The single sunspot with fine penumbra was crossed the Sun disc since 25.08 to 6.09 across the middle latitudes of the Northern hemisphere. Time to time the total sunspot area exceeded 100 m.h.s.
The small bipolar group was marked at the phase moderate development since 3.09 to 8.09 at the middle latitudes of the Northern hemisphere, in the Western part of the Sun disc.
The long shain of fine sunspots was crossed the Sun disc since 11.09 to 21.09 along the high latiudes of the Southern hemisphere. The head sunspot had a stable symmetrical penumbra.
The pair of the close located large sunspots with developed penumbraes was crossed the Sun disc since 16.09 to 28.09 along the high latiudes of the Southern hemisphere. Time to time the total group's area exceeded 400 m.h.s., and sunspo's number reached fifteen units.
The long shain of the developed sunspots was crossed the Sun disc since 22.09 to 3.10 along the high latitudes of the Northern hemisphere. The larg head sunspot had a developed penumbra. In process of advance on the Sun disc the sunspot shain was gradually broken up. Time to time the total group's area exceeded 400 m.h.s., and sunspot's number reached twenty five units.
The stable sunspot with the symmetrical penumbra crossed the Sun disc since 16.10 to 28.10 along the 30th parallel of the Southern hemisphere. Time to time neighboring the sunspot there were pores of opposite magneic polarity, and the total group's area reached 200 m.h.s.
The developing bipolar group crossed the Sun disc since 20.10 to 31.10 along the high latitudes of the Northern hemisphere. The group appeared near the Eastern limb as a developed sunspot with symmetrical penumbra. Three days later to the South from the single umbra there was a new sunspots shain, its development had finished by formation of head and tail sunspots with large penumbraes. Near the Western limb the total region's area reached 500 m.h.s., and in the group it was counted thirty sunspots.
The bipolar cloud of fine sunspots were marked at the high latitudes of the Southern hemisphere since 10.11 to 16.11. In the group it was counted ten-fifteen sunspots whereas the total area of the region didn't exceed hundred m.h.s.
The growing bipolar group had arisen on 9.11 at the fifteen parallel of the Northern hemisphere, not far from the Eastern limb. In the process of development head and tail sunspots increased and gradually got a symmetrical form. Time to time the total region's area exceeded 300 m.h.s., and in the group it was counted not over ten-fifteen sunspots. On 19.11 the bipole reached the Western limb.
The small bipolar group crossed the Sun disc since 12.11 to 23.11 along the 30th parallel of the Southern hemisphere. The bipole had an arrow-shaped configuration, main sunspots had fine symmetrical penumbraes. The total region's area didn't exceed hundred m.h.s., in the group it was counted not over ten sunspots.
The single sunspot with a stable symmetrical penumbra crossed the Sun disc since 16.11 to 27.11 along the 25th parallel of the Northern hemisphere. Time to time neighboring the sunspot there were pores of a opposite magnetic polarity.
The new bipolar group had appeared at the middle latitudes of the Northern hemisphere on 29.11, neighbouring the central meridian. In the process of development the total region's area exceeded 30 m.h.s., in the group it was counted fifteen sunspots. On 5.12 the head sunspot reached the Western limb.
The large sunspot with a stable symmetrical penumbra crossed the Sun disc since 1.12 to 14.12 along 30th parallel of the Northern hemisphere. The maximal total sunspot's area exceeded 400 m.h.s.
The noticeable sunspot with a stable symmetrical penumbra crossed the Sun disc since 1.01 to 12.01.11 along 33rd parallel of the Northern hemisphere. Time to time there were pores of a opposite magnetic polarity neighboring the sunspot, and total region's area reached 200 m.h.s.
The small bipolar group appeared at the high latitudes of the Northern hemisphere on 16.01, not far from the Eastern limb. The head sunspot had a stable symmetrical penumbra, and tail sunspots were gradually desintegrated. On 27.01 the group reached the Western limb.
The growing multipolar group was appeared at the 20th parallel of the Southern hemisphere on 12.02, neighboring the central meridian. The new group consisted of three parts with developed sunspots and penumbraes. The head sunspots had a stable symmetrical penumbra. In the evolution peak the total region's area exceeded 600 m.h.s., and in the group it was counted more thirty sunspots. On 21.02 the multipole reached the Western limb.
