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Дата индексирования: Sun Apr 10 02:16:44 2016
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The Sunspot Observer - The solar regions - The description of the solar regions

Statistics of sunspot activity

NOAA 09700 - NOAA 09799
The description of the solar regions

NOAA 09700The short-time sunspots were marked at the 24th parallel of the Southern hemisphere since 13.11 to 15.11.01, to the West from the central meridian.
 
NOAA 09701The bipolar one-day sunspots were fixed at the 33rd parallel of the Southern hemisphere on 13.11.01, to the East from the central meridian.
 
NOAA 09702The short-time pores were marked at the high latitudes of the Northern hemisphere on 14.11 and 15.11.01, to the West from the central meridian.
 
NOAA 09703The short-time sunspots were noticed at the high latitudes of the Northern hemisphere since 14.11 to 16.11.01, neighbouring the central meridian.
 
NOAA 09704The large double sunspot with general irregular penumbra crossed the Sun disc since 14.11 to 26.11.01 along the high latitudes of the Southern hemisphere. Many fine sunspots and pores were observed neighbouring the sunspot. From time to time the total region's area reached 700 m.s.h., and it was counted 30-40 sunspots in the group.
 
NOAA 09705The recurrent sunspots were observed at the mid latitudes of the Northern hemisphere since 14.11 to 20.11.01.
 
NOAA 09706The short-time sunspots were marked at the Eastern limb on 14.11 and 15.11.01.
 
NOAA 09708The fine bipolar sunspots were observed at the Sun equator since 16.11 to 20.11.01.
 
NOAA 09709The high latitude bipolar sunspots were noticed in the Northern hemisphere since 16.11 to 18.11.01, to the East from the central meridian.
 
NOAA 09710The small bipolar formation crossed the Sun disc since 18.11 to 27.11.01 along the tenth parallel of the Southern hemisphere.
 
NOAA 09711The short-time sunspot was marked on 20.11 and 21.11.01 to the West from the central meridian.
 
NOAA 09712The shapeless cloud of fine sunspots crossed the Sun disc since 21.11 to 1.12.01 along the mid latitudes of the Northern hemisphere. From time to time the total region's area reached 100 m.s.h.
 
NOAA 09713The short-time bipolar sunspots were noticed since 22.11 to 24.11.01 in the central part of the Sun disc.
 
NOAA 09714The small bipolar formation was observed at the tenth parallel of the Southern hemisphere since 22.11 to 2.12.01. Before set for the limb the tail sunspot with penumbra began extend, and the total region's area exceeded 100 m.s.h.
 
NOAA 09715The big bipolar group crossed the Sun disc since 23.11 to 6.12.01 along the low latitudes of the Northern hemisphere. In the evolution's peak the multipole had assumed closed configuration, the total area had exceeded 1000 m.s.h., and it was counted more 30 sunspots in the group.
 
NOAA 09716The fine bipolar group crossed the Sun disc since 25.11 to 7.12.01 along the low latitudes of the Southern hemisphere. The head sunspot had symmetrical penumbra.
 
NOAA 09717The perceptible sunspot with symmetricaal penumbra crossed the Sun disc since 27.11 to 9.12.01 along the low latitudes of the Northern hemisphere. Fine sunspots and pores of opposite magnetic polarity were observed to the East from the sunspot. The total region's area reached 250-300 m.s.h.
 
NOAA 09718The big bipolar group crossed the Sun disc since 27.11 to 10.12.01 along the low latitudes of the Southern hemisphere. The multipole consisted of several large sunspots with asymmetrical penumbraes. The total region's area reached 700 m.s.h., and it was counted 25-30 sunspots in the group.
 
NOAA 09719The fine bipolar group was settled at the low latitudes of the Northern hemisphere since 27.11 to 2.12.01.
 
NOAA 09720The small bipolar group crossed the Sun disc since 28.11 to 10.12.01. The bipole was outstanding because it was appreciably drifting to the South Pole, from the 17th to 28th parallel during the Sun disc's passing.
 
NOAA 09721The asymmetrical sunspot with oblong penumbra crossed the Sun disc since 28.11 to 11.12.01 along the mid latitudes of the Northern hemisphere. Before set for the limb the sunspot had bifurcated. From time to time the total region's area exceeded 200 m.s.h.
 
NOAA 09722The short-time bipolar sunspots were noticed on 1.12 and 2.12.01 to the West from the central meridian.
 
NOAA 09723The fine bipolar sunspots were observed since 1.12 to 10.12.01 to the East from the big region 09718.
 
NOAA 09724The small sunspot with symmetrical penumbra crossed the Sun disc since 1.12 to 13.12.01 along the tenth parallel of the Northern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
 
NOAA 09725The fine bipolar sunspots were marked at the tenth parallel of the Southern hemisphere since 2.12 to 5.12.01, not far from the Western limb.
 
