The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 1.09 to 12.09.02 along the high latitudes of the Southern hemisphere. In the first days the total region's area reached 200 m.s.h. Neighbouring the central meridian the sunspot had bifurcated and began decay.
The fine sunspot with symmetrical penumbra was observed at the low latitudes of the Northern hemisphere since 1.09 to 5.09.02, in the Eastern part of the Sun disc.
The spreading bipolar group crossed the Sun disc since 3.09 to 15.09.02 along the mid latitudes of the Northern hemisphere. In the evolution's peak the total area of the region exceeded 500 m.s.h., and it was counted 40-45 sunspots in the group.
The giant sunspot with asymmetrical penumbra was crossed the Sun disc since 7.09 to 20.09.02 along the low latitudes of the Southern hemisphere. Many fine spots and pores were observed neighbouring the sunspot. The region was classified as a closed multipole. On 10.09 the total group's area had exceeded 1500 m.s.h. It was counted more 50 sunspots in the group.
The perceptible bipolar group crossed the Sun disc since 8.09 to 20.09.02 along the tenth parallel of the Northern hemisphere. The head and tail parts of the group consisted of small sunspots with penumbraes. Several pores connected two parts of the group. Neighbouring the central meridian the total region's area reached 200 m.s.h., and it was counted 20-25 sunspots and pores in the group. After intersection of the central meridian the tail sunspots began decay, and one of the head sunspots assumed symmetrical form and reached the Western limb.
The fine bipolar sunspots were observed at the high latidudes of the Northern hemisphere since 10.09 to 18.09.02. The bipole had almost meridianal direct.
The tail part of the large region 10105 was classified as a separate bipole since 14.09 to 21.09.02. The new group consisted of perceptible sunspot with symmetrical penumbra, and many fine sunspots were settled behind it and were embedded into several pieces of penumbra. In the first days the total region's area exceeded 300 m.s.h., and it was counted more 30 sunspots in the group.
The perceptible bipolar group crossed the Sun disc since 13.09 to 23.09.02 along the equator. The head and tail sunspots had developed penumbraes. Neighbouring the central meridian the group lined into an unstable chain of developed sunspots which began soon crumble. The maximal total area of the region reached 250 m.s.h., and it was counted more 20 sunspots in the group. In several days the tail part of the group decayed, and the head sunspot assumed symmetrical form and reached the Western limb on 23.09.
The new bipolar group had appeared at the mid latitudes of the Southern hemisphere on 15.09.02, in the Eastern part of the Sun disc. The impetuous evolution's process started in the head sunspot with symmetrical penumbra, and new sunspots with powerful penumbraes appeared behind it. In several days the total region's area increased in tens times and exceeded 600 m.s.h. It was counted 30-40 sunspots in the group. On 25.09 the new multipole had come to the Western limb.
The perceptible bipolar group was observed at the mid latitudes of the Southern hemisphere since 20.09 to 27.09.02. The head and tail parts of the group consisted of several nearby sunspots with penumbraes. The sunspots regular changed form and combination. The total region's area reached 200 m.s.h.
The new bipolar group had appeared at the low latitudes of the Northern hemisphere on 21.09.02, in the Eastern part of the Sun disc. The bipole was slowly extending. Neighbouring the central meridian the total area reached 250 m.s.h. The head sunspot had big asymmetrical penumbra, and fine tail sunspots were enclosed into general oblong penumbra. Then the tail sunspots began decay, and the head sunspot assumed symmetrical form and had come to the Western limb on 2.10.
The new compact bipole had appeared at the high latitudes of the Northern hemisphere on 22.09.02, neighbouring the central meridian. The group consisted of several perceptible sunspots which were enclosed into general irregular penumbra. In the evolution's peak the total region's area reached 400 m.s.h. On 29.09 the new group reached the Western limb.
The spreading bipolar group crossed the Sun disc since 24.09 to 6.09.02 along the mid latitudes of the Northern hemisphere. The bipole consisted of developed sunspots and pores. Neighbouring the central meridian the total region's area exceeded 300 m.s.h., and it was counted more 30 sunspots in the group.
