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Дата изменения: Wed Feb 3 21:01:14 2016
Дата индексирования: Sun Apr 10 02:17:28 2016
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The Sunspot Observer - The solar regions - The description of the solar regions

Statistics of sunspot activity

NOAA 11200 - NOAA 11299
The description of the solar regions

NOAA 11200The recurrent bipolar pores were observed at the middle latitudes of the Southern hemisphere since 27.04 to 7.05.
 
NOAA 11201The middle latitude pores were noticed on 6.05 and 7.05 in the Northern hemisphere, near the Western limb.
 
NOAA 11202The recurrent sunspots were marked since 29.04 to 1.05 at the 15th parallel of the Northern hemisphere, near the Western limb.
 
NOAA 11203The symmetrcal sunspot with a stable penumbra crossed the Sun disc since 29.04 to 11.05 along the middle latitudes of the Northern hemisphere. Time to time neighboring the sunspot there were pores of an opposite magnetic polarity.
 
NOAA 11204The small bipolar group was observed to the West from the sunspot 11204 since 3.05 to 12.05.
 
NOAA 11205The middle latitude pores were noticed in the Northern hemisphere since 3.05 to 7.05 neighboring the central meridian.
 
NOAA 11206The bipolar pores were marked at the high latitudes of the Northern hemisphere since 4.05 to 7.05.
 
NOAA 11207The recurrent bipolar pores crossed the Sun disc along the high latitudes of the Northern hemisphere since 6.05 to 13.05.
 
NOAA 11208The fine bipolar sunspots crossed the Sun disc along the tenth parallel of the Northern hemisphere since 8.05 to 18.05.
 
NOAA 11209The short-time bipolar pores were marked at the 35th parallel of the Northern hemisphere on 9.05 and 10.05, neighboring the central meridian.
 
NOAA 11210The undeveloped sunspots were observed at the 20th parallel of the Northern hemisphere since 10.05 to 16.05, in the Western part of the Sun disc.
 
NOAA 11211The bipolar one-day pores were noticed at the 12th parallel of the Northern hemisphere on 10.05, in the Western part of the Sun disc.
 
NOAA 11212The one-day pore was marked at the 13th parallel of the Southern hemisphere on 10.05, in the Eastern part of the Sun disc.
 
NOAA 11213The high latitude pore was noticed at the Western limb on 15.05, in the Southern hemisphere.
 
NOAA 11214The high latitude shain of fine sunspots was observed in the Southern hemisphere since 15.05 to 22.05, to the West from the central meridian.
 
NOAA 11215The bipolar one-day pores were noticed at the 23rd parallel of the Southern hemisphere on 15.05, in the Weatern part of the Sun disc.
 
NOAA 11216The single sunspot with symmetrical penumbra crossed the Sun disc since 17.05 to 28.05 along 15th parallel of the Southern hemisphere.
 
NOAA 11217The short-time bipolar pores were marked on 18.05 and 19.05 at the 23rd parallel of the Southern hemisphere, in the Western part of the Sun disc.
 
NOAA 11218The middle latitude pores were observed in the Southern hemisphere since 19.05 to 23.05.
 
NOAA 11219The middle latitude one-day pore was observed in the Northern hemisphere on 22.05, not far from the Eastern limb.
 
NOAA 11220The bipolar pores were marked at the middle latitudes of the Northern hemisphere on 23.05 and 24.05, near the Western part.
 
NOAA 11221The bipolar pores were marked at the middle latitudes of the Southern hemisphere on 24.05 and 25.05, near the Western part.
 
NOAA 11222The recurrent pores were observed at the middle latitudes of the Northern hemisphere since 26.05 to 30.05, in the Western part of the Sun disc.
 
NOAA 11223The fine sunspots were noticed at the middle latitudes of the Southern hemisphere since 27.05 to 30.05, to the West from the central meridian.
 
NOAA 11224The small bipolar group was marked at the 20th parallel of the Northern hemisphere since 28.05 to 1.06, in the Western part of the Sun disc.
 
NOAA 11225The fine sunspot with symmetrical penumbra crossed the Sun disc along the middle latitudes of the Northern hemisphere since 28.05 to 5.06.
 