NOAA 09726The small bipolar group was observed since 2.12 to 10.12.01 to the North-West from the region 09727. The main sunspot had symmetrical penumbra.
 
NOAA 09727The compact combination of big sunspots crossed the Sun disc since 3.12 to 15.12.01 along the high latitudes of the Southern hemisphere. The total regin's area reached 600 m.s.h., and it was counted more 30 sunspots in the group.
 
NOAA 09728The small bipolar sunspots were observed at the 36 th parallel of the Northern hemisphere since 4.12 to 10.12.01, in the Western part of the Sun disc.
 
NOAA 09729The short-time bipolar sunspots were marked at the high latitudes of the Northern hemisphere since 5.12 to 7.12.01, neighbouring the central meridian.
 
NOAA 09730The short-time sunspots were noticed at the mid latitudes of the Southern hemisphere since 4.12 to 6.12.01, in the Eastern part of the Sun disc.
 
NOAA 09731The short-time bipolar sunspots were observed at the 25th parallel of the Northern hemisphere since 6.12 to 9.12.01, in the Eastern part of the Sun disc.
 
NOAA 09732The small sunspot with symmetrical penumbra crossed the Sun disc since 7.12 to 18.12.01 along the equator. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
 
NOAA 09733The big bipolar group crossed the Sun disc since 7.12 to 20.12.01 along the mid latitudes of the Northern hemisphere. The group was regular changing the form, at times assuming fanciful contours. In the first days the tail part of the group was like a horseshoe. In the evolution's peak the total region's area reached 500 m.s.h., and it was counted more 50 sunspots in the group.
 
NOAA 09734The fine sunspot with symmetrical penumbra was observed at the mid latitudes of the Southern hemisphere since 9.12 to 18.12.01. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
 
NOAA 09735The bipolar one-day pores were noticed at the tenth parallel of the Northern hemisphere on 10.12.01, to the West from the central meridian.
 
NOAA 09736The fine bipolar sunspots were marked at the tenth parallel of the Southern hemisphere since 10.12 to 14.12.01, in the Western part of the Sun disc.
 
NOAA 09737The fine bipolar group crossed the Sun disc since 10.12 to 22.12.01 along the 27th parallel of the Southern hemisphere.
 
NOAA 09738The small bipolar group crossed the Sun disc since 12.12 to 22.12.01 along the high latitudes of the Southern hemisphere.
 
NOAA 09739The opened bipolar group was observed at the mid latitudes of the Southern hemisphere since 13.12 to 20.12.01, in the Western part of the Sun disc. The head and tail parts of the group consisted of extending sunspots with penumbraes. Before set for the limb the total region's area exceeded 400 m.s.h.
 
NOAA 09740The fine sunspot was noticed on 13.12 and 14.12.01 near the Eastern limb.
 
NOAA 09741The fine bipolar formation was observed at the low latitudes of the Northern hemisphere since 13.12 to 22.12.01.
 
NOAA 09742The large multipolar group crossed the Sun disc since 15.12 to 28.12.01 along the low and the mid latitudes of the Northern hemisphere. Three big sunspots with penumbraes were as a base of the multipole and were settled by triangle. Many small sunspots and pores were observed between the sunspots. In the evolution's peak the total region's area exceeded 1000 m.s.h., and it was counted 60-70 sunspots in the group.
 
NOAA 09743The perceptible sunspot with penumbra crossed the Sun disc since 16.12 to 28.12.01 along the tenth parallel of the Southern hemisphere. 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 09744The short-time bipolar sunspots were noticed since 16.12 to 18.12.01 to the East from the central meridian.
 
NOAA 09745The fine bipolar formation was observed since 18.12 to 27.12.01 to the North-East from the region 09743.
 
NOAA 09746The short-time bipolar sunspots were noticed since 19.12 to 22.12.01 in the central part of the Sun disc.
 
NOAA 09747The fine bipolar group was marked at the mid latitudes of the Northern hemisphere since 19.12 to 26.12.01.
 
NOAA 09748The growing bipolar group was observed to the East from the bipolar region 09743 since 20.12 to 30.12.01. The new region's increase had a place in the same time when the group 09743 was decreasing. Before set for the limb the total bipole's region reached 300 m.s.h.
 
NOAA 09749The fine bipolar formation was observed at the low latitudes of the Southern hemisphere since 19.12 to 23.12.01, in the Eastern part of the Sun disc.
 
NOAA 09750The fine bipolar sunspots were noticed since 21.12 to 23.12.01 near the Western limb.
 
NOAA 09751The big bipolar group crossed the Sun disc since 20.12.01 to 2.01.02 along the low latitudes of the Northern hemisphere. The group consisted of the oblong head sunspot with penumbra and the long arc of developed sunspots with penumbraes. In the evolution's peak the total region's area reached 500 m.s.h., and it was counted 40-50 sunspots in the group.
 
