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Дата изменения: Wed Feb 3 21:00:49 2016
Дата индексирования: Sun Apr 10 02:13:16 2016
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The Sunspot Observer - The solar regions - The description of the solar regions

Statistics of sunspot activity

NOAA 09600 - NOAA 09699
The description of the solar regions

NOAA 09600The chain of small sunspots was observed since 27.08 to 30.08.01 to the North from the tail part of the big region 09601.
 
NOAA 09601The big multipolar group crossed the Sun disc since 27.08 to 9.09.01 along the mid latitudes of the Northern hemisphere. The most sunspot had powerful penumbra and nearby fine satellite with penumbra which were settled to the North from the main group's part. The Southern group's part consisted of two nearby sunspots with general penumbra which had "figure-of-eight", and fine sunspots behind it. The tail group's part was formed by the sunspot with perceptible sunspot and fine sunspots neighbouring it. In the first days a chain of fine sunspots was observed to the North from the tail sunspot. Neighbouring the central meridian the total region's area exceeded 700 m.s.h., and it was counted 50-60 sunspots in the group.
 
NOAA 09602The short-time bipolar sunspots were marked since 1.09 to 3.09.01 in the Eastern part of the Sun disc.
 
NOAA 09603The fine sunspot with symmetrical penumbra was observed at the low latitudes of the Southern hemisphere since 1.09 to 7.09.01, in the Eastern part of the Sun disc.
 
NOAA 09604The new bipolar sunspots were noticed at the Western limb since 3.09 to 5.09.01.
 
NOAA 09605The small sunspots adjoyned to the head sunspot of the bipolar region 09606. The sunspots were observed since 2.09 to 12.09.01.
 
NOAA 09606The fast development of a bipolar region was observed at the mid latitudes of the Southern hemisphere since 3.09 to 13.09.01. The bipole consisted of the developed head sunspot with oblong penumbra and many small sunspots and pores which built "kaleidoscopic" combinations behind the main sunspots. In the evolution's peak the total region's area reached 300 m.s.h., and it was counted more 30 sunspots in the group.
 
NOAA 09607The crumbled chain crossed the Sun disc since 4.09 to 15.09.01 along the mid latitudes of the Southern hemisphere. The central sunspot was the most developed and stable part of the group. The total region's area reached 300 m.s.h., and it was counted more 30 sunspots in the group.
 
NOAA 09608The long chain of developed sunspots crossed the Sun disc since 5.09 to 18.09.01 along the 26th parallel of the Southern hemisphere. The maximal total area of the multipole reached 1200 m.s.h., and it was counted more 60 sunspots in the group. The most developed sunspot with complex penumbra was settled in the central part of the group, and rest sunspots had decay's state.
 
NOAA 09609The fine bipolar sunspots were noticed since 6.09 to 8.09.01 near the Western limb.
 
NOAA 09610The big multipolar group crossed the Sun disc since 6.09 to 18.09.01 along the mid latitudes of the Southern hemisphere. The multipole consisted of the head sunspot with powerful oblong penumbra and a chain of many growing sunspots with penumbraes. Neighbouring the central meridian a growing sunspot with asymmetrical penumbra emerged in the forward chain's part which began moved to the North from the head sunspot, and the rest chain's part began decay. In the evolution's peak the total region's area exceeded 600 m.s.h., and it was counted more 50 sunspots in the group.
 
NOAA 09611The growing bipolar group was observed at the tenth parallel of the Northern hemisphere since 7.09 to 12.09.01, in the Western part of the Sun disc. In the first days the bipole consisted of the small double sunspot with oblong penumbra and fine sunspot's chain. In next days the head sunspots began extend and divide, and the chain transformed into tail sunspots with developed penumbraes. Before set for the limb the total region's area reached 400 m.s.h.
 
NOAA 09612The small bipolar group crossed the Sun disc since 6.09 to 16.09.01 along the high latitudes of the Northern hemisphere. From time to time the total bipole's area reached 100 m.s.h.
 
NOAA 09613The fine bipolar sunspots were observed since 7.09 to 9.09.01 near the Western limb.
 
NOAA 09614The recurrent sunspots were marked at the mid latitudes of the Northern hemisphere since 5.09 to 9.09.01.
 
NOAA 09615The short-time pore was observed at the tenth parallel of the Northern hemisphere since 8.09 to 10.09.01, in the Eastern part of the Sun disc.
 
