The long bipolar chain of small sunspots were observed at the 29th parallel of the Southern hemisphere since 6.04 to 14.04.02. The total region's area reached 150 m.s.h., and it was counted 15-20 sunspots in the group.
The long chain of developed sunspots adjoined to the bipolar region 09893 from the East. The group was observed at the high latitudes of the Northern hemisphere since 7.04 to 16.04.02. The total region's area reached 300-400 m.s.h.
The bipolar combination of sunspots crossed the Sun disc since 7.04 to 19.04.02 along the mid latitudes of the Northern hemisphere. The head sunspot had perceptible symmetrical penumbra, and the tail sunspots were moved away on the considerable longitude's distance. From time to time the total bipole's area exceeded 100 m.s.h.
The big multipolar group crossed the Sun disc since 9.04 to 21.04.02 along the mid latitudes of the Southern hemisphere. The group was slowly increasing the area and stretched by a latitude. Before set for the limb the total region's area had reached 800 m.s.h. The multipole was liked as a heavy chain of powerful, developed sunspots.
The spreading bipolar group was decaying at the Sun disc since 11.04 to 21.04.02. In the first days the total region's area reached 300-400 m.s.h. It was counted more 30 sunspots in the group.
The short-time bipolar sunspots were marked at the low latitudes of the Northern hemisphere since 12.04 to 15.04.02, in the Western part of the Sun disc.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 14.04 to 25.04.02 along the low latitudes of the Northern hemisphere. The total region's area exceeded 100 m.s.h. From time to time satellites with opposite magnetic polarity appeared neighbouring the sunspot.
The bipolar combination of developed sunspots with penumbraes crossed the Sun disc since 15.04 to 25.04.02 along the high latitudes of the Southern hemisphere. The total region's area reached 200 m.s.h. After intersection of the central meridian the tail part of the group began decay.
The short-time bipolar group was marked at the mid latitudes of the Southeern hemisphere since 18.04 to 20.04.02, to the East from the central meridian.
The developing bipolar group was observed at the tenth parallel of the Northern hemisphere since 18.04 to 27.04.02. The group originated to the East from the central meridian, and in three days the total area had increased in ten times and reached 300 m.s.h. It was counted more twenty sunspots in the bipole. The group was liked a curved serpent.
The opened bipolar group crossed the Sun disc since 19.04 to 1.05.02 along the low latitudes of the Northern hemisphere. The bipole consisted of the head and tail sunspots with developed penumbraes. Fine sunspots and pores appeared and disappeared between its. The total region's area reached 250 m.s.h.
The crowded congestion of bipolar sunspots crossed the Sun disc since 20.04 to 1.05.02 along the mid latitudes of the Norrthern hemisphere. Several sunspots were embedded into asymmetrical penumbra, and fine sunspots were behind it. The total region's area reached 200 m.s.h.
The small bipolar group was observed at the mid latitudes of the Southern hemisphere since 21.04 to 29.04.02. In the first days the total region's area reached 150 m.s.h.
The small bipolar group crossed the Sun disc since 22.04 to 4.05.02 along the mid latitudes of the Northern hemisphere. The bipole consisted of perceptible sunspot with symmetrical penumbra and fine tail sunspots. The group was settled to meridianal direct. In the first days the total region's area reached 200 m.s.h.
The short-time bipolar sunspots were marked at the low latitudes of the Southern hemisphere since 24.04 to 27.04.02, in the Western part of the Sun disc.
The short-time bipolar sunspots were marked at the mid latitudes of the Southern hemisphere since 24.04 to 27.04.02, in the Western part of the Sun disc.
The small bipolar group crossed the Sun disc since 24.04 to 5.05.02 along the mid latitudes of the Northern hemisphere. The bipole consisted of two nearby sunspots with penumbraes.
The fine bipolar group was situated at the 28th parallel of the Southern hemisphere since 29.04 to 5.05.02, in the Eastern part of the Sun disc. The head sunspot had symmetrical penumbra.
The small bipolar formation of irregular form was observed at the mid latitudes of the Northern hemisphere since 29.04 to 8.05.02. The total region's area reached 100 m.s.h.
The new bipolar group had originated at the high latitudes of the Northern hemisphere on 30.04.02, to the East from the central meridian. The head sunspot of the group was gradually extending and complicating the form. Before set for the limb the total region's area reached 200 m.s.h. The bipole was observed until 7.05.
The small sunspot with symmetrical penumbra crossed the Sun disc since 30.04 to 13.05.02 along the mid latitudes of the Northern hemisphere. From time to time the total sunspot's area reached 100 m.s.h.
The big bipolar group crossed the Sun disc since 1.05 to 15.05.02 along the mid latitudes of the Southern hemisphere. The bipole consisted of the large sunspot with symmetrical penumbra and developing congestion of many sunspots which was settled to the South.
