The small bipolar group crossed the Sun disc since 11.10 to 17.10 along the high latitudes of the Northern hemisphere. The head sunspot had a fine penumbra.
The small bipolar group crossed the Sun disc since 11.11 to 17.11 along the 33rd parallel of the Northern hemishere. The main spots had symmetrical penumbraes.
The small bipolar group was crossing the Sun disc since 4.07 to 11.07 along the high latitudes of the Southern hemisphere. The head sunspot had fine symmetric penumbra, and tail sunspots had undeveloped structure. There were pores appeared and disappeared between the main sunspots. In the peak of activity it was counted 10-15 sunspots in the group, and the total region area reached 200 m.h.s.
The fine bipolar group of sunspots with undeveloped penumbraes and an open configuration was crossing the Sun disc along the high latitudes of the Northern hemisphere since 23.09 to 1.10.
The erruptive bipolar structure was arisen on 24.10 to the South from the region 11028. In the peak of activity in the group it was counted twenty sunspots almost, and the total region area exseeded 150 m.h.s.
The high latitude erruptive structure had arisen 15.12 to the North from the region 11034. In the peak of activity the group reached closed configuration, it was counted twenty sunspots almost, and the total region area exceeded 200 m.h.s.
The small bipolar sunspots were observing at the high latitudes of the Southern hemisphere since 20.12 to 25.12 in ther Western part of the Sun disc. Time to time main sunspots had fine symmetrical penumbraes.
The small bipolar group was crossing the Sun disc along the high latitudes of the Southern hemisphere since 27.12.09 to 6.01.10. The group had an open structure, and main sunspots had fine penumbraes.
The one of the power events for new cycle. On 8.01 there were bipolar pores had arisen at the high latitudes of the Northern hemisphere, not far from the Eastern limb. In next days the group developed to the large bipole with solid head and tail sunspots. Neighboring the central meridian it was counted 25 sunspots in the group, and the total region area exceeded 300 m.h.s. On 18.01 the group had come to the Western limb turning slow dacay.
The simple bipolar group had arisen on 20.01 in the opposite area of the Sun disc than the region 11040. The bipole consisted of an head sunspot with stable penumbra and small tail sunspots. After crossing the central meridian the head sunspot assumed symmetrical form turning to slow decay.
The small sunspot was observed at the 25th parallel of the Northern hemisphere since 01.02 to 07.02. Time to time there were tail pores of the opposite magnetic polarity.
The long sunspot chain was gradually disintegrated at the high latitudes of the Northern hemisphere since 07.02 to 14.02, to the West from the central meridian. In the evolution peak it was more 30 sunspots in the group, and the total region area was exceeded 400 m.h.s.
The high-growth bipolar sunspots was crossing the sunspot disc since 8.02 to 18.02 along high latitudes of the Northern hemisphere. The group consisted of a small head sunspot and small tail sunspot cluster. Neighboring the central meridian it was counted more twenty small sunspots and total region area reached 200 m.h.s.
The small bipolar sunspots were observed at the middle latitudes of the Southern hemisphere since 17.02 to 23.02 to the West from the central meridian.
The small sunspot with symmetrical penumbra crossed the Sun disc since 24.02 to 5.03 across middle latitudes. Time to time tail sunspots were observed.
The noticeable bipolar group crossed the Sun disc since 10.03 to 20.03 along the middle latitudes of the Northern hemisphere. The head group's part consisted of several small sunspots interspersed in assymmetrical penumbra which was gradually breaking up. Tail sunspots had small sunpots, its were quickly disintegrated. Neighboring the central meridian the total region area exceeded 200 m.h.s., it counts more 20 sunspots in group.
The short-time bipolar sunspots were noticed at the high latitudes of the Southern hemisphere since 12.03 to 13.03 to the West from the central meridian.
The noticeable bipolar group crossed the Sun disc since 23.03 to 3.04 along the middle latitudes of the Northern hemisphere. The bipole consisted of a head sunspot with small symmetrical penumbra and a tail sunspot with big symmetrical penumbra. The head sunspot was gradually shattered and disappeared. The tail sunspot had lost symmetry and than it was scattered on smaller sunspots. Neighboring the central meridian the total region area reached 400 m.h.s., it was counted ten sunspots in the group.
The small sunspot with penumbra crossed the Sun disc since 27.03 to 6.04 along the high latitudes of the Southern hemisphere. Time to time there were pores neighboring the sunspot./TR>
The open bipolar group was observed at the middle latitudes of the Northern hemisphere since 06.04 to 10.04, to the West from the central meridian. The head sunspot had symmetrical penumbra.
The short-time bipolar pores were noticed at the middle latitudes of the Southern hemisphere since 13.04 to 15.04 to the West from the central meridian.
The small bipolar group had appeared on 21.05 at the middle latitudes of the Southern hemisphere to the East from the central meridian. The head sunspot had a small symmetrical penumbra and the tail sunspots were gradually disappeared. On 28.05 the leading sunspot had reached the Western limb.
The small bipolar group had appeared on 1.06 at the 20th parallel of the Southern hemisphere neighboring the central meridian. The main sunspots had small penumbraes. On 6.06 the bipole had reached the Western limb.
The small bipolar group crossed the Sun disc since 10.07 to 21.07 along the 20th parallel of the Northern hemisphere. The head sunspot had a stable penumbra.
The noticeable bipolar group crossed the Sun disc since 20.07 to 1.08 along the 24th parallel of the Southern hemisphere. The main sunspots had small penumbraes and combined a triangle configuration. In process of advance on the Sun disc the tail sunspot had collapsed. In the peak's evolution the total region area reached 300 m.h.s., and it counted more twenty sunspots in the group.
The noticeable sunspot with symmetrical penumbra crossed the Sun disc since 28.07 to 9.08 along the middle latitudes of the Northern hemisphere. Time to time there were pores of the opposit magnetic polarity.