NOAA 09616The big bipolar group was decaying at the mid latitudes of the Southern hemisphere since 11.09 to 24.09.01. In the first days the total region's area exceeded 300 m.s.h., and it was counted 20-25 sunspots in the group. The group consisted of the big head sunspot with asymmetrical penumbra and a long string of small sunspots and pores.
 
NOAA 09617The bipolar group's decay was observed at the tenth parallel of the Northern hemisphere since 12.09 to 19.09.01, in the Eastern part of the Sun disc. In the first days the total region's area reached 150 m.s.h.
 
NOAA 09618The fine bipolar sunspots were noticed since 12.09 to 16.09.01 between the big regions 09608 and 09610.
 
NOAA 09619The fine bipolar group was observed at the mid latitudes of the Northern hemisphere since 13.09 to 21.09.01. The head sunspot had symmetrical penumbra.
 
NOAA 09620The decaying sunspot with asymmetrical penumbra crossed the Sun disc since 16.09 to 28.09.01 along the mid latitudes of the Northern hemisphere. In the first days the total region's area reached 300 m.s.h.
 
NOAA 09621The perceptible sunspot with asymmetrical penumbra adjoyned to the bipolar region 09620 from the East since 16.09 to 28.09.01. The total region's area reached 200 m.s.h.
 
NOAA 09622The growing bipolar group crossed the Sun disc since 16.09 to 26.09.01 along the mid latitudes of the Northern hemisphere. Before set for the limb the total region's area reached 300 m.s.h., moreover the tail sunspot turned out the very developed part of the group.
 
NOAA 09623The fine sunspot was observed since 15.09 to 21.09.01 to the North-West from the bipole 09620.
 
NOAA 09624The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 17.09 to 29.09.01 along the equator. The total region's area reached 100 m.s.h.
 
NOAA 09625The fine bipolar sunspots were marked at the 30th parallel of the Southern hemisphere since 18.09 to 21.09.01, to the West from the central meridian.
 
NOAA 09626The fine bipolar formation was observed at the 25th parallel of the Northern hemisphere since 18.09 to 22.09.01, to the East from the central meridian.
 
NOAA 09627The small sunspot with penumbra crossed the Sun disc since 18.09 to 27.09.01 along the equator. After intersection of the central meridian several pore's fibres appeared at the sunspot's place which formed triangle form. The total region's area did not reach 100 m.s.h. even but in the same time it was counted more fifteen sunspots in the group.
 
NOAA 09628The large multipole crossed the Sun disc since 18.09 to 1.10.01 along the mid latitudes of the Southern hemisphere. The group consisted of many big and small sunspots which were solid adjoyned but occupied considerable parallel's lenght. The total region's area reached 1000 m.s.h., and it was counted more 50 sunspots in the group.
 
NOAA 09629The small bipolar group was noticed since 18.09 to 25.09.01 to the North from the region 09621.
 
NOAA 09630The one-day sunspots were noticed at the high latitudes of the Northern hemisphere on 20.09.01, in the Western part of the Sun disc.
 
NOAA 09631The triangle combination of small sunspots with penumbraes were observed since 19.09 to 25.09.01 to the South-West from the region 09622.
 
NOAA 09632The large sunspot with complex asymmetrical penumbra crossed the Sun disc since 20.09 to 2.10.01 along the high latitudes of the Southern hemisphere. Many fine umbra's pieces were embedded into the penumbra, and fine sunspots and pores appeared and disappeared neighbouring the penumbra. From time to time the total region's area reached 800 m.s.h., and it was counted 20-25 sunspots in the group.
 
NOAA 09633The small sunspot with symmetrical penumbra crossed the Sun disc since 22.09 to 4.10.01 along the 23rd parallel of the Northern hemisphere. From time to time the total region's area reached 100 m.s.h.
 
NOAA 09634The perceptible bipolar group crossed the Sun disc since 22.09 to 4.10.01 along the mid latitudes of the Northern hemisphere. The bipole consisted of fine sunspot's chain, and the tail sunspot had developed penumbra. From time to time the total region's area exceeded 100 m.s.h.
 
NOAA 09635The fine bipolar group was observed at the high latitudes of the Noorthern hemisphere since 23.09 to 1.10.01. The head sunspot had symmetrical penumbra.
 
