The fine bipolar sunspots crossed the Sun disc since 4.01 to 15.01.01 along the low latitudes of the Northern hemisphere. The head sunspot had symmetrical penumbra.
The small sunspot with symmetrical penumbra crossed the Sun disc since 5.01 to 15.01.01 along the high latitudes of the Northern hemisphere. Pores of opposite magnetic polarity were observed neighbouring the sunspot. From time to time the total region's area exceeded 100 m.s.h.
The small sunspot with symmetrical penumbra crossed the Sun disc since 6.01 to 18.01.01 along the tenth parallel of the Northern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
The long chain of small sunspots with penumbraes crossed the Sun disc since 8.01 to 19.01.01 along the mid latitudes of the Northern hemisphere. In the evolution's peak the total region's area exceeded 500 m.s.h., and it was counted more 50 sunspots in the group.
The bipolar chain of fine sunspots crosssed the Sun disc since 15.01 to 25.01.01 along the low latitudes of the Northern hemisphere. Before set for the limb perceptible extension of the sunspots was observed when the total bipole's area exceeded 200 m.s.h.
The fine sunspot with symmetrical penumbra was observed at the low latitudes of the Northern hemisphere since 16.01 to 20.01.01, in the Eastern part of the Sun disc.
The perceptible bipolar group crossed the Sun disc since 18.01 to 29.01.01 along the low latitudes of the Southern hemisphere. The bipole consisted of the small tail sunspot with stable asymmetrical penumbra and fine head sunspots which were continuously changing the combination. The maximal total region's area exceeded 200 m.s.h., and it was counted 20-25 sunspots in the group.
The bipolar combination of the perceptible sunspot with penumbra and fine tail sunspots crossed the Sun disc since 19.01 to 29.01.01 along the mid latitudes of the Southern hemisphere. In the first days the total bipole's area reached 200 m.s.h.
The perceptible bipolar group crossed the Sun disc since 21.01 to 1.02.01 along the low latitudes of the Southern hemisphere. The total region's area exceeded 250 m.s.h., and it was counted 30-35 sunspots in the group. The group consisted of several parts and was continuously changing the configuration.
The fine sunspot with penumbra crossed the Sun disc since 25.01 to 4.02.01 along the tenth parallel of the Northern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
The short-time bipolar sunspots were noticed at the 27th parallel of the Northern hemisphere since 26.01 to 29.01.01, in the Western part of the Sun disc.
The fine bipolar sunspots were marked at the tenth parallel of the Southern hemisphere since 29.01 to 3.02.01, in the Eastern part of the Sun disc. The head sunspot had symmetrical penumbra.
The perceptible bipole crossed the Sun disc since 30.01 to 11.02.01 along the 26th parallel of the Northern hemisphere. The group consisted of the head sunspot with stable symmetrical penumbra and small tail sunspots. In the first days the total region's area exceeded 200 m.s.h., and it was counted 10-15 sunspots in the group.
The curved chain of small sunspots with developed penumbraes crossed the Sun disc since 1.02 to 12.02.01 along the mid latitudes of the Northern hemisphere. From time to time the total region's area exceeded 200 m.s.h., and it was counted 15-20 sunspots in the group.
The perceptible bipolar group adjoined to the region 09334 from the East. The bipole was observed since 3.02 to 14.02.01. In the first days the total region's area exceeded 100 m.s.h.
The fast development of the bipolar region was observed at the high latitudes of the Southern hemisphere. Neighbouring the central meridian the total region's area exceeded 200 m.s.h., and it was counted more twenty sunspots in the group.
The opened bipolar group crossed the Sun disc since 4.02 to 16.02.01 along the tenth parallel of the Southern hemisphere. The bipole consisted of the perceptible head and tail sunspots with penumbraes. In the first days the total region's area reached 300 m.s.h. After intersection of the central meridian the tail sunspots decayed, and the head sunspot assumed symmetrical form and reached the Western limb.
The short-time bipolar sunspots were noticed at the thirtieth parallel of the Northern hemisphere since 8.02 to 10.02.01, to the East from the central meridian.
The perceptible bipolar group were marked at the low latitudes of the Southern hemisphere since 16.02 to 26.02.01. The bipole was continuously changing the form. The maximal total region's area reached 250 m.s.h., and it was counted 15-20 sunspots in the group.
The perceptible bipolar group crossed the Sun disc since 20.02 to 4.03.01 along the mid latitudes of the Northern hemisphere. The bipole consisted of two nearby sunspots with symmetrical penumbraes which had meridianal orient. Many pores appeared and disappeared behind the sunspot. From time to time the total region's area reached 250 m.s.h., and it was counted more twenty sunspots in the group.
