The perceptible bipolar group crossed the Sun disc since 14.06 to 26.06.02 along the high latitudes of the Northern hemisphere. The bipole consisted of the developed head sunspot with simmetrical penumbra and tail pores. The total region's area reached 150-200 m.s.h.
The fine bipolar group was observed at the mid latitudes of the Southern hemisphere since 14.06 to 21.06.02. From time to time it was counted 10-15 sunspots in the bipole.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 16.06 to 29.06.02 along the mid latitudes of the Northern hemisphere. Fine sunspots and pores with opposite magnetic polarity appeared and disappeared neighbouring the sunspot. The total region's area exceeded 150 m.s.h.
The big sunspot with imposing symmetrical penumbra crossed the Sun disc since 18.06 to 1.07.02 along the tenth parallel of the Southern hemisphere. Fine sunspots and pores appeared and disappeared neighbouring the sunspot. From time to time the total region's area exceeded 500 m.s.h.
The small bipolar group crossed the Sun disc since 21.06 to 3.07.02 along the tenth parallel of the Southern hemisphere. From time to time the total region's area reached 100 m.s.h.
The small sunspot with symmetrical penumbra crossed the Sun disc since 25.06 to 7.07.02 along the mid latitudes of the Southern hemisphere. From time to time pores with opposite magnetic polarity were observed neighbouring the sunspot.
The new bipolar group had appeared at the high latitudes of the Southern hemisphere on 27.06.02, to the East from the central meridian. The bipole was assuming triangle form and gradually extending. On 5.07 the new region had reached the Western limb, and before it the total area exceeded 600 m.s.h.
The triangle combination of several developed sunspots with penumbraes was observed at the mid latitudes of the Southern hemisphere since 29.06 to 11.07.02. The greater sunspot in the group was slowly bifurcating into two nuclears with penumbraes. From time to time the total region's area exceeded 500 m.s.h.
The fast development of a bipolar group had plase at the 34th parallel of the Southern hemisphere since 3.07 to 10.07.02. From time to time the total region's area reached 200 m.s.h.
The large multipolar group crossed the Sun disc since 9.07 to 23.07.02 along the high latitudes of the Northern hemisphere. The maximal total area of the region exceeded 1300 m.s.h., and it was counted 90 sunspots in the group. The multipole consisted of three big parts. In the first days the head sunspots were more developed part of the group. But then these sunspots began decay, and in the same time the central and tail parts of the group turned to the process of slow collapse.
The short-time bipolar formation was noticed at the high latitudes of the Southern hemisphere since 13.07 to 15.07.02, neighbouring the central meridian.
The large multipolar group crossed the Sun disc since 15.07 to 27.07.02 along the low latitudes of the Southern hemisphere. In the evolution's peak the total region's area exceeded 1000 m.s.h., and it was more 60 sunspots in the group. The multipole consisted of many developed sunspots with were united by several large pieces of penumbra. After intersection the central meridian the tail part of the group began slowly decay.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 16.07 to 28.07.02 along the mid latitudes of the Northern hemisphere. The total sunspot's area reached 150-200 m.s.h.
The large multipolar group crossed the Sun disc since 21.07 to 3.08.02 along the mid latitudes of the Southern hemisphere. From time to time the total region's area reached 1000 m.s.h. In the first days the head sunspots were more developed part of the group. After intersection of the central meridian the head sunspots began slowly decay, and the group was lining.
The perceptible bipolar chain was observed at the mid latitudes of the Northern hemisphere since 23.07 to 1.08.02. The total region's area reached 150-200 m.s.h. In the first days the tail sunspots were more developed part of the group. But slow decay of the tail part was simultaneously happened with gradual development of the head sunspots. In result the decay's process touched the whole group.
The big bipolar group crossed the Sun disc since 23.07 to 3.08.02 along the high latitudes of the Southern hemisphere. The group appeared in immediate nearness from the big region 10039. Its were parallelly situated. The new bipole was lining, and newly originating sunspots extended. From time to time the total region's area exceeded 500 m.s.h., and it was counted more 50 sunspots in the group.
The new multipolar group had appeared at the low latitudes of the Southern hemisphere on 26.07.02, in the Eastern part of the Sun disc. In three days the total region's area increased in tens times and exceeded 500 m.s.h. Several seats of sunspot formation were observed in the group, therefore it extended and developed "from the inside". In the evolution's peak the total multipole's area had reached 700 m.s.h., and the sunspot's quantity had 50-60 units. On 4.08 the new group had come to the Western limb.
The insignificant bipolar formation was marked at the low latitudes of the Northern hemisphere on 28.07 and 29.07.02, neighbouring the central meridian.
The developing bipolar chain of sunspots was observed at the low latitudes of the Southern hemisphere since 1.08 to 8.08.02, in the Western part of the Sun disc. The newly arising sunspots developed and extended. Not long before set for the limb the new group assumed closed magnetic configuration, and the total area reached 400 m.s.h. It was counted more 30 sunspots in the region.