NOAA 09636The spreading bipolar group crossed the Sun disc since 24.09 to 6.10.01 along the mid latitudes of the Northern hemisphere. The maximal total area exceeded 400 m.s.h., and it was counted 25-30 sunspots in the group. The most developed sunspot had symmetrical penumbra and was situated in the tail part of the group.
 
NOAA 09637The opened bipolar group crossed the Sun disc since 24.09 to 6.10.01 along the mid latitudes of the Southern hemisphere. The fine head sunspot had symmetrical penumbra. The tail sunspot was larger and had symmetrical penumbra also. Fine sunspots and pores were observed neighbouring the tail sunspot. In the first days the total region's area reached 250 m.s.h.
 
NOAA 09638The fine sunspot with symmetrical penumbra was observed at the Sun equator since 25.09 to 27.09.01, in the Eastern part of the Sun disc.
 
NOAA 09639The fine bipolar group crossed the Sun disc since 26.09 to 4.10.01 along the low latitudes of the Northern hemisphere. The head sunspot had symmetrical penumbra.
 
NOAA 09640The insignificant sunspots were observed at the tenth parallel of the Northern hemisphere since 27.09 to 4.10.01.
 
NOAA 09641The perceptible bipolar group crossed the Sun disc since 27.09 to 9.10.01 along the mid latitudes of the Southern hemisphere. The bipole consisted of the big sunspott with asymmetrical penumbra and string of fine sunspots and pores behind it. The total region's area reached 200 m.s.h.
 
NOAA 09642The fine sunspot with symmetrical penumbra crossed the Sun disc since 29.09 to 8.10.01 along the equator.
 
NOAA 09643The recurrent pores were observed at the 27th parallel of the Southern hemisphere since 24.09 to 2.10.01.
 
NOAA 09644The insignificant bipolar group was settled at the high latitudes of the Northern hemisphere since 1.10 to 4.10.01. The tail sunspot had symmetrical penumbra.
 
NOAA 09645The growing bipolar group was observed at the mid latitudes of the Southern hemisphere since 1.10 to 8.10.01, in the Western part of the Sun disc. Before set for the limb the total region area reached 200 m.s.h.
 
NOAA 09646The fine bipolar formation was observed since 1.10 to 4.10.01 to the North-West from the sunspot 09642.
 
NOAA 09647The recurrent pore was observed at the mid latitudes of the Southern hemisphere since 1.10 to 5.10.01, in the Eastern part of the Sun disc.
 
NOAA 09648The small sunspot with symmetrical penumbra was observed at the low latitudes of the Southern hemisphere since 2.10 to 12.10.01. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot. In the first days the total sunspot's area reached 100 m.s.h. The sunspot was slowly diminishing.
 
NOAA 09649The fine sunspots were noticed since 3.10 to 5.10.01 not far from the Eastern limb.
 
NOAA 09650The decaying bipolar sunspots crossed the Sun disc since 3.10 to 13.10.01 along the mid latitudes of the Northern hemisphere. In the first days the total region's area reached 100 m.s.h.
 
NOAA 09651The fine bipolar formation was marked at the high latitudes of the Southern hemisphere since 4.10 to 7.10.01, in the Western part of the Sun disc.
 
NOAA 09652The insignificant bipolar sunspots were observed at the high latitudes of the Northern hemisphere since 4.10 to 7.10.01, neighbouring the central meridian.
 
NOAA 09653The nearby sunspots with developed symmetrical penumbraes crossed the Sun disc since 4.10 to 15.10.01 along the high latitudes of the Southern hemisphere. In the first days the total region's area reached 300 m.s.h.
 
NOAA 09654The short-time pores were marked on 5.10 and 6.10.01 in the central part of the Sun disc.
 
NOAA 09655The small bipolar group was observed at the high latitudes of the Southern hemisphere since 6.10 to 14.10.01. The tail sunspot had perceptible symmetrical penumbra. In the first days the total bipole's area reached 200 m.s.h.
 
NOAA 09656The short-time sunspots were noticed at the high latitudes of the Southern hemisphere on 7.10 and 8.10.01, to the West from the central meridian.
 
NOAA 09657The fine sunspot with symmetrical penumbra was observed at the high latitudes of the Northern hemisphere since 8.10 to 14.10.01, in the Eastern part of the Sun disc. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
 
NOAA 09658The opened bipolar group crossed the Sun disc since 9.10 to 21.10.01 along the mid latitudes of the Southern hemisphere. The bipole consisted of small sunspots with penumbraes which were parted by considerable longitude's distance. The total region's area reached 200 m.s.h.
 
