The developing bipolar chain adjoined to the giant region 09393 from the East. The group was observed since 24.03 to 5.04.01. The mors developed sunspots was settled in the tail group's part. From time to time the total chain's area exceeded 250 m.s.h., and it was counted 25-30 sunspots in the group.
The perceptible sunspot with penumbra crossed the Sun disc since 26.03 to 6.04.01 along the low latitudes of the Southern hemisphere. Neighbouring the central meridian the sunspot had suddenly crumbled into more fine sunspots. In the first days the total sunspot's area reached 100 m.s.h.
The triangle combination of small sunspots was slowly decaying at the mid latitudes of the Southern hemisphere since 22.03 to 30.03.01. In the first days the total bipole's area exceeded 200 m.s.h.
The big sunspot with oblong penumbra crossed the Sun disc since 28.03 to 9.04.01 along the 25th parallel of the Northern hemisphere. The total sunspot's area reached 250 m.s.h.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 28.03 to 9.04.01 along the tenth parallel of the Northern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot. The total sunspot's area reached 100 m.s.h.
The perceptible bipolar chain crossed the Sun disc since 28.03 to 6.04.01 along the low latitudes of the Southern hemisphere. The bipole consisted of the head sunspot with oblong penumbra and the long string of fine sunspots and pores. From time to time the total region's area reached 400 m.s.h., and it was counted 30-35 sunspots in the group.
The small bipolar group was observed at the tenth parallel of the Northern hemisphere since 1.04 to 6.04.01, in the Western part of the Sun disc. The total region's area exceeded 100 m.s.h.
The big bipolar group crossed the Sun disc since 3.04 to 16.04.01 along the high latitudes of the Southern hemisphere. The head and tail sunspots had powerful penumbraes. From time to time the total region's area exceeded 1000 m.s.h., and it was counted 30-35 sunspots in the group. The tail sunspots were gradually decaying.
The fast development of the bipolar region was observed at the low latitudes of the Southern hemisphere since 3.04 to 14.04.01. The maximal total bipole's area reached 300 m.s.h., and it was counted 20-25 sunspots in the group.
The perceptible bipolar group crossed the Sun disc since 4.04 to 16.04.01 along the 26th parallel of the Northern hemisphere. The bipole consisted of the perceptible head sunspot with stable penumbra and fine tail sunspots. The total region's area reached 250 m.s.h.
The small sunspot with symmetrical penumbra crossed the Sun disc since 5.04 to 17.04.01 along the low latitudes of the Southern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
The small bipolar group was noticed at the low latitudes of the Southern hemisphere since 11.04 to 18.04.01. The head sunspot had symmetrical penumbra.
The small sunspot with symmetrical penumbra crossed the Sun disc since 13.04 to 25.04.01 along the low latitudes of the Northern hemisphere. In the first days the total sunspot's area exceeded 100 m.s.h.
The short-time bipolar sunspots were noticed at the mid latitudes of the Southern hemisphere since 16.04 to 18.04.01, in the Western part of the Sun disc.
The small bipolar group was observed at the low latitudes of the Northern hemisphere since 17.04 to 26.04.01. The head sunspot had symmetrical penumbra. From time to time the total bipole's area reached 100 m.s.h.
The long multipolar group crossed the Sun disc since 18.04 to 2.05.01 along the mid latitudes of the Northern hemisphere. The head group's part consisted of two big sunspots with penumbraes and many fine sunspots neighbouring its. The tail part was presented by the big sunspot with penumbra, and the long and solid chain of small sunspots and pores adjoined it from the South. The chain was gradually curving and crumbling. Neighbouring the central meridian the total region's area exceeded 1100 m.s.h., it was counted more 60 sunspots in the group, and longitude's lenght of the multipole exceeded 25 degrees.
The small bipolar sunspots were marked at the high latitudes of the Northern hemisphere since 18.04 to 22.04.01. The head sunspot had symmetrical penumbra.
The bipolar combination of two perceptible sunspots with symmetrical penumbraes was observed at the high latitudes of the Southern hemisphere since 19.04 to 28.04.01. The total bipole's area reached 200 m.s.h.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 21.04 to 4.05.01 along the tenth parallel of the Southern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot. The total sunspot's area reached 200 m.s.h.
The fine sunspot with symmetrical penumbra crossed the Sun disc since 21.04 to 30.04.01 along the tenth parallel of the Northern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
The big bipolar group crossed the Sun disc since 26.04 to 6.05.01 along the low latitudes of the Northern hemisphere. The bipole consisted of the big head sunspot with penumbra and many fine sunspots in the tail group's part. The total region's area reached 300 m.s.h., and it was counted 25-30 sunspots in the group.
The insignificant bipolar sunspots were observed at the tenth parallel of the Southern hemisphere since 28.04 to 4.05.01, in the Eastern part of the Sun disc.
The long chain of decaying sunspots crossed the Sun disc since 28.04 to 10.05.01 along the 25th parallel of the Northern hemisphere. From time to time the total region's area reached 450 m.s.h., and it was counted more thirty sunspots in the group.
The quick-growing sunspot's chain was observed at the mid latitudes of the Northern hemisphere since 29.04 to 7.05.01. The bipole consisted of the head sunspot with developed penumbra and string of many sunspots and pores. Before set for the limb the total region's area exceeded 250 m.s.h.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 1.05 to 13.05.01 along the high latitudes of the Northern hemisphere. From time to time pores of opposite magnetic polarity appeared neighbouring the sunspot. The total sunspot's area reached 150 m.s.h.