The developed bipolar group crossed the Sun disc since 28.09 to 10.10.02 along the high latitudes of the Southern hemisphere. In the first days the new bipole was quickly extended. Neighbouring the central meridian the total region's area exceeded 300 m.s.h., and it was counted 25-30 sunspots in the group. Then the tail part of the group began decay, and the head sunspot assumed symmetrical form and reached the Western limb.
The big multipole crossed the Sun disc since 2.10 to 15.10.02 along the tenth parallel of the Northern hemisphere. Two sunspots with general penumbra were as a base of the group. The oblong sunspot had large sizes, and the asymmetrical sunspot had perceptible sizes. Two sunspots were like exclamation point. Many small sunspots and pores were observed neighbouring the sunspots. The maximal total area of the region exceeded 600 m.s.h., and it was counted more 40 sunspots in the group.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 4.10 to 17.10.02 along the low latitudes of the Southern hemisphere. The rest of the bipolar region 10114. From time to time the total sunspot's area reached 200 m.s.h.
The new bipolar group had appeared at the mid latitudes of the Northern hemisphere on 7.10.02, in the Eastern part of the Sun disc. The head sunspot's penumbra had formed in the first day, and the tail sunspot's penumbra appeared in next day. Then the tail part of the group began crush and gradually decay. The maximal total area of the region exceeded 100 m.s.h., then it was counted more twenty sunspots in the group. On 17.10 the group had come to the Western limb.
The small sunspot with symmetrical penumbra crossed the Sun disc since 8.10 to 20.10.02 along the mid latitudes of the Northern hemisphere. From time to time pores with opposite magnetic polarity appeared neighbouring the sunspot.
The big multipole crossed the Sun disc since 8.10 to 21.10.02 along the mid latitudes of the Northern hemisphere. The sunspot with big asymmetrical penumbra was as a base of the group. In the first days a chain of small sunspots appeared to the South from the sunspot which began extend and develop. More developing sunspot stood out in the head part of the chain which was situated to the South-West from the base sunspot of the group. In time the tail part of the chain decayed, and all the group assumed bipolar configuration of two developed and nearby sunspots. The total region's area exceeded 300 m.s.h. From time to time it was counted more 40 sunspots in the group.
The recurrent group crossed the Sun disc since 12.10 to 24.10.02 along the low latitudes of the Southern hemisphere. In the first days the group was as a perceptible sunspot with symmetrical penumbra. Then many fine sunspots with opposite magnetic polarity appeared to the North from the sunspot, and its had fast development. From time to time the total region's area reached 150 m.s.h., and it was counted 20-25 sunspots in the group.
The sunspot with asymmetrical penumbra was spliting up into three fine and lined spots. The region crossed the Sun disc since 13.10 to 22.10.02 along the mid latitudes of the Southern hemisphere.
The perceptible bipolar group crossed the Sun disc since 13.10 to 24.10.02 along the high latitudes of the Southern hemisphere. The bipole was quickly developing and decaying. The maximal total area of the region exceeded 200 m.s.h., and it was counted 25-30 sunspots in the group.
The large bipolar group crossed the Sun disc since 17.10 to 31.10.02 along the 25th parallel of the Northern hemisphere. The bipole consisted of the imposing head sunspot with symmetrical penumbra and the big tail part which had complex structure. Neighbouring the central meridian the main tail sunspots built fanciful form like a three-leaf flower. In the evolution peak the total region's area exceeded 1000 m.s.h., and it was counted 50-60 sunspots in the group.
The insignificant recurrent sunspots were observed at the tenth parallel of the Northern hemisphere since 19.10 to 25.10.02, in the Eastern part of the Sun disc.
The perceptible double sunspot with oblong penumbra crossed the Sun disc since 19.10 to 1.11.02, along the high latitudes of the Northern hemisphere. The maximal total area of the region exceeded 250 m.s.h. The sunspot was slowly diminished and assumed more symmetrical form.
The small bipolar group crossed the Sun disc since 24.10 to 1.11.02 along the high latitudes of the Southern hemisphere. The bipole consisted of two fine, nearby sunspots with penumbraes. In the first days the total region's area reached 100 m.s.h.