NOAA 09659The insignificant sunspots were observed at the Sun equator since 10.10 to 17.10.01.
 
NOAA 09660The fine sunspots were noticed at the mid latitudes of the Northern hemisphere since 10.10 to 15.10.01.
 
NOAA 09661The big bipolar group crossed the Sun disc since 10.10 to 23.10.01 along the mid latitudes of the Northern hemisphere. The bipole consisted of powerful sunspots with penumbraes, and space between the head and the tail parts of the group was almost free for sunspots. From time to time the total region's area exceeded 800 m.s.h.
 
NOAA 09662The small bipolar group crossed the Sun disc since 10.10 to 21.10.01 along the tenth parallel of the Northern hemisphere.
 
NOAA 09663The fine sunspot with symmetrical penumbra was observed at the mid latitudes of the Southern hemisphere since 11.10 to 17.10.01.
 
NOAA 09664The fine sunspot with rudimentar penumbra was observed on 12.10.01 in the Sun disc's center.
 
NOAA 09665The bipolar one-day pores were noticed on 13.10.01 to the East from the region 09653.
 
NOAA 09666The short-time pores were marked on 14.10 and 15.10.01 near the bipolar sunspots 09663.
 
NOAA 09667The fine sunspot with symmetrical penumbra crossed the Sun disc since 14.10 to 24.10.01 along the high latitudes of the Northern hemisphere. Pores of opposite magnetic polarity appeared and disappeared neighbouring the sunspot.
 
NOAA 09668The bipolar one-day pores were noticed on 15.10.01 to the North-West from the big region 09661.
 
NOAA 09669The curved sunspot's chain crossed the Sun disc since 15.10 to 26.10.01 along the mid latitudes of the Northern hemisphere. The total region's area reached 200 m.s.h., and it was counted 20-25 sunspots in the group.
 
NOAA 09670The perceptible sunspot with oblong penumbra crossed the Sun disc since 16.10 to 28.10.01 along the mid latitudes of the Southern hemisphere. The sunspot was gradually bifurcated. The maximal total area of the region reached 500 m.s.h.
 
NOAA 09671The short bipolar chain adjoyned to the region 09669 from the West. The group was observed since 16.10 to 24.10.01.
 
NOAA 09672The crowded congestion of developed sunspots crossed the Sun disc since 17.10 to 30.10.01 along the high latitudes of the Southern hemisphere. The total region's area reached 550 m.s.h.
 
NOAA 09673The perceptible sunspot with asymmetrical penumbra crossed the Sun disc since 18.10 to 30.10.01 along the equator. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot. The total region's area reached 150 m.s.h.
 
NOAA 09674The fine bipolar sunspots were observed at the low latitudes of the Southern hemisphere since 19.10 to 24.10.01.
 
NOAA 09675The fine sunspots were noticed at the mid latitudes of the Northern hemisphere since 20.10 to 26.10.01, in the Eastern part of the Sun disc.
 
NOAA 09676The fine sunspot with symmetrical penumbra crossed the Sun disc since 20.10 to 31.10.01 along the low latitudes of the Northern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
 
NOAA 09677The fine bipolar sunspots were observed at the high latitudes of the Northern hemisphere since 22.10 to 29.10.01.
 
NOAA 09678The big multipolar group crossed the Sun disc since 23.10 to 2.11.01 along the low latitudes of the Northern hemisphere. The head part of the group consisted of double sunspot with powerful penumbra. The tail sunspot's congestion with general penumbra was continuously changing the form. The total region's area reached 700 m.s.h., and it was counted 40-50 sunspots in the group.
 
NOAA 09679The fine bipolar sunspots were observed at the tenth parallel of the Southern hemisphere since 23.10 to 2.11.01.
 
NOAA 09680The recurrent pores were marked at the high latitudes of the Northern hemisphere since 23.10 to 29.10.01.
 
NOAA 09681The small group was observed at the 24th parallel of the Southern hemisphere since 25.10 to 31.10.01, in the Western part of the Sun disc. The main sunspot had stable symmetrical penumbra.
 