The small bipolar group crossed the Sun disc since 2.08 to 10.08.02 along the mid latitudes of the Northern hemisphere. The head sunspot had fine asymmetrical penumbra.
The short-time bipolar sunspots were marked at the 28th parallel of the Southern hemisphere since 3.08 to 5.08.02, in the Western part of the Sun disc.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 3.08 to 16.08.02 along the low latitudes of the Northern hemisphere. The rapid development of sunspots and pores with opposite magnetic polarity was observed behind the sunspot. In the evolution's peak the total region's area exceeded 300 m.s.h.
The opened bipolar group crossed the Sun disc since 6.08 to 19.08.02 along the mid latitudes of the Northern hemisphere. The bipole consisted of head and tail sunspots with penumbraes of moderate sizes. The head sunspot had oblong form, and after intersection of the central meridian it bifurcated and gradually decayed. The tail sunspot had stable symmetrical form. Neighbouring the central meridian a chain of pores was observed to the South from the tail sunspot. From time to time the total region's area reached 200 m.s.h.
The shapeless bipolar formation crossed the Sun disc since 9.08 to 21.08.02 along the mid latitudes of the Northern hemisphere. Neighbouring the central meridian the total region's area reached 100-150 m.s.h.
The unstable bipolar chain of sunspots crossed the Sun disc since 10.08 to 23.08.02 along the tenth parallel of the Northern hemisphere. Neighbouring the central meridian the total region's area reached 300 m.s.h., and it was counted 40 sunspots in the group.
The bipolar combination of small sunspots was parted by considerable longitude's distance. The group was observed since 10.08 to 19.08 to the West from the large region 10069.
The large multipole crossed the Sun disc since 11.08 to 24.08.02 along the low latitudes of the Southern hemisphere. The greater part of sunspots was embedded into giant irregular penumbra. Neighbouring the central meridian the total region's area reached 2000 m.s.h., and it was counted more 60 sunspots in the group.
The growing bipolar group was observed at the mid latitudes of the Southern hemisphere since 11.08 to 16.08.02, in the Western part of the Sun disc. Before set for the limb the total region's area had reached 300 m.s.h.
The developing bipolar group crossed the Sun disc since 14.08 to 25.08.02 along the high latitudes of the Southern hemisphere. The main seats of sunspot's formation were scattered on the whole group. Neighbouring the central meridian the group had assumed closed configuration, and the total region's area had exceeded 300 m.s.h. It was counted more 30 sunspots in the group. Then the tail part of the group began impetuously decay, and the head sunspots reached the Western limb.
The small bipolar group crossed the Sun disc since 13.08 to 26.08.02 along the mid latitudes of the Northern hemisphere. The tail sunspot had aswymmetrical penumbra and was gradually decaying. In the first days the total region's area exceeded 100 m.s.h.
The spreading bipolar group crossed the Sun disc since 17.08 to 28.08.03 along the high latitudes of the Southern hemisphere. The region had not regular configuration of sunspots, from time to time the total area exceeded 150 m.s.h.
The small sunspot with symmetrical penumbra was observed to the South-West from the big region 10085 since 17.08 to 29.08.02. There were fine sunspots and pores of opposite magnetic polarity neighbouring the sunspot.
The big sunspot with imposing penumbra crossed the Sun disc since 18.08 to 31.08 along the tenth parallel of the Southern hemisphere. Fine sunspots and pores appeared and disappeared neighbouring the sunspot. The total region's area exceeded 500 m.s.h.
The big sunspot crossed the Sun disc since 22.08 to 3.09.02 along the low latitudes of the Southern hemisphere. In the first days the total region's area reached 400 m.s.h. Neighbouring the central meridian the sunspot began crumbled. In result the sunspot had diminished in several times.
The new bipolar group had appeared at the high latitudes of the Southern hemisphere on 23.08.02, to the West from the central meridian. The bipole was dynamic developing, in three days the total area exceeded 200 m.s.h. On 27.08 the new region had come to the Western limb.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 29.08 to 9.09.02 along the high latitudes of the Southern hemisphere. In the first days sunspots of opposite magnetic polarity were observed behind the sunspot. The total region's area exceeded 100 m.s.h.
The long bipolar group crossed the Sun disc since 29.08 to 10.09.02 along the low latitudes of the Northern hemisphere. The bipole consisted of developed sunspots with penumbraes and pores stretching on the twenty degrees at a longitude and more. Maximal total area of the region exceeded 800 m.s.h., and it was counted more 50 sunspots in the group.
The developing bipolar group crossed the Sun disc since 30.08 to 10.09.02 along the mid latitudes of the Southern hemisphere. The bipole consisted of the head sunspot with stable symmetrical penumbra and the string of developing sunspots. In the evolution's peak the total region's area exceeded 200 m.s.h., and it was counted more twenty sunspots and pores in the group.
The perceptible bipolar chain of small sunspots with penumbraes was marked to the West from the big region 10095 since 1.09 to 8.09.02. From time to time the total region's area exceeded 100 m.s.h., and it was counted more twenty sunspots and pores in the group.
