The long bipolar configuration of several perceptible sunspots with penumbraes crossed the Sun disc since 26.11 to 9.12.02, along the high latitudes of the Southern hemisphere. In the first days the head and tail parts of the group consisted of several sunspots but later there was a sunspot each in the parts which assumed symmetrical form. The maximal total region's area exceeded 300 m.s.h.
The shapeless bipolar formation crossed the Sun disc since 29.11 to 8.12.02, along the tenth parallel of the Northern hemisphere. The total region's area exceeded 100 m.s.h.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 29.11 to 11.12.02, along the high latitudes of the Southern hemisphere. The hardly visible tail sunspots were in the first days. The maximal total region's area exceeded 150 m.s.h.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 2.12 to 11.12.02, along the mid latitudes of the Northern hemisphere. Small sunspots and pores appeared and disappeared neighbouring the sunspot. In the first days the total region's area reached 200 m.s.h. After intersection of the central meridian the group began decay.
The small bipolar group crossed the Sun disc since 3.12 to 13.12.02, along the mid latitudes of the Northern hemisphere. The head sunspot had fine symmetrical penumbra.
The new bipolar group was observed at the mid latitudes of the Southern hemisphere since 5.12 to 10.12.02, in the Western part of the Sun disc. The head sunspot had perceptible symmetrical penumbra, and the tail sunspot had fine penumbra. Many pores were scattered between the sunspots.
The rest of the big bipolar region 10191 crossed the Sun disc since 5.12 to 14.12.02 along the high latitudes of the Southern hemisphere. On 8.12 the sunspot with symmetrical penumbra had bifurcated and began slowly decay.
The small bipolar formation was noticed at the high latitudes of the Southern hemisphere since 7.12 to 10.12.02, in the Western part of the Sun disc. The main sunspots had rudiments of penumbra.
The fine high latitude sunspot with symmetrical penumbra was observed to the South-East from the region 10220 since 7.12 to 19.12.02. Single pores appeared and disappeared behind the sunspot.
The perceptible bipolar group crossed the Sun disc since 7.12 to 19.12.02, along the mid latitudes of the Southern hemisphere. In the first days the tail part of the group was developed and consisted of several perceptible sunspots with penumbraes and pores. In next days the head sunspot with asymmetrical penumbra was extending, and the tail sunspots began decay. In the evolution's peak the total region's area had exceeded 300 m.s.h., and it was counted 20-25 sunspots in the group.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 12.12 to 24.12.02, along the high latitudes of the Northern hemisphere. Fine sunspots and pores appeared and disappeared around it.
The perceptible bipolar group was observed at the Western district of the big region 10229 since 12.12 to 23.12.02. In the evolution's peak the total bipole's area had reached 100 m.s.h., and it was counted 15-20 sunspots in the group.
The big bipolar group crossed the Sun disc since 13.12 to 24.12.02, along the high latitudes of the Southern hemisphere. In result of the development the region turned into very long and solid chain of sunspots with penumbraes which was like a giant sword. The maximal total area of the chain reached the 700 m.s.h., and it was counted 50 sunspots in the group.
The big multipolar group crossed the Sun disc since 14.12 to 26.12.02, along the mid and high latitudes of the Northern hemisphere. The head part of the group was settled at the mid latitudes and consisted of two nearby sunspots with perceptible asymmetrical penumbraes. The tail part of the group was situated at the high latitudes and was made by two duplex nuclears with general oblong penumbra. Many small sunspots with asymmetrical penumbraes and pores were scattered in the intermediate part of the group. The maximal total area of the region exceeded 400 m.s.h., and it was counted 40-45 sunspots in the group. All parts of the group were gradually diminished and decayed.
The perceptible bipolar group crossed the Sun disc since 17.12 to 28.12.02, along the low latitudes of the Southern hemisphere. The bipole consisted of the head sunspot with stable symmetrical penumbra and woven string of many small sunspots with penumbraes. Neighbouring the central meridian the total region's area reached 300 m.s.h. Later the tail part of the group had decayed, and the head sunspot reached the Western limb.
The small bipolar group crossed the Sun disc since 19.12 to 27.12.02, along the 25th parallel of the Southern hemisphere. The main sunspots had fine penumbraes.
The small sunspot with symmetrical penumbra crossed the Sun disc since 24.12 to 30.12.02, along the high latitudes of the Northern hemisphere. The rest of the region 10205.
The perceptible bipolar group crossed the Sun disc since 2.01 to 13.01.03, along the low latitudes of the Southern hemisphere. In the evolution's peak the total region's area exceeded 300 m.s.h.
The small bipolar group crossed the Sun disc since 2.01 to 12.01.03, along the high latitudes of the Southern hemisphere. The bipole consisted of the head sunspot with asymmetrical penumbra and the string of the few fine spots behind it. In the first days the total region's area exceeded 100 m.s.h.
The new bipolar group crossed the Sun disc since 6.01 to 18.01.03, along the mid latitudes of the Southern hemisphere. The group was quick developing but it had not stable form. In the evolution's peak the total region's area had exceeded 300 m.s.h., and it was counted 40-50 sunspots in the group.
The perceptible sunspot with oblong penumbra crossed the Sun disc since 7.01 to 20.01, along the high latitudes of the Southern hemisphere. The total region's area exceeded 100 m.s.h.