NOAA 11226The sprawling bipolar group crossed the Sun disc since 28.05 to 8.06 along the high latitudes of the Southern hemisphere. The bipole arose with the developed head part and numerous small spots behind it. Two-three days later the head sunspots started moving away from each other. When the East head sunspot reached the tail part of the group, the bipole started being scattered. In the evolution's peak the total region's area exceeded 300 m.h.s.
 
NOAA 11227The simple bipolar group followed the region 11226. It was observed since 30.05 to 10.06.
 
NOAA 11228The small bipolar group crossed the Sun disc since 30.05 to 10.06 along the middle latitudes of the Northern hemisphere. The head sunspot had a stable symmetrical penumbra.
 
NOAA 11229The fine bipolar sunspots were observed at the middle latitudes of the Northern hemisphere since 31.05 to 5.06.
 
NOAA 11230The pores were noticed to the East from the region 11228. Its were observed since 1.06 to 5.06.
 
NOAA 11231The fine sunspots were marked at the tenth parallel of the Northern hemisphere since 2.06 to 5.06, to the East from the central meridian.
 
NOAA 11232The small sunspot with a symmetrical penumbra was following the region 11231. It was observed since 3.06 to 12.06. Time to time neighboring the sunspot there were pores with an opposite magnetic polarity.
 
NOAA 11233The short-time pore was noticed in the Southern hemisphere 6.06 and 7.06, not far from the Western limb.
 
NOAA 11234The small bipolar group crossed the Sun disc since 10.06 to 20.06 along the middle latitudes of the Southern hemisphere.
 
NOAA 11235The recurrent pores were observed at the middle latitudes of the Northern hemisphere 12.06 and 15.06, neighboring the central meridian.
 
NOAA 11236The noticeable bipolar group crossed the Sun disc since 15.06 to 26.06 along the middle latitudes of the Northern hemisphere. The bipole consisted of two umbras with general symmetrical penumbra and small tail sunspots. Couple of the head sunspots gradually merged in uniform symmetrical formation, and the tail part of the group broke up. Time to time the total region's area reached 350 m.h.s., and in the group it was counted more fifteen sunspots.
 
NOAA 11237The short-time pore was noticed 18.06 and 19.06 at the middle latitudes of the Southern hemisphere, in the Eastern part of the Sun disc.
 
NOAA 11238The one-day pores were marked at the central meridian 20.06, at the middle latitudes of the Southern hemisphere.
 
NOAA 11239The bipolar pores were observed at the middle latitudes of the Northern hemisphere since 21.06 to 26.06, to the West from the central meridian.
 
NOAA 11240The fine sunspots were marked at the 20th parallel of the Southern hemisphere since 21.06 to 26.06.
 
NOAA 11241The fine bipolar sunspots were observed at the middle latitudes of the Northern hemisphere since 24.06 to 28.06, in the Western part of the Sun disc.
 
NOAA 11242The fine bipolar sunspots were observed at the middle latitudes of the Northern hemisphere since 28.06 to 4.07, in the Western part of the Sun disc.
 
NOAA 11243The fine bipolar sunspots crossed the Sun disc since 28.06 to 9.07 along the middle latitudes of the Northern hemisphere.
 
NOAA 11244The fine bipolar sunspots were observed at the middle latitudes of the Northern hemisphere since 2.07 to 6.07, in the Western part of the Sun disc.
 
NOAA 11245The fine sunspots crossed the Sun disc since 7.07 to 17.07 along the middle latitudes of the Northern hemisphere.
 
NOAA 11246The middle latitude pores were noticed in the Northern hemisphere since 7.07 to 10.07, not far from the Western limb.
 
NOAA 11247The undistinguished bipolar sunspots were observed at the middle latitudes of the Southern hemisphere since 8.07 to 15.07 to the West from the central meridian.
 
NOAA 11248The short-time pore was marked at the 20th parallel of the Northern hemisphere 8.07 and 9.07, in the Eastern part of the Sun disc.
 
NOAA 11249The fine sunspots were observed at the middle latitudes of the Northern hemisphere since 9.07 to 15.07.
 
NOAA 11250The small bipolar group crossed the Sun disc since 10.07 to 20.07 along the 25th parallel of the Southern hemisphere. The head sunspot had a stable symmetrical penumbra.
 
NOAA 11251The single sunspot with a stable symmetrical penumbra crossed the Sun disc since 11.07 to 23.07 along the 15th parallel of the Northern hemisphere.
 
