The fine bipolar sunspots were marked at the tenth parallel of the Northern hemisphere since 11.06 to 20.06.01. From time to time the total bipole's area reached 100 m.s.h.
The small sunspot with asymmetrical penumbra crossed the Sun disc since 11.06 to 23.06.01 along the mid latitudes of the Southern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot, and the total region's area reached 150 m.s.h.
The triangle combination of small sunspots and pores was decaying at the 25th parallel of the Southern hemisphere since 12.06 to 20.06.01, in the Eastern part of the Sun disc. In the first days the total region's area reached 200 m.s.h.
The long chain of developed sunspots and pores crossed the Sun disc since 12.06 to 25.06.01 along the mid latitudes of the Northern hemisphere. From time to time the total region's area reached 600 m.s.h., and it was counted 40-45 sunspots in the group.
The double sunspot with powerful asymmetrical penumbra was marked since 13.06 to 26.06.01 hardly to the South-East from the big region 09503. The total sunspot's area exceeded 300 m.s.h.
The long bipolar group followed the big region 09503 since 14.06 to 27.06.01. The bipole consisted of the developed head sunspot with penumbra and fine tail sunspots which were parted by considerable longitude's distance. From time to time the total region's area exceeded 300 m.s.h.
The triangle combination of fine sunspots and pores was observed at the tenth parallel of the Southern hemisphere since 19.06 to 24.06.01, in the Western part of the Sun disc.
The fast bipolar group's development was marked at the tenth parallel of the Northern hemisphere since 19.06 to 30.06.01. 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 fast bipolar region's development was observed at the high latitudes of the Southern hemisphere since 21.06 to 29.06.01. The total region's area reached 250 m.s.h., and it was counted more 30 sunspots in the group.
The long bipolar group crossed the Sun disc since 21.06 to 3.07.01 along the high latitudes of the Northern hemisphere. The bipole consisted of a small head sunspot with symmetrical penumbra and decaying tail sunspots. In the first days the total region's area reached 200 m.s.h.
The small sunspot with symmetrical penumbra was marked since 22.06 to 30.06.01 hardly to the South from the bipolar region 09513. Pores of opposite magnetic polarity were observed neighbouring the sunspot. From time to time the total group's area reached 100 m.s.h.
The fast development of a bipolar region was observed at the low latitudes of the Southern hemisphere since 23.06 to 3.07.01. The bipole consisted of a stable sunspot with symmetrical penumbra and a small string of fine sunspots. In the first days the total group's area reached 150 m.s.h.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 23.06 to 5.07.01 along the tenth parallel of the Northern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot. The total region's area reached 200 m.s.h.
The short-time bipolar pores were noticed at the mid latitudes of the Northern hemisphere on 27.06 and 28.06.01, to the East from the central meridian.
The small bipolar group was noticed at the 50th parallel of the Southern hemisphere since 29.06 to 5.07.01. In the first days the total region's area reached 150 m.s.h.
The fine sunspot with symmetrical penumbra was observed at the low latitudes of the Northern hemisphere since 1.07 to 4.07.01, in the Eastern part of the Sun disc.
The perceptible sunspot with asymmetrical penumbra crossed the Sun disc since 1.07 to 11.07.01 along the mid latitudes of the Southern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot. The total region's area reached 150 m.s.h.
The fine sunspot with symmetrical penumbra and tail sunspots were observed at the low latitudes of the Northern hemisphere since 2.07 to 7.07.01, in the Eastern part of the Sun disc.
The small sunspot with symmetrical penumbra crossed the Sun disc since 3.07 to 15.07.01 along the low latitudes of the Northern hemisphere. From time to time fine sunspots and pores of opposite magnetic polarity were observed neighbouring the sunspot.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 10.07 to 22.07.01 along the low latitudes of the Northern hemisphere. The total sunspot's area reached 150 m.s.h.
The big sunspot with symmetrical penumbra crossed the Sun disc since 11.07 to 24.07.01 along the mid latitudes of the Northern hemisphere. The total sunspot's area exceeded 200 m.s.h.
The growing bipolar group was observed at the mid latitudes of the Southern hemisphere since 12.07 to 20.07.01. The bipole consisted of the head sunspot with developed penumbra and a string of fine sunspots and pores. The total region's area reached 200 m.s.h., and it was counted 20-25 sunspots in the group.
The perceptible sunspot with symmetrical penumbra and fine tail sunspots followed the region 09538 since 13.07 to 24.07.01. In the first days the total region's area reached 150 m.s.h.
The developing chain of bipolar sunspots crossed the Sun disc since 15.07 to 28.07.01 along the high latitudes of the Southern hemisphere. The total region's area exceeded 200 m.s.h., and from time to time it was counted 40-50 sunspots in the group.
The fast development of the bipolar region was observed at the mid latitudes of the Northern hemisphere since 17.07 to 29.07.01. After intersection of the central meridian the bipole had decayed, and the head sunspot with symmetrical penumbra reached the Western limb.
The fast development of the bipolar region had observed at the mid latitudes of the Northern hemisphere since 23.07 to 29.07.01. In the evolution's peak the total region's area reached 200 m.s.h.
