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The Sunspot Observer - The solar regions - The description of the solar regions

Statistics of sunspot activity

NOAA 11100 - NOAA 11199
The description of the solar regions

NOAA 11100The high-latitude pore was marked in the Southern hemisphere since 17.08 to 22.08.
 
NOAA 11101The single sunspot with fine penumbra was crossed the Sun disc since 25.08 to 6.09 across the middle latitudes of the Northern hemisphere. Time to time the total sunspot area exceeded 100 m.h.s.
 
NOAA 11102The fine bipolar sunspots were noticed at the high latitudes of the Northern hemisphere since 10.08 to 5.09, in the Western part of the Sun disc.
 
NOAA 11103The bipolar pores were observed at the high latitudes of the Northern hemisphere since 2.09 to 5.09 near the Western limb.
 
NOAA 11104The bipolar one-day pores were noticed 2.09 at the high latitudes of the Northern hemisphere, in the Western part of the Sun disc.
 
NOAA 11105The small bipolar group was marked at the phase moderate development since 3.09 to 8.09 at the middle latitudes of the Northern hemisphere, in the Western part of the Sun disc.
 
NOAA 11106The long shain of fine sunspots was crossed the Sun disc since 11.09 to 21.09 along the high latiudes of the Southern hemisphere. The head sunspot had a stable symmetrical penumbra.
 
NOAA 11107The high-latitude one-day pore was noticed at the 33rd parallel of the Northern hemisphere on 13.09, not far from the Eastern limb.
 
NOAA 11108The pair of the close located large sunspots with developed penumbraes was crossed the Sun disc since 16.09 to 28.09 along the high latiudes of the Southern hemisphere. Time to time the total group's area exceeded 400 m.h.s., and sunspo's number reached fifteen units.
 
NOAA 11109The long shain of the developed sunspots was crossed the Sun disc since 22.09 to 3.10 along the high latitudes of the Northern hemisphere. The larg head sunspot had a developed penumbra. In process of advance on the Sun disc the sunspot shain was gradually broken up. Time to time the total group's area exceeded 400 m.h.s., and sunspot's number reached twenty five units.
 
NOAA 11110The fine sunspots were observed at the 20th parallel of the Northern hemisphere since 27.09 to 2.10, in the Western part of the Sun disc.
 
NOAA 11111The small bipolar sunspots were marked at the high latitudes of the Northern hemisphere since 30.09 to 5.10.
 
NOAA 11112The fine sunspots crossed the Sun disc since 10.10 to 20.10 along the middle latitudes of the Southern hemisphere.
 
NOAA 11113The two umbraes with the general symmetric penumbra crossed the Sun disc since 14.10 to 25.10 along the middle latitudes of the Northern hemisphere.
 
NOAA 11114The high-latiude pores were noticed since 15.10 to 17.10 in the Southern hemisphere, near the Western limb.
 
NOAA 11115The stable sunspot with the symmetrical penumbra crossed the Sun disc since 16.10 to 28.10 along the 30th parallel of the Southern hemisphere. Time to time neighboring the sunspot there were pores of opposite magneic polarity, and the total group's area reached 200 m.h.s.
 
NOAA 11116The undistinguished pores were marked at the high latitudes of the Northern hemisphere since 18.10 to 21.10, in the Western part of the Sun disc.
 
NOAA 11117The developing bipolar group crossed the Sun disc since 20.10 to 31.10 along the high latitudes of the Northern hemisphere. The group appeared near the Eastern limb as a developed sunspot with symmetrical penumbra. Three days later to the South from the single umbra there was a new sunspots shain, its development had finished by formation of head and tail sunspots with large penumbraes. Near the Western limb the total region's area reached 500 m.h.s., and in the group it was counted thirty sunspots.
 
NOAA 11118The fine sunspots were marked since 24.10 to 30.10 to the West from the group NOAA 11117.
 
NOAA 11119The fine sunspots were noticed since 25.10 to 27.10 at the high latitudes of the Northern hemisphere, not far from the Western limb.
 
NOAA 11120The undistinguished sunspots crossed the Sun disc since 31.10 to 8.11 along 38th parallel of the Northern hemisphere.
 
NOAA 11121The shain of fine sunspots crossed the Sun disc since 5.11 to 11.11 along the 20th parallel of the Southern hemisphere.
 