NOAA 09682The large multipolar group crossed the Sun disc since 25.10 to 6.11.01 along the mid latitudes of the Northern hemisphere. The multipole consisted of many developed sunspots with jagged penumbra. The group was continuously changing the contours. In the evolution's peak the total region's area reached 1200 m.s.h., and it was counted 60-65 sunspots in the group.
 
NOAA 09683The insignificant bipolar sunspots were observed at the 28th parallel of the Northern hemisphere since 26.10 to 31.10.01.
 
NOAA 09684The large sunspot with penumbra crossed the Sun disc since 27.10 to 8.11.01 along the low latitudes of the Northern hemisphere. Small sunspots and pores of opposite magnetic polarity appeared and disappeared neighbouring the sunspot. From time to time the total region's area reached 600 m.s.h., and it was counted 25-30 sunspots in the group.
 
NOAA 09685The bipolar chain of small sunspots crossed the Sun disc since 1.11 to 11.11.01 along the low latitudes of the Northern hemisphere. From time to time the total region's area exceeded 100 m.s.h., and it was counted 15-20 sunspots in the group.
 
NOAA 09686The fine sunspots were noticed to the North from the bipole 09685 since 31.10 to 3.11.01.
 
NOAA 09687The long chain of small sunspots and pores crossed the Sun disc since 1.11 to 13.11.01 along the high latitudes of the Southern hemisphere. The group was gradually decaying into three sunspot's clusters, and than it was slowly melting away the Sun disc's background. From time to time the total region's area exceeded 400 m.s.h., and it was counted 40-45 sunspots in the group.
 
NOAA 09688The bipolar combination of several fine sunspots were parted by considerable longitude's distance. The group was observed at the 26th parallel of the Northern hemisphere since 3.11 to 13.11.01.
 
NOAA 09689The fast development of the bipolar region was observed at the 27th parallel of the Southern hemisphere since 4.11 to 11.11.01. In the evolution's peak the total region's area reached 150 m.s.h., and it was counted 15-20 sunspots in the group.
 
NOAA 09690The long multipolar group crossed the Sun disc since 4.11 to 18.11.01 along the mid latitudes of the Southern hemisphere. The head part of the group consisted of several developed sunspots with penumbraes which were gradually lining. The tail part of the group formed of several developed sunspots with general penumbra which were slowly stretching. Many fine sunspots and pores were settled between the big sunspots. Neighbouring the central meridian the multipole assumed closed magnetic configuration, the total region's area reached 1400 m.s.h., and it was counted more 60 sunspots in the group.
 
NOAA 09691The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 6.11 to 19.11.01 along the low latitudes of the Northern hemisphere. In the first days the total region's area reached 100 m.s.h.
 
NOAA 09692The quick-growing bipolar group was observed at the low latitudes of the Northern hemisphere since 7.11 to 13.11.02, in the Western part of the Sun disc. The head and the tail parts of the group extended in several times. Before set for the limb the total region's area reached 500 m.s.h.
 
NOAA 09693The fine sunspots were noticed since 7.11 to 11.11.01 to the North-East from the big region 09692.
 
NOAA 09694The fine sunspot with symmetrical penumbra crossed the Sun disc since 7.11 to 20.11.01 along the mid latitudes of the Northern hemisphere. In the first days the total region's area reached 100 m.s.h.
 
NOAA 09695The small sunspot with symmetrical penumbra crossed the Sun disc since 10.11 to 22.11.01 along the mid latitudes of the Northern hemisphere. From time to time the total region's area reached 100 m.s.h.
 
NOAA 09696The fine bipolar formation was observed at the low latitudes of the Southern hemisphere since 10.11 to 16.11.01, in the Eastern part of the Sun disc.
 
NOAA 09697The large sunspot with asymmetrical penumbra crossed the Sun disc since 11.11 to 24.11.01 along the mid latitudes of the Northern hemisphere. Many fine sunspots and pores of opposite magnetic polarity were observed to the North from the sunspot. In the evolution's peak the total region's area reached 400 m.s.h., and it was counted 20-25 sunspots in the group.
 
NOAA 09698The small bipolar group crossed the Sun disc since 12.11 to 24.11.01 along the 24th parallel of the Southern hemisphere. The bipole was oriented to the meridian. The Southern sunspot had symmetrical penumbra. In time the Northern sunspot had decayed. The total region's area reached 100-150 m.s.h.
 
NOAA 09699The fine bipolar sunspots were noticed on 12.11 and 13.11.01 near the Western limb.
 












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