The large double sunspot with general irregular penumbra crossed the Sun disc since 14.11 to 26.11.01 along the high latitudes of the Southern hemisphere. Many fine sunspots and pores were observed neighbouring the sunspot. From time to time the total region's area reached 700 m.s.h., and it was counted 30-40 sunspots in the group.
The shapeless cloud of fine sunspots crossed the Sun disc since 21.11 to 1.12.01 along the mid latitudes of the Northern hemisphere. From time to time the total region's area reached 100 m.s.h.
The small bipolar formation was observed at the tenth parallel of the Southern hemisphere since 22.11 to 2.12.01. Before set for the limb the tail sunspot with penumbra began extend, and the total region's area exceeded 100 m.s.h.
The big bipolar group crossed the Sun disc since 23.11 to 6.12.01 along the low latitudes of the Northern hemisphere. In the evolution's peak the multipole had assumed closed configuration, the total area had exceeded 1000 m.s.h., and it was counted more 30 sunspots in the group.
The fine bipolar group crossed the Sun disc since 25.11 to 7.12.01 along the low latitudes of the Southern hemisphere. The head sunspot had symmetrical penumbra.
The perceptible sunspot with symmetricaal penumbra crossed the Sun disc since 27.11 to 9.12.01 along the low latitudes of the Northern hemisphere. Fine sunspots and pores of opposite magnetic polarity were observed to the East from the sunspot. The total region's area reached 250-300 m.s.h.
The big bipolar group crossed the Sun disc since 27.11 to 10.12.01 along the low latitudes of the Southern hemisphere. The multipole consisted of several large sunspots with asymmetrical penumbraes. The total region's area reached 700 m.s.h., and it was counted 25-30 sunspots in the group.
The small bipolar group crossed the Sun disc since 28.11 to 10.12.01. The bipole was outstanding because it was appreciably drifting to the South Pole, from the 17th to 28th parallel during the Sun disc's passing.
The asymmetrical sunspot with oblong penumbra crossed the Sun disc since 28.11 to 11.12.01 along the mid latitudes of the Northern hemisphere. Before set for the limb the sunspot had bifurcated. From time to time the total region's area exceeded 200 m.s.h.
The small sunspot with symmetrical penumbra crossed the Sun disc since 1.12 to 13.12.01 along the tenth parallel of the Northern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
The compact combination of big sunspots crossed the Sun disc since 3.12 to 15.12.01 along the high latitudes of the Southern hemisphere. The total regin's area reached 600 m.s.h., and it was counted more 30 sunspots in the group.
The short-time bipolar sunspots were observed at the 25th parallel of the Northern hemisphere since 6.12 to 9.12.01, in the Eastern part of the Sun disc.
The small sunspot with symmetrical penumbra crossed the Sun disc since 7.12 to 18.12.01 along the equator. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
The big bipolar group crossed the Sun disc since 7.12 to 20.12.01 along the mid latitudes of the Northern hemisphere. The group was regular changing the form, at times assuming fanciful contours. In the first days the tail part of the group was like a horseshoe. In the evolution's peak the total region's area reached 500 m.s.h., and it was counted more 50 sunspots in the group.
The fine sunspot with symmetrical penumbra was observed at the mid latitudes of the Southern hemisphere since 9.12 to 18.12.01. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
The opened bipolar group was observed at the mid latitudes of the Southern hemisphere since 13.12 to 20.12.01, in the Western part of the Sun disc. The head and tail parts of the group consisted of extending sunspots with penumbraes. Before set for the limb the total region's area exceeded 400 m.s.h.
The large multipolar group crossed the Sun disc since 15.12 to 28.12.01 along the low and the mid latitudes of the Northern hemisphere. Three big sunspots with penumbraes were as a base of the multipole and were settled by triangle. Many small sunspots and pores were observed between the sunspots. In the evolution's peak the total region's area exceeded 1000 m.s.h., and it was counted 60-70 sunspots in the group.
The perceptible sunspot with penumbra crossed the Sun disc since 16.12 to 28.12.01 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 150 m.s.h.
The growing bipolar group was observed to the East from the bipolar region 09743 since 20.12 to 30.12.01. The new region's increase had a place in the same time when the group 09743 was decreasing. Before set for the limb the total bipole's region reached 300 m.s.h.
The big bipolar group crossed the Sun disc since 20.12.01 to 2.01.02 along the low latitudes of the Northern hemisphere. The group consisted of the oblong head sunspot with penumbra and the long arc of developed sunspots with penumbraes. In the evolution's peak the total region's area reached 500 m.s.h., and it was counted 40-50 sunspots in the group.
The spreading congestion of fine sunspots and pores crossed the Sun disc since 22.12.01 to 1.01.02 along the high latitudes of the Southern hemisphere.
The long chain of developed sunspts with penumbraes crossed the Sun disc since 23.12.01 to 4.01.02 along the low latitudes of the Southern hemisphere. The total region's area reached 300 m.s.h., and it was counted 25-30 sunspots in the group.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 25.12.01 to 5.01.02 along the low latitudes of the Southern hemisphere. Pores of opposite magnetic polarity were observed to the North from the sunspot. The total region's area reached 200 m.s.h.