NOAA 09752The short-time pores were noticed to the West from the region 09743 since 22.12 to 25.12.01.
 
NOAA 09753The spreading congestion of fine sunspots and pores crossed the Sun disc since 22.12.01 to 1.01.02 along the high latitudes of the Southern hemisphere.
 
NOAA 09754The long chain of developed sunspts with penumbraes crossed the Sun disc since 23.12.01 to 4.01.02 along the low latitudes of the Southern hemisphere. The total region's area reached 300 m.s.h., and it was counted 25-30 sunspots in the group.
 
NOAA 09755The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 25.12.01 to 5.01.02 along the low latitudes of the Southern hemisphere. Pores of opposite magnetic polarity were observed to the North from the sunspot. The total region's area reached 200 m.s.h.
 
NOAA 09756The small sunspot with symmetrical penumbra was observed at the 28th parallel of the Southern hemisphere since 26.12.01 to 1.01.02, in the Eastern part of the Sun disc.
 
NOAA 09757The fine bipolar sunspots were observed at the low latitudes of the Northern hemisphere since 26.12 to 30.12.01, to the West from the central meridian.
 
NOAA 09759The short-time bipolar pores were noticed at the mid latitudes of the Northern hemisphere since 26.12 to 29.12.01, to the East from the central meridian.
 
NOAA 09760The fine bipolar sunspots were marked at the low latitudes of the Northern hemisphere since 26.12 to 29.12.01, to the East from the central meridian.
 
NOAA 09761The fine sunspot with symmetrical penumbra crossed the Sun disc since 26.12.01 to 7.01.02 along the tenth parallel of the Northern hemisphere.
 
NOAA 09762The short-time pore was noticed at the Sun disc's center on 27.12 and 28.12.01.
 
NOAA 09763The fine sunspot with symmetrical penumbra crossed the Sun disc since 27.12.01 to 7.01.02 along the low latitudes of the Northern hemisphere.
 
NOAA 09764The growing bipolar group was observed at the mid latitudes of the Northern hemisphere since 27.12.01 to 5.01.02. The head sunspot had symmetrical penumbra. Before set for the limb the total region's area reached 200 m.s.h.
 
NOAA 09765The small bipolar group crossed the Sun disc since 28.12.01 to 9.01.02 along the low latitudes of the Northern hemisphere. The head sunspot had stable symmetrical penumbra. From time to time the total region's area reached 100 m.s.h.
 
NOAA 09766The fine sunspots were noticed to the East from the region 09765 since 29.12.01 to 3.01.02.
 
NOAA 09767The long bipolar group crossed the Sun disc since 30.12.01 to 12.01.02 along the high latitudes of the Southern hemisphere. The head part of the group consisted of the big sunspot with oblong penumbra and a short pores chain which was situated to the North. The tail part was made from two fine sunspots with penumbraes which were parted a longitude. Later the tail sunspots had decayed. In the evolution's peak the total region's area reached 500 m.s.h., and it was counted 50-55 sunspots.
 
NOAA 09768The fine bipolar sunspots were noticed to the East from the region 09755 since 1.01 to 7.01.02. The head sunspot had symmetrical penumbra.
 
NOAA 09769The fine bipolar formation was marked at the high latitudes of the Southern hemisphere since 1.01 to 6.01.02, in the Western part of the Sun disc.
 
NOAA 09770The fine bipolar formation was marked at the low latitudes of the Northern hemisphere since 2.01 to 5.01.02, in the Western part of the Sun disc.
 
NOAA 09771The fine bipolar formation was observed at the high latitudes of the Southern hemisphere since 1.01 to 6.01.02.
 
NOAA 09772The small sunspot with oblong penumbra crossed the Sun disc since 3.01 to 15.01.02 along the mid latitudes of the Southern hemisphere.
 
NOAA 09773The big bipolar group crossed the Sun disc since 4.01 to 15.01.02 along the mid latitudes of the Northern hemisphere. The group had three centers of sunspot's formation which extended. The head part of the group consisted of several nuclears with general asymmetrical penumbra. Before set for the limb the head sunspot had considerable diminished and assumed symmetrical form. The immediate sunspots were the most large and dynamic ddeveloping part of the group which consisted of many sunspots with general jagged penumbra. The tail sunspot had perceptible sizes and asymmetrical penumbra. In the evolution's peak the total region's area reached 600 m.s.h., and it was counted 40-45 sunspots in the group.
 
NOAA 09774The bipolar one-day pores were noticed on 7.01.02 in the Western part of the Sun disc.
 
NOAA 09775The new bipolar group had appeared at the low latitudes of the Southern hemisphere on 7.01.02, in the Eastern part of the Sun disc. Since the first days several seats of activity were observed in the group which uneven developed. Before set for the limb the total region's area reached 300 m.s.h., and it was counted 20-25 sunspots in the group. The group was observed until 17.01.
 
