total bipole's area had reached 300 m.h.s.
The big bipolar group crossed the Sun disc since 28.12 to 10.01 along the 23rd parallel of the Southern hemisphere. The head sunspot had a large penumbra, and the group's axis had considerable inclination to a parallel. Tail sunspots were gradually collapsing. In the evolution's peak the total region area reached 500 m.h.s.
The noteciable bipolar group crossed the Sun disc since 2.01.12 to 15.01.12 along the 13th parallel of the Northern hemisphere. The head sunspot had a large penumbra, and the tail group's part consisted of fine sunspots. The maximal bipole's area reached 500 m.h.s.
The growing bipolar group was observed at the midlle latitudes of the Northern hemisphere since 5.01 to 12.01, in the Western part of the Sun disc. Before the Western limb the total region's area exceeded 500 m.h.s.
