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Дата изменения: Wed Feb 3 21:00:55 2016
Дата индексирования: Sun Apr 10 02:13:22 2016
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Поисковые слова: ngc 7023
The Sunspot Observer - The solar regions - The description of the solar regions

Statistics of sunspot activity

NOAA 09900 - NOAA 09999
The description of the solar regions

NOAA 09900The long bipolar chain of small sunspots were observed at the 29th parallel of the Southern hemisphere since 6.04 to 14.04.02. The total region's area reached 150 m.s.h., and it was counted 15-20 sunspots in the group.
 
NOAA 09901The long chain of developed sunspots adjoined to the bipolar region 09893 from the East. The group was observed at the high latitudes of the Northern hemisphere since 7.04 to 16.04.02. The total region's area reached 300-400 m.s.h.
 
NOAA 09902The bipolar combination of sunspots crossed the Sun disc since 7.04 to 19.04.02 along the mid latitudes of the Northern hemisphere. The head sunspot had perceptible symmetrical penumbra, and the tail sunspots were moved away on the considerable longitude's distance. From time to time the total bipole's area exceeded 100 m.s.h.
 
NOAA 09903The insignificant bipolar formation was observed since 8.04 to 16.04.02 hardly to the North from the bipolar region 09902.
 
NOAA 09904The fine bipolar group was noticed at the mid latitudes of the Southern hemisphere since 8.04 to 13.04.02, in the Western part of the Sun disc.
 
NOAA 09905The fine bipolar group was observed since 10.04 to 16.04.02 to South-West from the sunspot 09896.
 
NOAA 09906The big multipolar group crossed the Sun disc since 9.04 to 21.04.02 along the mid latitudes of the Southern hemisphere. The group was slowly increasing the area and stretched by a latitude. Before set for the limb the total region's area had reached 800 m.s.h. The multipole was liked as a heavy chain of powerful, developed sunspots.
 
NOAA 09907The spreading bipolar group was decaying at the Sun disc since 11.04 to 21.04.02. In the first days the total region's area reached 300-400 m.s.h. It was counted more 30 sunspots in the group.
 
NOAA 09908The short-time bipolar sunspots were marked at the low latitudes of the Northern hemisphere since 12.04 to 15.04.02, in the Western part of the Sun disc.
 
NOAA 09909The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 14.04 to 25.04.02 along the low latitudes of the Northern hemisphere. The total region's area exceeded 100 m.s.h. From time to time satellites with opposite magnetic polarity appeared neighbouring the sunspot.
 
NOAA 09910The bipolar combination of developed sunspots with penumbraes crossed the Sun disc since 15.04 to 25.04.02 along the high latitudes of the Southern hemisphere. The total region's area reached 200 m.s.h. After intersection of the central meridian the tail part of the group began decay.
 
NOAA 09911The short-time bipolar group was marked at the mid latitudes of the Southeern hemisphere since 18.04 to 20.04.02, to the East from the central meridian.
 
NOAA 09912The developing bipolar group was observed at the tenth parallel of the Northern hemisphere since 18.04 to 27.04.02. The group originated to the East from the central meridian, and in three days the total area had increased in ten times and reached 300 m.s.h. It was counted more twenty sunspots in the bipole. The group was liked a curved serpent.
 
NOAA 09913The fine bipolar group was observed at the mid latitudes of the Southern hemisphere since 19.04 to 26.04.02.
 
NOAA 09914The opened bipolar group crossed the Sun disc since 19.04 to 1.05.02 along the low latitudes of the Northern hemisphere. The bipole consisted of the head and tail sunspots with developed penumbraes. Fine sunspots and pores appeared and disappeared between its. The total region's area reached 250 m.s.h.
 
NOAA 09915The crowded congestion of bipolar sunspots crossed the Sun disc since 20.04 to 1.05.02 along the mid latitudes of the Norrthern hemisphere. Several sunspots were embedded into asymmetrical penumbra, and fine sunspots were behind it. The total region's area reached 200 m.s.h.
 
NOAA 09916The small bipolar group was observed at the mid latitudes of the Southern hemisphere since 21.04 to 29.04.02. In the first days the total region's area reached 150 m.s.h.
 
NOAA 09917The fine one-day group was marked at the thirtieth parallel of the Southern hemisphere on 22.04.02 in the Eastern part of the Sun disc.
 
NOAA 09918The bipolar one-day pores was noticed on 22.04.02 in the Sun disc's center.
 
NOAA 09919The small bipolar group crossed the Sun disc since 22.04 to 4.05.02 along the mid latitudes of the Northern hemisphere. The bipole consisted of perceptible sunspot with symmetrical penumbra and fine tail sunspots. The group was settled to meridianal direct. In the first days the total region's area reached 200 m.s.h.
 