The small sunspot with symmetrical penumbra was observed at the 28th parallel of the Southern hemisphere since 26.12.01 to 1.01.02, in the Eastern part of the Sun disc.
The fine bipolar sunspots were observed at the low latitudes of the Northern hemisphere since 26.12 to 30.12.01, to the West from the central meridian.
The short-time bipolar pores were noticed at the mid latitudes of the Northern hemisphere since 26.12 to 29.12.01, to the East from the central meridian.
The growing bipolar group was observed at the mid latitudes of the Northern hemisphere since 27.12.01 to 5.01.02. The head sunspot had symmetrical penumbra. Before set for the limb the total region's area reached 200 m.s.h.
The small bipolar group crossed the Sun disc since 28.12.01 to 9.01.02 along the low latitudes of the Northern hemisphere. The head sunspot had stable symmetrical penumbra. From time to time the total region's area reached 100 m.s.h.
The long bipolar group crossed the Sun disc since 30.12.01 to 12.01.02 along the high latitudes of the Southern hemisphere. The head part of the group consisted of the big sunspot with oblong penumbra and a short pores chain which was situated to the North. The tail part was made from two fine sunspots with penumbraes which were parted a longitude. Later the tail sunspots had decayed. In the evolution's peak the total region's area reached 500 m.s.h., and it was counted 50-55 sunspots.
The big bipolar group crossed the Sun disc since 4.01 to 15.01.02 along the mid latitudes of the Northern hemisphere. The group had three centers of sunspot's formation which extended. The head part of the group consisted of several nuclears with general asymmetrical penumbra. Before set for the limb the head sunspot had considerable diminished and assumed symmetrical form. The immediate sunspots were the most large and dynamic ddeveloping part of the group which consisted of many sunspots with general jagged penumbra. The tail sunspot had perceptible sizes and asymmetrical penumbra. In the evolution's peak the total region's area reached 600 m.s.h., and it was counted 40-45 sunspots in the group.
The new bipolar group had appeared at the low latitudes of the Southern hemisphere on 7.01.02, in the Eastern part of the Sun disc. Since the first days several seats of activity were observed in the group which uneven developed. Before set for the limb the total region's area reached 300 m.s.h., and it was counted 20-25 sunspots in the group. The group was observed until 17.01.
The fine bipolar group was observed at the tenth parallel of the Northern hemisphere since 7.01 to 15.01.02. The head sunspot had symmetrical penumbra.
The decaying bipolar group crossed the Sun disc since 8.01 to 18.01.02 along the mid latitudes of the Southern hemisphere. The head part of the group consisted of many fine sunspots with penumbraes. In the first days the total region's area reached 300 m.s.h., and it was counted 25-30 sunspots in the group.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 8.01 to 20.01.02 along the 29th 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 150 m.s.h.
The small sunspot with symmetrical penumbra crossed the Sun disc since 10.01 to 23.01.02 along the low latitudes of the Southern hemisphere. From time to time the total sunspot's area reached 100 m.s.h.
The big sunspot with asymmetrical penumbra crossed the Sun disc since 11.01 to 23.01.02 along the low latitudes of the Northern hemisphere. The total region's area reached 400 m.s.h. Fine sunspots and pores appeared and disappeared neighbouring the sunspot.
The big double sunspot crossed the Sun disc since 12.01 to 25.01.02 along the tenth parallel of the Southern hemisphere. The total region's area reached 250 m.s.h.
The perceptible bipolar group crossed the Sun disc since 11.01 to 24.01.02 along the tenth parallel of the Northern hemisphere. The bipole consisted of two crowded sunspots with symmetrical penumbraes. The Eastern sunspot was more in two times than the Western sunspot. Fine sunspots and pores appeared and disappeared to the South from the sunspots. The total region's area reached 250 m.s.h.
The small bipolar group was observed at the 26th parallel of the Southern hemisphere since 16.01 to 23.01.02. The head sunspot had asymmetrical penumbra.
The big sunspot with imposing asymmetrical penumbra crossed the Sun disc since 17.01 to 30.01.02 along the low latitudes of the Northern hemisphere. From time to time the total region's area reached 500 m.s.h.
The opened bipolar group crossed the Sun disc since 18.01 to 28.01.02 along the mid latitudes of the Northern hemisphere. The bipole consisted of several head sunspots with general penumbra and many fine sunspots in the tail part of the group. 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 Southern hemisphere since 20.01 to 24.01.02, in the Western part of the Sun disc. The main sunspot had symmetrical penumbra.
The short-time bipolar group was noticed at the tenth parallel of the Northern hemisphere since 22.01 to 25.01.02, to the East from the central meridian.
The insignificant recurrent sunspots were situated at the mid latitudes of the Southern hemisphere since 23.01 to 26.01.02, in the Eastern part of the Sun disc.
The small bipolar group was observed at the 24th parallel of the Southern hemisphere since 22.01 to 1.02.02. The tail sunspot had oblong penumbra and bifurcated from time to time. The total region's area reached 150 m.s.h.