The perceptible bipolar group crossed the Sun disc since 7.01 to 18.01.03, along the mid latitudes of the Southern hemisphere. In the first days the total region's area reached 400 m.s.h. The head sunspot had big assymetrical penumbra. Three small tail sunspots with symmetrical penumbraes were lined. These sunsspots were slowly decayed.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 10.01 to 22.01.03, along the mid latitudes of the Southern hemisphere. The total region's area exceeded 100 m.s.h.
The Western district of the region 10251 crossed the Sun disc since 8.01 to 20.01.03, along the mid latitudes of the Southern hemisphere. In the first days the total region's area exceeded 400 m.s.h. The sunspot had big asymmetrical penumbra which had bifurcated later. The greater part assumed symmetrical form, and the lesser sunspot was slowly decaying.
The bipolar chain of fine sunspots crossed the Sun disc since 14.01 to 22.01.03, along the tenth parallel of the Northern hemisphere. The chain was slowly crumbling.
The new bipolar group had appeared at the mid latitudes of the Southern hemisphere on 19.01.03, neighbouring the central meridian. In two days the sunspots began extend. On 25.01 the new region had come to the Western limb.
The long sunspot's chain crossed the Sun disc since 19.01 to 31.01.03, along the high latitudes of the Southern hemisphere. Neighbouring the central meridian the head sunspot was divided into parts which began extend. In several days the sunspots retutned in the decay's process. From time to time the total region's area reached 200 m.s.h., and it was counted 25-30 sunspots in the group.
The small sunspot had symmetrical penumbra, and a long string of the few fine sunspots streched behind it. In the first days the total region's area exceeded 150 m.s.h.
The solid congestion of small sunspots was slowly streching and decaying. The group was observed at the mid latitudes of the Northern hemisphere since 21.01 to 29.01.03. From time to time the total region's area exceeded 100 m.s.h.
The perceptible bipolar group crossed the Sun disc since 21.01 to 2.02.03, along the low latitudes of the Southern hemisphere. The bipole consisted of two nearby sunspots with penumbraes. The head sunspot had stable symmetrical penumbra. The tail sunspot was slowly decaying. In the first days the total region's area reached 150-200 m.s.h.
The insignificant bipolar formation was situated at the low latitudes of the Southern hemisphere since 25.01 to 30.01.03, in the Western part of the Sun disc.
The bipolar configuration of fine sunspots and pores crossed the Sun disc since 26.01 to 3.02.03, along the low latitudes of the Southern hemisphere. On 30.01 it was counted 20 sunspots in the group.
The new bipolar group was observed at the low latitudes of the Northern hemisphere since 27.01 to 1.02.03, in the Western part of the Sun disc. The total region's area exceeded 100 m.s.h.
The small eruptive group crossed the Sun disc since 28.01 to 9.02.03, along the low latitudes of the Southern hemisphere. In the first days the group was as single sunspot with symmetrical penumbra. On 1.02 the sunspot had acquired a satellite with the opposite magnetic polarity. The bipole consisted of two small sunspots with symmetrical penumbraes. From time to time the total region's area exceeded 100 m.s.h.
The long chain of small sunspots crossed the Sun disc since 1.02 to 14.02.03, along the mid latitudes of the Southern hemisphere. In the first days the total region's area reached 300 m.s.h. The sunspots were slowly dissolving against the Sun disc.
The amorph bipolar formation crossed the Sun disc since 4.02 to 13.02.03, along the mid latitudes of the Northern hemisphere. The continuation of the region 10257. In the first days the total group's area exceeded 100 m.s.h.
The fine sunspot with symmetrical penumbra crossed the Sun disc since 6.02 to 15.02.03, along the mid latitudes of the Southern hemisphere. The rest of the bipolar region 10263.
The small group was noticed to the South-West from the region 10278 since 5.02 to 16.02.03. In the first days the group was as a single pore, later a small bipolar configuration appeared in the place.
The small sunspot with symmetrical penumbra crossed the Sun disc since 8.02 to 16.02.03, along the tenth parallel of the Southern hemisphere. The rest of the bipolar region 10263. The sunspot was slowly diminished.
The fine sunspot with symmetrical penumbra crossed the Sun disc since 15.02 to 27.02.03, along the mid latitudes of the Northern hemisphere. More fine sunspots and pores appeared and disappeared behind the sunspot.
The new quick-growing group was observed at the tenth parallel of the Northern hemisphere since 18.02 to 21.02.03, near the Western limb. The total region's area exceeded 200 m.s.h.
The new bipolar group had appeared at the mid latitudes of the Southern hemisphere on 18.02.03, in the Eastern part of the Sun disc. The group was rapidly extending and developing. Neighbouring the central meridian the total area reached 400 m.s.h. It was counted 25-30 sunspots and pores in the bipole. The head and tail sunspots had developed penumbraes and were connected by a chain of fine sunspots and pores. Then the tail sunspots began slowly decay, and the head part of the group had come to the Western limb on 1.03.
The short-time bipolar sunspots were observed at the high latitudes of the Southern hemisphere since 26.02 to 1.03.03, in the Eastern part of the Sun disc.
The small sunspot with symmetrical penumbra crossed the Sun disc since 26.02 to 8.03.03, along the mid latitudes of the Southern hemisphere. On 5.03 the sunspot had bifurcated and began decay.
The sunspot with large penumbra crossed the Sun disc since 28.02 to 12.03.03, along the mid latitudes of the Northern hemisphere. Several small spots were observed behind the sunspot. The total region's area reached 600-700 m.s.h.