The small sunspot with penumbra crossed the Sun disc since 2.05 to 12.05.01 along the mid latitudes of the Southern hemisphere. In the first days the total sunspot's area reached 100 m.s.h.
The perceptible sunspot with penumbra crossed the Sun disc since 4.05 to 17.05.01 along the high latitudes of the Southern hemisphere. From time to time pores of opposite magnetic polarity appeared neighbouring the sunspot. The total sunspot's area reached 200 m.s.h.
The decaying bipolar group crossed the Sun disc since 10.05 to 20.05.01 along the mid latitudes of the Northern hemisphere. The bipole consisted of the perceptible head and tail sunspots, and fine sunspots between its. From time to time the total region's area exceeded 400 m.s.h., and it was counted more twenty sunspots in the group.
The curved chain of small sunspots with developed penumbraes was observed at the mid latitudes of the Southern hemisphere since 10.05 to 19.05.01. The total region's area reached 250 m.s.h., and it was counted 20-25 sunspots in the group.
The small bipolar group was observed at the low latitudes of the Northern hemisphere since 11.05 to 17.05.01, in the Western part of the Sun disc. From time to time the total bipole's area exceeded 100 m.s.h.
The perceptible bipolar group crossed the Sun disc since 15.05 to 27.05.01 along the high latitudes of the Northern hemisphere. The bipole was oriented along a meridian. In the first days the total region's area reached 200 m.s.h. The group was gradually decaying.
The small sunspot with symmetrical penumbra was marked to the North-West from the big region 09462 since 17.05 to 29.05.01. From time to time the total sunspot's area reached 100 m.s.h.
The fast development of the big bipolar region was observed at the low latitudes of the Northern hemisphere since 18.05 to 29.05.01. The bipole consisted of the large head sunspot with penumbra and the rapid developing string of many small sunspots and pores. Neighbouring the central meridian the total region's area exceeded 700 m.s.h., and it was counted more thirty sunspots in the group. After intersection of the central meridian the sunspot's string began rapidly decay.
The small sunspot with symmetrical penumbra crossed the Sun disc since 20.05 to 31.05.01 along the low latitudes of the Southern hemisphere. From time to time the total sunspot's area reached 100 m.s.h.
The spreading bipolar group crossed the Sun disc since 21.05 to 1.06.01 along the low latitudes of the Northern hemisphere. In the first days the total region's area reached 200 m.s.h., and it was counted 20-25 sunspots in the group. After intersection of the central meridian the bipole began decay.
The crumbled chain of small sunspots crossed the Sun disc since 26.05 to 7.06.01 along the mid latitudes of the Northern hemisphere. The most developed tail sunspot displayed recurrent activity. After the chain's decay many fine sunspots and pores began appeared neighbouring the sunspot. From time to time the total region's area reached 200 m.s.h.
The fast development of the bipolar region took a place at the low latitudes of the Southern hemisphere since 1.06 to 10.06.01. The group consisted of three active centers. The stable head sunspot with penumbra was gradually assuming symmetrical form, and rest sunspots began decay after short development. The maximal total bipole's area reached 400 m.s.h., and it was counted 20-25 sunspots in the group.
The fast development of the bipolar region took a place at the 28th parallel of the Northern hemisphere since 1.06 to 8.06.01, in the Western part of the Sun disc. In the evolution's peak the total group's area reached 200 m.s.h.
The big sunspot with asymmetrical penumbra was slowly crumbling at the high latitudes of the Northern hemisphere since 2.06 to 15.06.01. From time to time the total region's area reached 400 m.s.h.
The solid and slowly crumbled chain of small sunspots with developed penumbraes crossed the Sun disc since 3.06 to 14.06.01 along the high latitudes of the Southern hemisphere. In the first days the total region's area reached 400 m.s.h., and neighbouring the central meridian it was counted more twenty sunspots in the group.
The fast development of the bipolar region was observed at the mid latitudes of the Northern hemisphere since 4.06 to 15.06.01. The bipole consisted of the slowly growing head sunspot with asymmetrical penumbra and many fine sunspots and pores which appeared and disappeared behind the sunspot. In the evolution's peak the total region's area exceeded 200 m.s.h., and it was counted 35-40 sunspots in the group.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 5.06 to 18.06.01 along the 25th parallel of the Northern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot. The total sunspot's area exceeded 150 m.s.h.
The perceptible bipolar group was observed since 6.06 to 17.06 hardly to the South from the sunspot 09491. The bipole consisted of the duplex head sunspots with developed penumbraes and fine tail sunspots. In the first days the total region's area reached 300 m.s.h.
The unstable bipolar configuration crossed the Sun disc since 6.06 to 18.06.01 along the low latitudes of the Northern hemisphere. The bipole consisted of the head sunspot with symmetrical penumbra and fine tail sunspots which were parted by considerable longitude's distance. From time to time the total region's area reached 200 m.s.h.
The quick-growing bipolar group was marked at the low latitudes of the Southern hemisphere since 6.06 to 13.06.01, in the Western part of the Sun disc. The head sunspot with developed penumbra had bifurcated. The tail sunspots made composite figure. From time to time the total region's area reached 500 m.s.h.
The eruptive group crossed the Sun disc since 7.06 to 17.06.01 along the low latitudes of the Northern hemisphere. Before set for the limb the bipole began suddenly extend, and the total area reached 250 m.s.h.
The short-time bipolar sunspots were noticed at the low latitudes of the Northern hemisphere since 8.06 to 11.06.01, in the Western part of the Sun disc.
The small bipolar group was observed at the mid latitudes of the Northern hemisphere since 9.06 to 18.06.01. The region consisted of the head sunspot with symmetrical penumbra and unstable tail sunspots.