NOAA 11122The fine sunspots were observed at the middle latitudes of the Northern hemisphere since 6.11 to 10.11, in the Western part of the Sun disc.
 
NOAA 11123The bipolar cloud of fine sunspots were marked at the high latitudes of the Southern hemisphere since 10.11 to 16.11. In the group it was counted ten-fifteen sunspots whereas the total area of the region didn't exceed hundred m.h.s.
 
NOAA 11124The growing bipolar group had arisen on 9.11 at the fifteen parallel of the Northern hemisphere, not far from the Eastern limb. In the process of development head and tail sunspots increased and gradually got a symmetrical form. Time to time the total region's area exceeded 300 m.h.s., and in the group it was counted not over ten-fifteen sunspots. On 19.11 the bipole reached the Western limb.
 
NOAA 11125The recurrent sunspots were noticed since 12.11 to 17.11 to the North from the group 11124.
 
NOAA 11126The small bipolar group crossed the Sun disc since 12.11 to 23.11 along the 30th parallel of the Southern hemisphere. The bipole had an arrow-shaped configuration, main sunspots had fine symmetrical penumbraes. The total region's area didn't exceed hundred m.h.s., in the group it was counted not over ten sunspots.
 
NOAA 11127The single sunspot with a stable symmetrical penumbra crossed the Sun disc since 16.11 to 27.11 along the 25th parallel of the Northern hemisphere. Time to time neighboring the sunspot there were pores of a opposite magnetic polarity.
 
NOAA 11128The short-time pores were noticed on 26.11 and 27.11 at the middle latitudes of the Southern hemisphere, in the Eastern part of the Sun disc.
 
NOAA 11129The high-latitude pores were marked at the Western limb of the Southern hemisphere on 29.11 and 30.11.
 
NOAA 11130The new bipolar group had appeared at the middle latitudes of the Northern hemisphere on 29.11, neighbouring the central meridian. In the process of development the total region's area exceeded 30 m.h.s., in the group it was counted fifteen sunspots. On 5.12 the head sunspot reached the Western limb.
 
NOAA 11131The large sunspot with a stable symmetrical penumbra crossed the Sun disc since 1.12 to 14.12 along 30th parallel of the Northern hemisphere. The maximal total sunspot's area exceeded 400 m.h.s.
 
NOAA 11132The recurrent pores were observed at the tenth parallel of the Northern hemisphere since 4.12 to 11.12, in the Western part of the Sun disc.
 
NOAA 11133The small sunspot with a symmetrical penumbra crossed the Sun disc since 4.12 to 16.12 along the middle latitudes of the Northern hemisphere.
 
NOAA 11134The fine sunspots were noticed at the middle latitudes of the Northern hemisphere 14.12 and 15.12, not far from the Western limb.
 
NOAA 11135The recurrent pores were observed at the middle latitudes of the Northern hemisphere since 14.12 to 25.12.
 
NOAA 11136The high latitude pores were noticed at the Western limb of the Southern hemisphere on 26.12 and 27.12.
 
NOAA 11137The short-time pores were noticed at the middle latitudes of the Northern hemisphere since 26.12 to 29.12, neighboring the central meridian.
 
NOAA 11138The fine bipolar sunspots were marked since 27.12.2010 to 1.01.2011 at the middle latitudes of the Northern hemisphere.
 
NOAA 11139The recurrent pores were noticed at the high latitudes of the Southern hemisphere since 30.12.2010 to 2.01.2011, neighboring the central meridian.
 
NOAA 11140The noticeable sunspot with a stable symmetrical penumbra crossed the Sun disc since 1.01 to 12.01.11 along 33rd parallel of the Northern hemisphere. Time to time there were pores of a opposite magnetic polarity neighboring the sunspot, and total region's area reached 200 m.h.s.
 
NOAA 11141The fine bipolar sunspots were noticed since 2.01 to 6.01 at the high latitudes of the Northern hemisphere, in the Western part of the Sun disc.
 
NOAA 11142The fine bipolar sunspots crossed the Sun disc since 2.01 to 10.01 along the middle latitudes of the Southern hemisphere.
 
NOAA 11143The short-time sunspots were noticed at the high latitudes of the Southern hemisphere on 8.01 and 9.01.
 