The perceptible eruptive group crossed the Sun disc since 26.07 to 8.08.01 along the high latitudes of the Southern hemisphere. In the first days the region did not display activity. After intersection of the central meridian the sunspots began suddenly extend, and in several days its acquired a general penumbra. Before set for the limb the total region's area exceeded 500 m.s.h.
The small bipolar sunspots crossed the Sun disc since 29.07 to 9.08.01 along the mid latitudes of the Southern hemisphere. The head and the tail sunspots were parted by considerable longitude's distance. Before set for the limb the head sunspot had decayed.
The decaying bipolar group crossed the Sun disc since 30.07 to 9.08.01 along the low latitudes of the Northern hemisphere. The bipole consisted of the head sunspot with asymmetrical penumbra and fine tail sunspots. In the first days the total region's area reached 200 m.s.h.
The quick-growing multipolar group crossed the Sun disc since 31.07 to 12.08.01 along the 25th parallel of the Northern hemisphere. The multipole consisted of many developed sunspots with penumbraes which were gradually lining along a parallel. From time to time the total region's area exceeded 500 m.s.h., and it was counted 20-25 sunspots in the group.
The developed bipolar group crossed the Sun disc since 1.08 to 13.08.01 to the South-East from the big region 09563. The group consisted of perceptible head and tail sunspots with developed penumbraes which were connected by a chain of fine sunspots and pores. The total region's area reached 250 m.s.h., and it was counted 20-25 sunspots in the group.
The small bipolar sunspots were observed at the mid latitudes of the Southern hemisphere since 1.08 to 9.08.01. The head and the tail sunspots were parted by considerable longitude's sunspots. From time to time the total region's area reached 100 m.s.h.
The fast development of the bipolar group was observed at the mid latitudes of the Southern hemisphere since 4.08 to 13.08.01, in the Western part of the Sun disc. The bipole consisted of the growing head sunspot with asymmetrical penumbra and fine tail sunspots with penumbraes. In the evolution's peak the total region's area exceeded 200 m.s.h.. and it was counted twenty sunspots in the group.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 5.08 to 17.08.01 along the tenth parallel of the Southern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot. The total region's area reached 300 m.s.h.
The decaying bipolar group crossed the Sun disc since 8.08 to 20.08.01 along the low latitudes of the Southern hemisphere. In the first days the total region's area reached 150 m.s.h. The head sunspot with symmetrical penumbra reached the Western limb.
The new bipolar group appeared on 10.08.01 hardly to the North from the region 09570. The main sunspots were perceptible developing and dispersing. The most sunspot was settled in the tail group's part. In the evolution's peak the total bipole's area reached 400 m.s.h. On 17.08 the group had come to the Western limb.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 11.08 to 23.08.01 along the tenth parrallel of the Northern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot. The total region's area reached 200 m.s.h.
The fine sunspot with symmetrical penumbra was observed at the high latitudes of the Southern hemisphere since 13.08 to 18.08.01, to the West from the central meridian. The sunspot drifted from 17th to 24th parallel.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 14.08 to 27.08.01 along the 25th parallel of the Northern hemisphere. From time to time the total sunspot's area reached 200 m.s.h.
The fine bipolar sunspots were observed at the 25th parallel of the Southern hemisphere since 15.08 to 20.08.01, to the West from the central meridian.
The fast development of the bipolar group was marked since 15.08 to 24.08.01 to the East from the region 09580. In the evolution's peak the total bipole's area reached 150 m.s.h., and it was counted 20-25 sunspots in the group.
The fast development of the bipolar group was observed at the mid latitudes of the Northern hemisphere since 16.08 to 28.08.01. The head group's part consisted of the double sunspot with developed penumbra. The fine tail sunspots had general irregular penumbra. There were separate sunspots in the central group's part. From time to time the total region's area reached 300 m.s.h., and it was counted 20-25 sunspots in the group.
The short-time bipolar sunspots were marked at the mid latitudes of the Southern hemisphere since 16.08 to 18.08.01, in the Western part of the Sun disc.
The fine sunspots were observed at the tenth parallel of the Southern hemisphere since 17.08 to 28.08.01. Before set for the limb the new group began suddenly extend.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 20.08 to 1.09.01 along the 29th parallel of the Southern hemisphere. From time to time the total sunspot's region reached 200 m.s.h.
The big bipolar group crossed the Sun disc since 21.08 to 4.09.01 along the high latitudes of the Southern hemisphere. The bipole consisted of three parts. The small head and central sunspots were gradually decaying. The tail part of the group consisted of large sunspots with general irregular penumbra. From time to time the total region's area reached 1000 m.s.h.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 25.08 to 7.09.01 along the high latitudes of the Northern hemisphere. The total sunspot's area reached 200 m.s.h.
The opened bipolar group crossed the Sun disc since 27.08 to 6.09.01 along the mid latitudes of the Southern hemisphere. The head sunspot had developed symmetrical penumbra. The tail part of the group consisted of fine sunspots with genersl penumbra which decayed later. Neighbouring the central meridian the total region's area reached 250 m.s.h.
