The long bipolar group crossed the Sun disc since 25.01 to 5.02.02 along the low latitudes of the Northern hemisphere. The total region's area reached 600 m.s.h., and it was counted 50-60 sunspot in the group. The head and tail parts of the group consisted of developed sunspots with asymmetrical penumbra, and many fine sunspots and pores were settled between its.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 25.01 to 6.02.02 along the equator. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot. The total region's area reached 100 m.s.h.
The big bipolar group crossed the Sun disc since 26.01 to 8.02.02 along the mid latitudes of the Southern hemisphere. The total region's area reached 600 m.s.h., and it was counted 50-60 sunspots in the group. The multipole consisted of several big penumbra's pieces with embedded sunspots. The group was continuously changing the form.
The fine sunspot with symmetrical penumbra crossed the Sun disc since 28.01 to 8.02.02 along the tenth parallel of the Northern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
The crumbled chain of small sunspots were marked at the 27th parallel of the Southern hemisphere since 31.01 to 8.02.02. In the first days the total region's area exceeded 300 m.s.h.
The opened bipolar group crossed the Sun disc since 30.01 to 12.02.02 along the low latitudes of the Southern hemisphere. The tail sunspot had symmetrical penumbra. In the first days the total region's area reached 150 m.s.h.
The big sunspot with symmetrical penumbra crossed the Sun disc since 1.02 to 14.02.02 along the tenth parallel of the Northern hemisphere. The total region's area reached 250 m.s.h. From time to time pores with opposite magnetic polarity were observed neighbouring the sunspot.
The bipolar group crossed the Sun disc since 2.02 to 14.02.02 along the 26th parallel of the Southern hemisphere. The total region's area reached 200 m.s.h. The bipole consisted of the perceptible head sunspot with asymmetrical penumbra and fine tail sunspots.
The fine bipolar formation was observed at the mid latitudes of the Northern hemisphere since 2.02 to 6.02.02, in the Western part of the Sun disc. The head sunspot had symmetrical penumbra.
The insignificant bipolar sunspots were situated at the mid latitudes of the Northern hemisphere since 7.02 to 10.02.02, in the Eastern part of the Sun disc.
The perceptible bipolar group was observed at the mid latitudes of the Southern hemisphere since 8.02 to 15.02.02. The total region's area reached 350 m.s.h., and it was counted 25-30 sunspots in the group. The bipole consisted of the large head sunspot with asymmetrical penumbra and string of many fine sunspots and pores.
The perceptible sunspot with symmetrical penumbra was situated to the North from the big region 09825 since 9.02 to 21.02.02. The total sunspot's area reached 200 m.s.h.
The long bipolar group crossed the Sun disc since 8.02 to 21.02.02 along the mid latitudes of the Southern hemisphere. The total region's area reached 500 m.s.h., and it was counted 50-60 sunspots in the group. The group consisted of two big sunspots with asymmetrical penumbraes which were connected by a short pore's chain. Another two chains of many fine sunspots and pores adjoined to the main sunspots from the East and the West.
The big bipolar group crossed the Sun disc since 14.02 to 26.02.02 along the high latitudes of the Southern hemisphere. The total region's area reached 700 m.s.h., and it was counted 40-50 sunspots in the group. The leading part of the group consisted of sunspot's solid chain, and the tail sunspot with penumbra was situated hardly to North.
The small bipolar group was marked at the low latitudes since 20.02 to 28.02.02. In the first days the total region's area reached 150 m.s.h. The head sunspot with asymmetrical penumbra was gradually bifurcating and decaying.
The growing bipolar group was observed at the mid latitudes of the Southern hemisphere since 20.02 to 28.02.02. The group consisted of many small sunspots which were regular changing the combination. Before set for the limb the total bipole's area reached 250 m.s.h.
The growing bipolar group was observed at the high latitudes of the Southern hemisphere since 22.02 to 1.03.02. Before set for the limb the total bipole's area reached 250 m.s.h.
The bipolar combination of many small sunspots was observed at the high latitudes of the Northern hemisphere since 23.02 to 4.03.02. The sunspot's quantity, the sunspot's form and the sunspot's combination had regular changes. The total region's area reached 150-200 m.s.h., and it was counted 20-25 sunspots in the group.
The big bipolar group crossed the Sun disc since 23.02 to 7.03.02 along the mid latitudes of the Northern hemisphere. In the first days the group consisted of three parts: the small head sunspot with symmetrical penumbra, and two tail sunspots with asymmetrical penumbraes which were connected by a short chain of pores. In next days the tail sunspots began extend and dispersed. Many fine sunspots with penumbraes appeared at the head sunspot's place. In the evolution's peak the total region's area reached 500 m.s.h., and it was counted 25-30 sunspots in the group.
The growing bipolar group was observed at the low latitudes of the Southern hemisphere since 22.02 to 28.02.02, in the Western part of the Sun disc. Before set for the limb the total region area reached 200 m.s.h.