The noticeable bipolar group crossed the Sun disc since 15.02 to 25.02 along the tenth parallel of the Northern hemisphere. In the evolution peak the total region's area reached 250 m.h.s., in the group it was counted forty sunspots about.
The large multipolar group crossed the Sun disc since 26.02 to 9.03 along the high latitudes of the Northern hemisphere. Main sunspots of the multipole formed triangle with a right angle in the South-Western direction. Between the main sunspots it was observed numerous pores and small spots. The magnetic design of the group underwent continuous changes. Before the Western limb the multipole took a freakish form of a huge butterfly. In the evolution peak the total region's area exceeded 750 m.h.s., and in the group it was counted forty sunspots about.
The small bipolar sunspots crossed the Sun disc since 27.02 to 8.03 along the high latitudes of the Southern hemisphere. Before the Western limb the group had unexpected development.
The big bipolar group crossed the Sun disc since 3.03 to 15.03 along the tenth parallel of the Northern hemisphere. The head sunspot had a stable symmetrical penumbra, and the bipole had an arrow-shaped form. In the evolution peak the total region's area reached 750 m.h.s., and in the group it was counted fifty sunspots about.
The noticeable bipolar group crossed the Sun disc since 7.03 to 17.03 along the 20th parallel of the Northern hemisphere. The bipole consisted of several clusters of small sunspots which were rearranged relatively each other. Head sunspots were gradually increased, other parts of the group broke up. Before the western limb the total area of the head sunspots exceeded 300 m.h.s., and neighboring the central meridian in the group it was counted more twenty sunspots.
The big bipolar group crossed the Sun disc since 22.03 to 3.04 along the middle latitudes of the Southern hemisphere. The bipole consisted of the head sunspot with a stable penumbra and the tail sunspots with a oblong penumbra which had separated from each other. In the evolution process intermediate sunspots disappeared, and in the tail part there was one sunspot with a penumbra. In the evolution's peak the total region's area exceeded 400 m.h.s., and in the group it was counted thirty sunspots about.
The noteciable bipolar group crossed the Sun disc since 28.03 to 7.04 along the 15th parallel of the Northern hemisphere. A spot which was situated in the middle part of the group was gradually approached and merge with the head sunspot. Tail sunspots formated a triangle configuration, then its desintegrated. In the evolution's peak the total region's area exceeded 300 m.h.s., and in the group it was counted not over twenty sunspots.
The small bipolar group was observed at the 15th parallel of the Northern hemisphere since 2.04 to 10.04. Before the Western limb its tail part had collapsed.
The fast-growing group was observed at the middle latitudes of the Northern hemisphere since 12.04 to 19.04, in the Western part of the Sun disc. The multipole appeared neighboring the central meridian and consisted of three sunspot's clusters. Head and intermediate parts of the group united subsequently and continued growth. Tail sunspots had no development and turned in disintegration. In the evolution peak the total region's area exceeded 400 m.h.s., and in the group it was counted more thirty sunspots.
The fine sunspot with a symmetrical penumbra crossed the Sun disc along the low latitdes of the Northern hemisphere since 13.04 to 24.04. Time to time there were pores with an opposite magnetic polarity neighboring the sunspot.
The noticeable bipolar group crossed the Sun disc since 14.04 to 26.04 along the middle latitudes of the Northern hemisphere. The head sunspot had a stable symmetrical penumbra. Neighboring the central meridian the total region's area reached 400 m.h.s., and in the group it was counted twenty sunspots about.
The noteciable bipolar group crossed the Sun disc since 20.04 to 1.05 along the middle latitudes of the Southern hemisphere. In first days the group consisted of three parts. Intermediate sunspots disappeared, and head and tail sunspots continued the growth. Over time the tail part was scattered, and the head sunspot got a symmetrical form. Time to time the total region's area reached 400 m.h.s.
The new bipolar group was developing at the 21st parallel of the Northern hemisphere since 27.04 to 2.05, in the Western part of the Sun disc. Before the Western limb the total region's area reached 200 m.h.s.