The fine sunspot with symmetrical penumbra was observed at the mid latitudes of the Southern hemisphere since 26.10 to 30.10.02, in the Eastern part of the Sun disc.
The small bipolar chain was observed at the 25th parallel of the Southern hemisphere since 28.10 to 3.11.02, in the Eastern part of the Sun disc. There was a sunspot with fine asymmetrical penumbra in the chain's middle.
The opened bipolar group crossed the Sun disc since 28.10 to 8.11.02, along the mid latitudes of the Southern hemisphere. The head sunspot had perceptible symmetrical penumbra, the fine tail sunspot slowly decayed. Many fine spots and pores were observed around the sunspots. In the evolution's peak the total region's area exceeded 150 m.s.h., and it was counted more twenty sunspots in the group.
The sunspot with symmetrical penumbra crossed the Sun disc since 29.10 to 11.11.02, along the tenth parallel of the Northern hemisphere. The rest of the big bipolar region 10139. The total sunspot's area exceeded 100 m.s.h.
The perceptible bipolar group crossed the Sun disc since 30.10 to 11.11.02, along the mid latitudes of the Northern hemisphere. The bipole consisted of the big head sunspot with asymmetrical penumbra and many fine sunspots and pores behind it. On 5.11 the head sunspot began bifurcated, and then the newly formated sunspots slowly moved away along the meridianal direct. The total region's area reached 400 m.s.h., and it was counted 25-30 sunspots in the group.
The new bipolar group was observed since 31.10 to 5.11.02 in the Western part of the Sun disc. The bipole consisted of perceptible sunspot with penumbra and string of fine spots and pores which lined behind it. From time to time the total region's area reached 100 m.s.h.
The big multipole crossed the Sun disc since 1.11 to 13.11.02 along the tenth parallel of the Southern hemisphere. The group consisted of many sunspots with different sizes which were scattered at a latitude on considerable distance. In the evolution's peak the total area of the region exceeded 500 m.s.h., and it was counted more 50 sunspots in the group.
The small group was observed to the South-East from the region 10180 since 2.11 to 14.11.02. The head sunspot had stable symmetrical penumbra. The fine tail sunspot quickly decayed.
The perceptible nuclears were united by general asymmetrical penumbra. The region crossed the Sun disc since 3.11 to 15.11.02, along the mid latitudes of the Southern hemisphere. In the first days the total group's area reached 300 m.s.h.
The briskly developing bipolar group was marked at the tenth parallel of the Northern hemisphere since 5.11 to 11.11.02. The maximal total area of the region reached 150 m.s.h., and it was counted twenty sunspots in the group.
The big multipolar group crossed the Sun disc since 8.11 to 21.11.02. along the high latitudes of the Southern hemisphere. The multipole consisted of many sunspots and pores which were enclosed by several big pieces of penumbra. The total region's area reached 600-700 m.s.h., and it was counted 60-70 sunspots in the group. Before set for the limb the group began decay.
The new bipolar group had appeared on 11.11.02 neighbouring the central meridian. In the first days the sunspots were almost not noticeable. On 14.11 a small net had appeared in the place which was woven by fine sunspots and pores. In next day the structure turned into perceptible bipolar group which consisted of developed sunspots with penumbraes. The total region's area reached 500 m.s.h. On 19.11 the new group set for the limb.
The perceptible bipolar group crossed the Sun disc since 13.11 to 26.11.02, along the mid latitudes of the Southern hemisphere. The head sunspot had stable penumbra with moderate sizes, the tail part consisted of two sunspots with penumbraes which were parted by a longitude and gradually decayed. The total region's area reached 300-350 m.s.h.
The symmetrical penumbra with impressive penumbra crossed the Sun disc since 14.11 to 27.11.02, along the 25th parallel of the Northern hemisphere. The rest of the large region 10162. The total sunspot's area reached 300-400 m.s.h.
The big bipolar group crossed the Sun disc since 15.11 to 29.11.02, along the mid latitudes of the Southern hemisphere. The head part of the group consisted of double sunspot with general penumbra and had imposing sizes. A long string of fine sunspots and pores lined behind the sunspot which was slowly decaying. From time to time the total region's area exceeded 600 m.s.h.