NOAA 09920The short-time bipolar sunspots were noticed at 24th parallel of the Southern hemisphere since 23.04 to 27.04.02.
 
NOAA 09921The fine bipolar sunspots were noticed since 24.04 to 29.04.02 to the East from the bipolar region 09915.
 
NOAA 09922The high latitude pores were observed in the Northern hemisphere since 23.04 to 1.05.02.
 
NOAA 09923The short-time bipolar sunspots were marked at the low latitudes of the Southern hemisphere since 24.04 to 27.04.02, in the Western part of the Sun disc.
 
NOAA 09924The short-time bipolar sunspots were marked at the mid latitudes of the Southern hemisphere since 24.04 to 27.04.02.
 
NOAA 09925The short-time bipolar sunspots were marked at the mid latitudes of the Southern hemisphere since 24.04 to 27.04.02, in the Western part of the Sun disc.
 
NOAA 09926The small bipolar group crossed the Sun disc since 24.04 to 5.05.02 along the mid latitudes of the Northern hemisphere. The bipole consisted of two nearby sunspots with penumbraes.
 
NOAA 09927The fine bipolar group was situated at the 28th parallel of the Southern hemisphere since 29.04 to 5.05.02, in the Eastern part of the Sun disc. The head sunspot had symmetrical penumbra.
 
NOAA 09928The small bipolar formation of irregular form was observed at the mid latitudes of the Northern hemisphere since 29.04 to 8.05.02. The total region's area reached 100 m.s.h.
 
NOAA 09929The new bipolar group had originated at the high latitudes of the Northern hemisphere on 30.04.02, to the East from the central meridian. The head sunspot of the group was gradually extending and complicating the form. Before set for the limb the total region's area reached 200 m.s.h. The bipole was observed until 7.05.
 
NOAA 09930The fine bipolar formatiion was marked at the mid latitudes of the Northern hemisphere since 30.04 to 3.05.02, in the Western part of the Sun disc.
 
NOAA 09931The fine bipolar group crossed the Sun disc since 30.04 to 9.05.02 along the mid latitudes of the Northern hemisphere.
 
NOAA 09932The length bipolar combination of fine sunspots was observed at the 27th parallel of the Southern hemisphere since 1.05 to 11.05.02.
 
NOAA 09933The small sunspot with symmetrical penumbra crossed the Sun disc since 30.04 to 13.05.02 along the mid latitudes of the Northern hemisphere. From time to time the total sunspot's area reached 100 m.s.h.
 
NOAA 09934The big bipolar group crossed the Sun disc since 1.05 to 15.05.02 along the mid latitudes of the Southern hemisphere. The bipole consisted of the large sunspot with symmetrical penumbra and developing congestion of many sunspots which was settled to the South.
 
NOAA 09935The fine bipolar group was observed at the high latitudes of the Southern hemisphere since 2.05 to 9.05.02.
 
NOAA 09936The fine bipolar group was observed at the mid latitudes of the Southern hemisphere since 2.05 to 9.05.02.
 
NOAA 09937The perceptible bipolar group crossed the Sun disc since 3.05 to 15.05.02 along the low latitudes of the Southern hemisphere. The bipole consisted of two nearby sunspots with penumbraes which were slowly dispersed. Pores appeared and disappeared neighbouring the sunspots. The total region's area reached 200-250 m.s.h.
 
NOAA 09938The fine sunspot with symmetrical penumbra was noticed since 3.05 to 12.05.02 hardly to the North-East from the region 09937.
 
NOAA 09939The fine sunspot with symmetrical penumbra was observed at the high latitudes of the Northern hemisphere since 4.05 to 10.05.02, in the Eastern part of the Sun disc.
 
NOAA 09940The fine bipolar group was marked since 4.05 to 14.05.02 hardly to the South from the region 09939.
 
NOAA 09941The fine bipolar formation was observed since 4.05 to 10.05.02 hardly to the North from the bipolar region 09932.
 
NOAA 09942The short-time sunspots were marked at the high latitudes of the Northern hemisphere since 5.05 to 7.05.02, in the Eastern part of the Sun disc.
 
NOAA 09943The fine sunspots were settled at the tenth parallel of the Southern hemisphere since 4.05 to 11.05.02.
 
NOAA 09944The short-time bipolar formation was noticed since 7.05 to 9.05.02 near the fine regions 09939 and 09940.
 
NOAA 09945The big bipolar group crossed the Sun disc since 6.05 to 19.05.02 along the equator. The bipole consisted of the large sunspot with penumbra and fine sunspots behind it. From time to time the total region's area reached 400 m.s.h.
 
NOAA 09946The fine bipolar group was observed to the East from the big region 09945 since 8.05 to 18.05.02.
 
NOAA 09947The fine bipolar formation was situated at the high latitudes of the Northern hemisphere since 5.05 to 11.05.02.
 