NOAA 11252The fine sunspots were marked at the 25th parallel of the Northern hemisphere since 13.07 to 17.07, in the Eastern part of the Sun disc.
 
NOAA 11253The bipolar pores were noticed at the middle latitudes of the Northern hemisphere 13.07 and 14.07, to the West from the central meridian.
 
NOAA 11254The fine bipolar sunspots crossed the Sun disc since 13.07 to 26.07 along the high latitudes of the Southern hemisphere.
 
NOAA 11255The bipolar pores were marked at the middle latitudes of the Northern hemisphere since 15.07 to 19.07, neighboring the central meridian.
 
NOAA 11256The undistinguished bipolar sunspots were observed since 15.07 to 20.07 at the tenth parallel of the Northern hemisphere.
 
NOAA 11257The growing bipolar sunspots were noticed at the 20th parallel of the Northern hemisphere since 17.07 to 20.07, not far from the Western limb.
 
NOAA 11258The fine bipolar sunspots were noticed at the tenth parallel of the Northern hemisphere since 18.07 to 22.07, not far from the Western limb.
 
NOAA 11259The fine bipolar sunspots were observed since 18.07 to 25.07 at the 25th parallel of the Northern hemisphere.
 
NOAA 11260The noticable bipolar group crossed the Sun disc since 24.07 to 5.08 along the 20th parallel of the Northern hemisphere. In the first days the bipole represented a shain of developed sunspots with penumbraes. In the next days the shain began fail, and the head sunspot was growing. In the evolution's peak the total region's area exceeded 300 m.h.s., and in the group it was counted more twenty sunspots.
 
NOAA 11261The big multipolar group crossed the Sun disc since 26.07 to 7.08 along the 15th parallel of the Northern hemisphere. The multipole continuously changed the spatial configuration, in the first days the group accepted a freakish form of a horseshoe. In the evolution's peak the total region's area reached 350 m.h.s., and in the group it was counted fifty sunspots about.
 
NOAA 11262The fine bipolar group was noticed in the Northern hemisphere since 27.07 to 29.07, not far from the Western limb.
 
NOAA 11263The large bipolar formation crossed the Sun disc since 28.07 to 10.08. The bipole followed the group 11261 and represented two large umbraes with developed penumbraes. Neighboring the central meridian these sunspots began split up stretching all the group along parallel. In the evolution's peak the total region's area exceeded 700 m.h.s., in the group it was counted more twenty sunspots.
 
NOAA 11264The bipolar pores were marked at the 30th parallel of the Southern hemisphere since 28.07 to 1.08, to the East from the central meriidian.
 
NOAA 11265The bipolar pores were noticed in the Northern hemisphere since 30.07 to 3.08, not far from the Western limb.
 
NOAA 11266The undistinguished sunspots were observed since 3.08 to 14.08 at the middle latitudes of the Northern hemisphere.
 
NOAA 11267The fine bipolar sunspots were observed since 5.08 to 10.08 at the middle latitudes of the Southern hemisphere.
 
NOAA 11268The middle latitude pores were marked in the Northern hemisphere since 6.08 to 11.08.
 
NOAA 11269The short-time pores were noticed at the high latitudes of the Southern hemisphere since 11.08 to 14.08, neighboring the central meridian.
 
NOAA 11270The undistinguished sunspots were observed at the high latitudes of the Northern hemisphere since 11.08 to 14.08, in the Eastern part of the Sun disc.
 
NOAA 11271The noticeable bipolar group crossed the Sun disc since 15.08 to 28.08 along the middle latitudes of the Northern hemisphere. In the first days the bipole consisted of three sunspots with developed penumbraes making a rectangular triangle. In the next days the tail sunspot started growing and was split up. In the evolution's peak the total region's area reached 300 m.h.s., and in the group it was counted more twenty five sunspots.
 
NOAA 11272The fine bipolar sunspots crossed the Sun disc since 16.08 to 26.08 along the 20th parallel of the Southern hemisphere.
 
NOAA 11273The bipolar pores were marked at the 18th parallel of the Southern hemisphere since 17.08 to 20.08, to the West from the central meridian.
 
NOAA 11274The fine recurrent sunspots were observed at the middle latitudes of the Northern hemisphere since 20.08 to 2.09.
 
NOAA 11275The undistinguished sunspots crossed the Sun disc since 21.08 to 30.08 along the low latitides of the Northern hemisphere.
 