The long chain of fine sunspots crossed the Sun disc since 28.02 to 11.03.02 along the low latitudes of the Southern hemisphere. From time to time the total region's area reached 100 m.s.h.
The short-time bipolar sunspots were observed at the mid latitudes of the Northern hemisphere on 3.03 and 4.03.02, to the East from the central meridian.
The perceptible sunspot with oblong penumbra crossed the Sun disc since 3.03 to 15.03.02 along the low latitudes of the Southern hemisphere. From time to time pores with opposite magnetic polarity were observed neighbouring the sunspot. The total region's area reached 200 m.s.h.
The short-time bipolar formation was marked at the thirtieth parallel of the Southern hemisphere since 4.03 to 6.03.02, neighbouring the central meridian.
The small sunspot with symmetrical penumbra was observed at the high latitudes of the Northern hemisphere since 7.03 to 19.03.02. From time to time fine tail sunspots with opposite magnetic polarity were marked.
The big bipolar group crossed the Sun disc since 8.03 to 22.03.02 along the tenth parallel of the Southern hemisphere. The head and tail parts of the group consisted of large sunspots with powerful penumbraes, and space between its was free for sunspots. In the first days the total region's area reached 1000 m.s.h.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 10.03 to 22.03.02 along the high latitudes of the Southern hemisphere. The fine tail sunspots were settled from the head sunspot on the considerable distance. The total region's area reached 150 m.s.h.
The opened bipolar group crossed the Sun disc since 13.03 to 25.03.02 along the high latitudes of the Southern hemisphere. The bipole consisted of two sunspots with symmetrical penumbraes. In the first days the tail sunspot was perceptibly more than the head sunspot. But the leading sunspot was gradually extending with siimultaneous curtailment of the supporting sunspot. The total region's area reached 300 m.s.h. Fine sunspots and pores appeared and disappeared neighbouring the main sunspots.
The small bipolar group was marked at the mid latitudes of the Southern hemisphere since 16.03 to 23.03.02. In the first days the total region's area reached 100 m.s.h.
The decaying bipolar group crossed the Sun disc since 19.03 to 28.03.02 along the high latitudes of the Southern hemisphere. In the first days the total region's area reached 150 m.s.h.
The spreading bipolar group crossed the Sun disc since 19.03 to 1.04.02 along the mid latitudes of the Southern hemisphere. The total region's area reached 200 m.s.h., and it was counted 25-30 sunspots in the group.
The bipolar chain of small sunspots crossed the Sun disc since 20.03 to 1.04.02 along the low latitudes of the Northern hemisphere. The total region's area reached 150 m.s.h.
The new eruptive group had appeared at the low latitudes of the Northern hemisphere on 20.03.02, in the Eastern part of the Sun disc. In the first days the group did not display perceptible activity. On 27.03 the new bipole began extend. In two days the total region's area exceeded 300 m.s.h. On 30.03 the new group reached the Western limb.
The small bipolar group was observed at the low latitudes of the Southern hemisphere since 22.03 to 28.03.02, in the Western part of the Sun disc. The tail sunspot had developed penumbra. The total region's area reached 150 m.s.h.
The small sunspot with symmetrical penumbra was observed at the low latitudes of the Northern hemisphere since 23.03 to 30.03.02, in the Eastern part of the Sun disc.
The small bipolar group was observed at the mid latitudes of the Southern hemisphere since 27.03 to 6.04.02. From time to time the total region's area reached 100 m.s.h.
The big bipolar group crossed the Sun disc since 27.03 to 8.04.02 along the mid latitudes of the Northern hemisphere. The group consisted of developed head and tail sunspots which were connected by long and solid chain of more fine sunspots. Neighbouring the central meridian the total region's area exceeded 700 m.s.h., and it was counted more 30 sunspots in the group.
The perceptible bipolar group was situated between the big regions 09885 and 09887 since 29.03 to 8.04.02. The total region's area reached 100-150 m.s.h., and it was counted more twenty sunspots in the group.
The multipolar sunspot's development was observed at the Sun equator since 29.03 to 10.04.02. The group's extension began in the head sunspot, and then it enveloped all the group. Neighbouring the central meridian the total region's area had exceeded 700 m.s.h. In next days slow collapse of the multipolar structure was outlined.
The perceptible bipolar group crossed the Sun disc since 29.03 to 10.04.02 along the mid latitudes of the Southern hemisphere. The bipole consisted of the developed head sunspot with asymmetrical penumbra and gradually decaying tail sunspots. The total region's area exceeded 200 m.s.h.
The long multipolar chain crossed the Sun disc since 3.04 to 16.04.02 along the high latitudes of the Northern hemisphere. The group consisted of the large head sunspots and string of more fine sunspots. The total region's area reached 500 m.s.h., and it was counted more 30 sunspots in the group.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 6.04 to 18.04.02 along the high latitudes of the Northern hemisphere. Fine sunspots and pores with opposite magnetic polarity were observed neighbouring the sunspot. The total region's area reached 200-300 m.s.h.