NOAA 09776The fine bipolar group was observed at the tenth parallel of the Northern hemisphere since 7.01 to 15.01.02. The head sunspot had symmetrical penumbra.
 
NOAA 09777The pores were noticed on 8.01.02 in the Eastern limb.
 
NOAA 09778The decaying bipolar group crossed the Sun disc since 8.01 to 18.01.02 along the mid latitudes of the Southern hemisphere. The head part of the group consisted of many fine sunspots with penumbraes. In the first days the total region's area reached 300 m.s.h., and it was counted 25-30 sunspots in the group.
 
NOAA 09779The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 8.01 to 20.01.02 along the 29th parallel of the Northern hemisphere. 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 09780The fine bipolar sunspots were observed at the tenth parallel of the Southern hemisphere since 9.01 to 12.01.02, not far from the Western limb.
 
NOAA 09781The small sunspot with symmetrical penumbra crossed the Sun disc since 10.01 to 23.01.02 along the low latitudes of the Southern hemisphere. From time to time the total sunspot's area reached 100 m.s.h.
 
NOAA 09782The big sunspot with asymmetrical penumbra crossed the Sun disc since 11.01 to 23.01.02 along the low latitudes of the Northern hemisphere. The total region's area reached 400 m.s.h. Fine sunspots and pores appeared and disappeared neighbouring the sunspot.
 
NOAA 09783The big double sunspot crossed the Sun disc since 12.01 to 25.01.02 along the tenth parallel of the Southern hemisphere. The total region's area reached 250 m.s.h.
 
NOAA 09784The fine recurrent sunspots were noticed at the 30th parallel of the Southern hemisphere on 13.01, 14.01 and since 23.01 to 25.01.02.
 
NOAA 09785The perceptible bipolar group crossed the Sun disc since 11.01 to 24.01.02 along the tenth parallel of the Northern hemisphere. The bipole consisted of two crowded sunspots with symmetrical penumbraes. The Eastern sunspot was more in two times than the Western sunspot. Fine sunspots and pores appeared and disappeared to the South from the sunspots. The total region's area reached 250 m.s.h.
 
NOAA 09786The small bipolar group was observed at the 26th parallel of the Southern hemisphere since 16.01 to 23.01.02. The head sunspot had asymmetrical penumbra.
 
NOAA 09787The big sunspot with imposing asymmetrical penumbra crossed the Sun disc since 17.01 to 30.01.02 along the low latitudes of the Northern hemisphere. From time to time the total region's area reached 500 m.s.h.
 
NOAA 09788The opened bipolar group crossed the Sun disc since 18.01 to 28.01.02 along the mid latitudes of the Northern hemisphere. The bipole consisted of several head sunspots with general penumbra and many fine sunspots in the tail part of the group. The total region's area reached 250 m.s.h., and it was counted 20-25 sunspots in the group.
 
NOAA 09789The insignificant bipolar sunspots were situated at the mid latitudes of the Northern hemisphere since 15.01 to 23.01.02.
 
NOAA 09790The insignificant bipolar formation was observed at the 28th parallel of the Northern hemisphere since 19.01 to 26.01.02.
 
NOAA 09791The small bipolar group was observed at the low latitudes of the Southern hemisphere since 20.01 to 24.01.02, in the Western part of the Sun disc. The main sunspot had symmetrical penumbra.
 
NOAA 09792The short-time pores were noticed at the Sun equator since 23.01 to 25.01.02, to the West from the central meridian.
 
NOAA 09793The fine bipolar group was marked at the mid latitudes of the Southern hemisphere since 20.01 to 27.01.02. The main sunspot had symmetrical penumbra.
 
NOAA 09794The fine bipolar group was marked at the mid latitudes of the Northern hemisphere since 20.01 to 29.01.02. The main sunspot had symmetrical penumbra.
 
NOAA 09795The new bipolar group was observed at the high latitudes of the Northern hemisphere since 23.01 to 25.01.02, not far from the Western limb.
 
NOAA 09796The short-time bipolar group was noticed at the tenth parallel of the Northern hemisphere since 22.01 to 25.01.02, to the East from the central meridian.
 
NOAA 09797The insignificant recurrent sunspots were situated at the mid latitudes of the Southern hemisphere since 23.01 to 26.01.02, in the Eastern part of the Sun disc.
 
NOAA 09798The insignificant bipolar sunspots were settled at the Sun equator since 22.01 to 29.01.02.
 
NOAA 09799The small bipolar group was observed at the 24th parallel of the Southern hemisphere since 22.01 to 1.02.02. The tail sunspot had oblong penumbra and bifurcated from time to time. The total region's area reached 150 m.s.h.
 












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