The perceptible bipolar group crossed the Sun disc since 3.05 to 15.05.02 along the low latitudes of the Southern hemisphere. The bipole consisted of two nearby sunspots with penumbraes which were slowly dispersed. Pores appeared and disappeared neighbouring the sunspots. The total region's area reached 200-250 m.s.h.
The fine sunspot with symmetrical penumbra was observed at the high latitudes of the Northern hemisphere since 4.05 to 10.05.02, in the Eastern part of the Sun disc.
The big bipolar group crossed the Sun disc since 6.05 to 19.05.02 along the equator. The bipole consisted of the large sunspot with penumbra and fine sunspots behind it. From time to time the total region's area reached 400 m.s.h.
The big sunspot with imposing symmetrical penumbra crossed the Sun disc since 10.05 to 22.05.02 along the high latitudes of the Southern hemisphere. The total region's area reached 400 m.s.h.
The small bipolar formation crossed the Sun disc since 11.05 to 20.05.02 along the low latitudes of the Southern hemisphere. The head sunspot had symmetrical penumbra. From time to time the total region's area reached 100 m.s.h.
The small double sunspot crossed the Sun disc since 14.05 to 25.05.02 along the high latitudes of the Southern hemisphere. In the first days the total region's area exceeded 100 m.s.h.
The big multipolar group crossed the Sun disc since 15.05 to 28.05.02 along the tenth parallel of the Northern hemisphere. The multipole had very unusual, arrow-like form. The arrow's top was made from developed sunspots with penumbraes, and the arrow's base consisted of many fine sunspots which were embedded into several pieces of penumbra. From time to time the total region's area reached 1000 m.s.h., and it was counted more 50 sunspots in the group. After intersection of the central meridian the group began decay.
The small bipolar group crossed the Sun disc since 17.05 to 29.05.02 along the mid latitudes of the Northern hemisphere. The double head sunspot was gradually diminishing and assuming symmetrical form. In the first days the total region's area exceeded 150 m.s.h.
The long bipolar group crossed the Sun disc since 19.05 to 31.05.02 along the high latitudes of the Southern hemisphere. In the first days the total region's area exceeded 300 m.s.h. The group consisted of several developed sunspots, but it was the head sunspot with symmetrical penumbra only which reached the Western limb.
The big bipolar group crossed the Sun disc since 20.05 to 1.06.02 along the mid latitudes of the Northern hemisphere. The group consisted of the large sunspot with asymmetrical penumbra and many fine spots and pores behind it. The total region's area reached 400 m.s.h., and maximal sunspot's quantity exceeded 30 units.
The fine sunspot with symmetrical penumbra crossed the Sun disc since 21.05 to 1.06.02 along the low latitudes of the Southern hemisphere. From time to time pores with opposite magnetic polarity were observed neighbouring the sunspot.
The opened bipolar group crossed the Sun disc since 25.05 to 5.06.02 along the low latitudes of the Northern hemisphere. The head and tail sunspots had developed symmetrical penumbraes. The total region's area reached 150-200 m.s.h.
The big bipolar group crossed the Sun disc since 28.05 to 10.06.02 along the mid latitudes of the Southern hemisphere. The group consisted of developed sunspots with powerful penumbraes. In the first days the total region's area exceeded 800 m.s.h. After intersection the central meridian the head part of the group began decay, and the most developed tail sunspot assumed symmetrical form and reached the Western limb.
The short-time bipolar pores were observed at the tenth parallel of the Southern hemisphere since 30.05 to 1.06.02, to the West from the central meridian.
The developed bipolar group crossed the Sun disc since 31.05 to 11.06.02 along the high latitudes of the Southern hemisphere. The total region's area reached 250 m.s.h. After intersection of the central meridian the decay's process formed which began since the tail sunspots.
The fine sunspot with symmetrical penumbra was observed at the 24th parallel of the Northern hemisphere since 2.06 to 8.06.02, in the Eastern part of the Sun disc.
The long bipolar group was observed since 4.06 to 13.06.02 at the high latitudes of the Northern hemisphere. The bipole consisted of developed head and tail sunspots with penumbraes. From time to time many fine sunspots and pores were visible between its. The total region's area reached 200 m.s.h.
The solid chain of small sunspots had appeared at the mid latitudes of the Southern hemisphere on 6.06.02, to the East from the central meridian. After intersection of the central meridian one of the head sunspots began extend, and the chain turned into slow decay. Before set for the limb the total region's area reached 400 m.s.h. The group was observed until 14.06.
The big sunspot with oblong penumbra crossed the Sun disc since 7.06 to 19.06.02 along the high 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 300 m.s.h.
The small sunspot with symmetrical penumbra was observed at the low latitudes of the Northern hemisphere since 9.06 to 13.06.02, in the Western part of the Sun disc. In the first days pores with opposite magnetic polarity were observed neighbouring the sunspot.