NOAA 09948The big sunspot with imposing symmetrical penumbra crossed the Sun disc since 10.05 to 22.05.02 along the high latitudes of the Southern hemisphere. The total region's area reached 400 m.s.h.
 
NOAA 09949The fine bipolar formation was observed at the mid latitudes of the Southern hemisphere since 10.05 to 15.05.02, in the Western part of the Sun disc.
 
NOAA 09950The small bipolar formation crossed the Sun disc since 11.05 to 20.05.02 along the low latitudes of the Southern hemisphere. The head sunspot had symmetrical penumbra. From time to time the total region's area reached 100 m.s.h.
 
NOAA 09951The insignificant sunspot with symmetrical penumbra was observed at the tenth parallel of the Northern hemisphere since 12.05 to 18.05.02.
 
NOAA 09952The one-day pore was noticed on 13.05.02 to the South-West from the region 09945.
 
NOAA 09953The fine bipolar sunspots were noticed on 15.05 and 16.05.02 not far from the Western limb.
 
NOAA 09954The small double sunspot crossed the Sun disc since 14.05 to 25.05.02 along the high latitudes of the Southern hemisphere. In the first days the total region's area exceeded 100 m.s.h.
 
NOAA 09955The fine sunspot with symmetrical penumbra was observed since 15.05 to 22.05.02 to the North from the region 09954.
 
NOAA 09956The one-day pore was noticed on 16.05.02 in the central part of the Sun disc.
 
NOAA 09957The big multipolar group crossed the Sun disc since 15.05 to 28.05.02 along the tenth parallel of the Northern hemisphere. The multipole had very unusual, arrow-like form. The arrow's top was made from developed sunspots with penumbraes, and the arrow's base consisted of many fine sunspots which were embedded into several pieces of penumbra. From time to time the total region's area reached 1000 m.s.h., and it was counted more 50 sunspots in the group. After intersection of the central meridian the group began decay.
 
NOAA 09958The small sunspot with symmetrical penumbra was observed since 15.05 to 27.05.02 to the South-West from the big region 09957.
 
NOAA 09959The bipolar one-day pores were marked on 17.05.02 in the central part of the Sun disc.
 
NOAA 09960The small bipolar group crossed the Sun disc since 17.05 to 29.05.02 along the mid latitudes of the Northern hemisphere. The double head sunspot was gradually diminishing and assuming symmetrical form. In the first days the total region's area exceeded 150 m.s.h.
 
NOAA 09961The long bipolar group crossed the Sun disc since 19.05 to 31.05.02 along the high latitudes of the Southern hemisphere. In the first days the total region's area exceeded 300 m.s.h. The group consisted of several developed sunspots, but it was the head sunspot with symmetrical penumbra only which reached the Western limb.
 
NOAA 09962The small sunspot with symmetrical penumbra was observed since 19.05 to 29.05.02 between the regions 09960 and 09963.
 
NOAA 09963The big bipolar group crossed the Sun disc since 20.05 to 1.06.02 along the mid latitudes of the Northern hemisphere. The group consisted of the large sunspot with asymmetrical penumbra and many fine spots and pores behind it. The total region's area reached 400 m.s.h., and maximal sunspot's quantity exceeded 30 units.
 
NOAA 09964The fine bipolar group was observed since 21.05 to 27.05.02 to the North-West from the big region 09961.
 
NOAA 09965The fine sunspot with symmetrical penumbra crossed the Sun disc since 21.05 to 1.06.02 along the low latitudes of the Southern hemisphere. From time to time pores with opposite magnetic polarity were observed neighbouring the sunspot.
 
NOAA 09966The insignificant bipolar group was situated at the South-Western district of the big region 09963 since 23.05 to 29.05.02.
 
NOAA 09967The insignificant bipolar group was situated at the Eastern district of the big region 09963 since 23.05 to 31.05.02.
 
NOAA 09968The short-time formation was noticed since 24.05 to 26.05.02 between the regions 09961 and 09965.
 
NOAA 09969The fine bipolar group was observed since 25.05 to 1.06.02 hardly to the North from the region 09970.
 
NOAA 09970The opened bipolar group crossed the Sun disc since 25.05 to 5.06.02 along the low latitudes of the Northern hemisphere. The head and tail sunspots had developed symmetrical penumbraes. The total region's area reached 150-200 m.s.h.
 
NOAA 09971The bipolar one-day pores were noticed on 28.05.02 in the central part of the Sun disc.
 
NOAA 09972The fine bipolar sunspots were marked since 28.05 to 6.06.02 to the West from the big region 09973.
 