The fine sunspot with symmetrical penumbra crossed the Sun disc since 20.02 to 2.03.01 along the tenth parallel of the Southern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
The insignificant bipolar group was observed at the tenth parallel of the Southern hemisphere since 28.02 to 5.03.01, in the Western part of the Sun disc.
The fine bipolar sunspots were observed at the tenth parallel of the Southern hemisphere since 28.02 to 9.03.01. The head sunspot had symmetrical penumbra.
The fine sunspot with symmetrical penumbra was observed at the tenth parallel of the Northern hemisphere since 1.03 to 7.03.01, in the Eastern part of the Sun disc.
The big bipolar group crossed the Sun disc since 2.03 to 12.03.01 along the 26th parallel of the Northern hemisphere. The head and tail sunspots had developed asymmetrical penumbraes. The maximal total region's area reached 700 m.s.h., and it was counted more twenty sunspots in the group.
The developing bipolar group crossed the Sun disc since 3.03 to 14.03.01 along the tenth parallel of the Northern hemisphere. The bipole consisted of the fine head sunspot with symmetrical penumbra and the solid tail chain of small sunspots with penumbraes. In the evolution's peak the total region's area reached 200 m.s.h., and it was counted more twenty sunspots in the group.
The long chain of small sunspots and pores crossed the Sun disc since 9.03 to 22.03.01 along the low latitudes of the Southern hemisphere. The bipole consisted of the small head sunspot with stable symmetrical penumbra and long spreading string of fine sunspots and pores. After intersection of the central meridian the string began decay, and new sunspots with penumbraes appeared in the tail group's part. From time to time the total region's area exceeded 300 m.s.h., and it was counted more thirty sunspots in the group.
The fine sunspot with symmetrical penumbra was marked at the thirtieth parallel of the Northern hemisphere on 12.03 and 13.03.01, in the Eastern part of the Sun disc.
The recurrent bipolar sunspots were noticed at the mid latitudes of the Southern hemisphere since 13.03 to 19.03.01, in the Eastern part of the Sun disc.
The small bipolar group was marked at the tenth parallel of the Northern hemisphere since 14.03 to 20.03.01, in the Western part of the Sun disc. From time to time the total region's area reached 150 m.s.h.
The fast development of the bipolar region was observed at the low latitudes of the Northern hemisphere since 19.03 to 30.03.01. The bipole consisted of the extending head sunspot with symmetrical penumbra and unstable tail sunspots. The total region's area excceeded 150 m.s.h.
The long bipolar group crossed the Sun disc since 20.03 to 1.04.01 along the mid latitudes of the Southern hemisphere. The bipole consisted of the small head sunspot with symmetrical penumbra and small tail sunspots with penumbraes which formed a bipolar figure. In the first days the total region's area reached 200 m.s.h. In next days fine bipoolar sunspots appeared at the head sunspot's place, and the whole group was gradually dissolving against the Sun disc.
The spreading bipolar group crossed the Sun disc since 20.03 to 1.04.01 along the mid latitudes of the Northern hemisphere. The main sunspots had small penumbraes, and more fine sunspots and pores were settled between and behind its. The bipole was gradually decaying, and the head sunspot with stable penumbra reached the Western limb. In the first days the total region's area exceeded 200 m.s.h., and neighbouring the central meridian it was counted 20-25 sunspots in the group.
The giant multipolar group crossed the Sun disc since 22.03 to 4.04.01 along the mid latitudes of the Northern hemisphere. Neighbouring the central meridian the total region area reached 2500 m.s.h., and it was counted more 50 sunspots in the group. The multipole consisted of several large pieces of penumbra which were stretched as a chain along a parallel.
The slowly growing bipolar sunspots were observed at the low latitudes of the Southern hemisphere since 24.03 to 30.03.01, in the Western part of the Sun disc. Before set for the limb the total region's area reached 300 m.s.h.
The perceptible bipolar group crossed the Sun disc since 24.03 to 5.04.01 along the low latitudes of the Southern hemisphere. Neighbouring the central meridian the total region's area reached 300 m.s.h., and it was counted 20-25 sunspots in the group. The bipole consisted of the head sunspot with stable penumbra and short curved chain of developed sunspots.
The short-time bipolar sunspots were marked at the high latitudes of the Northern hemisphere since 24.03 to 26.03.01, neighbouring the central meridian.
