... sunspots with a large extended penumbra, tail sunspots with a common big penumbra ... the head group's part had again forked and the tail sunspots had gradually decayed ...
... exceeded 200 m.s.h. Besides, tail recurrent pores with against magnetic polarity ... The head and tail parts of the region were slowly extended. ... The head and tail parts of the group had perceptible penumbraes. ...
... The bipole consisted of head and tail sunspots with symmetrical penumbra which had ... reached 500 m.s.h. Later the tail sunspot had decayed, and the head sunspot reached ...
... of fine sunspots with penumbraes, the tail sunspots were assembled in a cluster with ... The fine tail sunspots decayed halfway. NOAA 10406 . ... The head sunspot had penumbra, and the tail sunspots decayed later. NOAA 10416 . ...
... The head and tail parts of the group consisted of small sunspots with penumbraes. ... After intersection of the central meridian the tail sunspots began decay, and one of ...
... sunspot had fine symmetric penumbra, and tail sunspots had undeveloped structure ... next days the group developed to the large bipole with solid head and tail sunspots ...
... head sunspot with penumbra and fine tail sunspots which were parted by considerable ... of a small head sunspot with symmetrical penumbra and decaying tail sunspots ... fine sunspot with symmetrical penumbra and tail sunspots were observed at the low ...
... The head and tail parts of the group consisted of developed sunspots with ... The tail sunspot had symmetrical penumbra. ... of the perceptible head sunspot with asymmetrical penumbra and fine tail sunspots ...
... The head and tail sunspots had symmetrical penumbraes. NOAA 10703 . ... region consisted of head sunspot with small penumbra and imsignificant tail spots ... From time to time there were tail pores in the group. ...
... since 27.08 to 30.08.01 to the North from the tail part of the big region 09601 ... The tail group's part was formed by the sunspot with perceptible sunspot and fine ...