NOAA 09973The big bipolar group crossed the Sun disc since 28.05 to 10.06.02 along the mid latitudes of the Southern hemisphere. The group consisted of developed sunspots with powerful penumbraes. In the first days the total region's area exceeded 800 m.s.h. After intersection the central meridian the head part of the group began decay, and the most developed tail sunspot assumed symmetrical form and reached the Western limb.
 
NOAA 09974The fine sunspot with symmetrical penumbra crossed the Sun disc since 28.05 to 5.06.02 along the mid latitudes of the Northern hemisphere.
 
NOAA 09975The fine bipolar sunspots were marked since 29.05 to 9.06.02 to the North from the region 09974.
 
NOAA 09976The short-time bipolar pores were observed at the tenth parallel of the Southern hemisphere since 30.05 to 1.06.02, to the West from the central meridian.
 
NOAA 09977The high latitude bipolar group was noticed in the Southern hemisphere since 1.06 to 3.06.02, near the Western limb.
 
NOAA 09978The developed bipolar group crossed the Sun disc since 31.05 to 11.06.02 along the high latitudes of the Southern hemisphere. The total region's area reached 250 m.s.h. After intersection of the central meridian the decay's process formed which began since the tail sunspots.
 
NOAA 09979The fine bipolar sunspots were marked at the thirtieth parallel of the Southern hemisphere since 31.05 to 6.06.02.
 
NOAA 09980The insignificant sunspot with symmetrical penumbra was observed at the 29th parallel of the Southern hemisphere since 1.06 to 5.06.02.
 
NOAA 09981The small sunspot with symmetrical penumbra crossed the Sun disc since 2.06 to 11.06.02 along the high latitudes of the Southern hemisphere.
 
NOAA 09982The recurrent pores were observed at the Sun disc since 2.06 to 10.06.02.
 
NOAA 09983The fine sunspot with symmetrical penumbra was observed at the 24th parallel of the Northern hemisphere since 2.06 to 8.06.02, in the Eastern part of the Sun disc.
 
NOAA 09984The short-time pores were noticed at the high latitudes of the Northern hemisphere since 3.06 to 5.06.02, neighbouring the central meridian.
 
NOAA 09985The long bipolar group was observed since 4.06 to 13.06.02 at the high latitudes of the Northern hemisphere. The bipole consisted of developed head and tail sunspots with penumbraes. From time to time many fine sunspots and pores were visible between its. The total region's area reached 200 m.s.h.
 
NOAA 09986The fine sunspot with symmetrical penumbra was observed at the Sun equator since 4.06 to 10.06.02, in the Eastern part of the Sun disc.
 
NOAA 09987The solid chain of small sunspots had appeared at the mid latitudes of the Southern hemisphere on 6.06.02, to the East from the central meridian. After intersection of the central meridian one of the head sunspots began extend, and the chain turned into slow decay. Before set for the limb the total region's area reached 400 m.s.h. The group was observed until 14.06.
 
NOAA 09988The bipolar one-day pores were observed on 6.06.02 in the central part of the Sun disc.
 
NOAA 09989The short-time sunspots were noticed at the 35th parallel of the Southern hemisphere since 6.06 to 8.06.02, in the Western part of the Sun disc.
 
NOAA 09990The bipolar pores were marked to the South-East from the bipolar region 09987 since 7.06 to 10.06.02.
 
NOAA 09991The big sunspot with oblong penumbra crossed the Sun disc since 7.06 to 19.06.02 along the high latitudes of the Southern hemisphere. From time to time pores with opposite magnetic polarity were observed neighbouring the sunspot. The total region's area reached 300 m.s.h.
 
NOAA 09992The fine bipolar group followed behind the big sunspot 09991 since 8.06 to 15.06.02.
 
NOAA 09993The small sunspot with symmetrical penumbra was observed at the low latitudes of the Northern hemisphere since 9.06 to 13.06.02, in the Western part of the Sun disc. In the first days pores with opposite magnetic polarity were observed neighbouring the sunspot.
 
NOAA 09994The insigniificant sunspots were marked at the tenth parallel of the Northern hemisphere since 9.06 to 11.06.02, in the Eastern part of the Sun disc.
 
NOAA 09995The bipolar pores were marked at the tenth parallel of the Northern hemisphere since 10.06 to 13.06.02, to the West from the central meridian.
 
NOAA 09996The high latitude pores were noticed in the Southern hemisphere since 11.06 to 13.06.02, in the Eastern part of the Sun disc.
 
NOAA 09997The insignificant sunspots crossed the Sun disc since 12.06 to 20.06.02 along the tenth parallel of the Sun disc.
 
NOAA 09998The insignificant sunspots were observed at the mid latitudes of the Northern hemisphere since 12.06 to 18.06.02, in the Eastern part of the Sun disc.
 
NOAA 09999The insignificant near equatorial sunspots were observed since 13.06 to 16.06.02 near the Western limb.
 












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