NOAA 11276The short-time pore was noticed at the 20th parallel of the Northern hemisphere 23.08 and 24.08, in the Eastern part of the Sun disc.
 
NOAA 11277The fine sunspot with a symmetrical penumbra crossed the Sun disc since 25.08 to 6.09 along the middle latitudes of the Northern hemisphere.
 
NOAA 11278The fine sunspots were observed in the Northern hemisphere since 25.08 to 29.08, not far from the Western limb.
 
NOAA 11279The small sunspot with a symmetrical penumbra crossed the Sun disc since 25.08 to 4.09 along the middle latitudes of the Northern hemisphere.
 
NOAA 11280The fine bipolar sunspots were observed at the middle latitudes of the Northern hemisphere since 26.08 to 4.09.
 
NOAA 11281The small bipolar group crossed the Sun disc since 28.08 to 8.09 along the middle latitudes of the Southern hemisphere.
 
NOAA 11282The small bipolar group was observed at the high latitudes of the Northern hemisphere since 30.08 to 6.09, to the West from the central meridian. Main sunspots had symmetrical penumbraes.
 
NOAA 11283The sprawling bipolar group crossed the Sun disc since 30.08 to 12.09 along the middle latitudes of the Northern hemisphere. In the evoluion's peak the total region's area exceeded 200 m.h.s., and in the group it was counted twenty sunspots about.
 
NOAA 11284The middle latitude pores were marked in the Southern hemisphere since 30.08 to 2.09, not far from the Western limb.
 
NOAA 11285The short-time pore was noticed at the high lattudes of the Northern hemisphere 31.08 and 1.09, in the Western part of the Sun disc.
 
NOAA 11286The bipolar sunspots were marked at the Western limb of the Northern hemisphere since 3.09 to 5.09.
 
NOAA 11287The fine sunspot with a symmetrical penumbra crossed the Sun disc since 3.09 to 15.09 along the 30th parallel of the Southern hemisphere. Time to time there were sunspots with an opposite magnetic polarity neighboring the sunspot.
 
NOAA 11288The high latitude pores were marked in the Northern hemisphere since 5.09 to 7.09 neighboring the central meridian.
 
NOAA 11289Two large umbraes with the general penumbra crossed the Sun disc since 5.09 to 19.09 along the high latitudes of the Northern hemisphere. Neighboring the double sunspot there were numerous sunspots and pores of different magnetic polarity. Neighboring the central meridian the total region's area reached 450 m.h.s., and in the group it was counted more fifteen sunspots.
 
NOAA 11290The fine bipolar sunspots were observed since 9.09 to 18.09 at the middle latitudes of the Southern hemisphere.
 
NOAA 11291The recurrent sunspots were observed at the high latitudes of the Northern hemisphere since 10.09 to 17.09, in the Western part of the Sun disc.
 
NOAA 11292The fine sunspots were marked at the low latitudes of the Northern hemisphere since 11.09 to 18.09, in the Western part of the Sun disc.
 
NOAA 11293The fine bipolar sunspots were noticed at the middle latitudes of the Northern hemisphere since 12.09 to 17.09, in the Eastern part of the Sun disc.
 
NOAA 11294The fine bipolar sunspots were observed at the middle latitudes of the Southern hemisphere since 12.09 to 18.09, to the West from the central meridian.
 
NOAA 11295The growing bipolar group crossed the Sun disc since 12.09 to 24.09 along the high latitudes of the Northern hemisphere. Main sunspot with a large stable penumbra was situated in the central part of the bipole. Before the Western limb the total region's area exceeded 500 m.h.s., in the group it was counted more twenty sunspots.
 
NOAA 11296The disintegrated bipolar group was observed at the high latitudes of the Northern hemisphere since 13.09 to 24.09. The greatest sunspot was situated in the tail bipole's part and represented two umbraes with the general penumbra. To the East from the central meridian the total group's area reached 130 m.h.s.
 
NOAA 11297The fine bipolar sunspots were noticed in the Southern hemisphere since 14.09 to 17.09, not far from the Western limb.
 
NOAA 11298The fine bipolar sunspots were noticed since 14.09 to 22.09 to the South from the region 11295.
 
NOAA 11299The fine bipolar sunspots were observed at the high latitudes of the Southern hemisphere since 16.09 to 24.09, to the West from the central meridian.
 












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