NOAA 11144The short-time pore was noticed on 10.01 at the high latitude of the Southern hemisphere, in the Western part of the Sun disc.
 
NOAA 11145The recurrent pores were observed at the middle latitudes of the Northern hemisphere since 10.01 to 15.01.
 
NOAA 11146The short-time pores were marked at the high latitudes of the Northern hemisphere since 11.01 to 14.01, neighboring the central meridian.
 
NOAA 11147The small bipolar group appeared at the high latitudes of the Northern hemisphere on 16.01, not far from the Eastern limb. The head sunspot had a stable symmetrical penumbra, and tail sunspots were gradually desintegrated. On 27.01 the group reached the Western limb.
 
NOAA 11148The fine bipolar sunspots were noticed at the 28th parallel of the Southern hemisphere since 18.01 to 21.01, not far from the Western limb.
 
NOAA 11149The developing bipolar sunspots were observed since 22.01 to 27.01 to the South from the group 11147.
 
NOAA 11150The fine bipolar sunspots were observed at the 20th parallel of the Southern hemisphere since 29.01 to 5.02.
 
NOAA 11151The middle latitude was noticed at the Western limb since 29.01 to 31.01.
 
NOAA 11152The short-time pores were marked at the 20th parallel of the Southern hemisphere since 4.02 to 7.02, to the West from the central meridian.
 
NOAA 11153The fine bipolar sunspots were observed at the middle latitudes of the Northern hemisphere since 5.02 to 10.02, not far from the Western limb.
 
NOAA 11154The one-day pore was noticed at the law latitudes of the Northern hemisphere on 9.02, in the Western part of the Sun disc.
 
NOAA 11155The bipolar one-day pores were noticed at the middle latitudes of the Northern hemisphere on 9.02, neighboring the central meridian.
 
NOAA 11156The recurrent sunspots were observed at the middle latitudes of the Southern hemisphere since 9.02 to 15.02.
 
NOAA 11157The fine bipolar sunspots crossed the Sun disc since 9.02 to 15.02 along the high latitudes of the Northern hemisphere.
 
NOAA 11158The growing multipolar group was appeared at the 20th parallel of the Southern hemisphere on 12.02, neighboring the central meridian. The new group consisted of three parts with developed sunspots and penumbraes. The head sunspots had a stable symmetrical penumbra. In the evolution peak the total region's area exceeded 600 m.h.s., and in the group it was counted more thirty sunspots. On 21.02 the multipole reached the Western limb.
 
NOAA 11159The short-time pores were noticed at the high latitudes of the Northern hemisphere since 13.02 to 16.02, to the West from the central meridian.
 
NOAA 11161The noticeable bipolar group crossed the Sun disc since 15.02 to 25.02 along the tenth parallel of the Northern hemisphere. In the evolution peak the total region's area reached 250 m.h.s., in the group it was counted forty sunspots about.
 
NOAA 11162The small bipolar group was observed at the middle latitudes of the Northern hemisphere since 19.02 to 25.02.
 
NOAA 11163The middle latitude pores were observed since 25.02 to 2.03 in the Northern hemisphere, in the Eastern part of the Sun disc.
 
NOAA 11164The large multipolar group crossed the Sun disc since 26.02 to 9.03 along the high latitudes of the Northern hemisphere. Main sunspots of the multipole formed triangle with a right angle in the South-Western direction. Between the main sunspots it was observed numerous pores and small spots. The magnetic design of the group underwent continuous changes. Before the Western limb the multipole took a freakish form of a huge butterfly. In the evolution peak the total region's area exceeded 750 m.h.s., and in the group it was counted forty sunspots about.
 
NOAA 11165The small bipolar sunspots crossed the Sun disc since 27.02 to 8.03 along the high latitudes of the Southern hemisphere. Before the Western limb the group had unexpected development.
 
NOAA 11166The big bipolar group crossed the Sun disc since 3.03 to 15.03 along the tenth parallel of the Northern hemisphere. The head sunspot had a stable symmetrical penumbra, and the bipole had an arrow-shaped form. In the evolution peak the total region's area reached 750 m.h.s., and in the group it was counted fifty sunspots about.
 
NOAA 11167The recurrent bipolar pores were observed at the middle latitudes of the Northern hemisphere since 4.03 to 11.03.
 
NOAA 11168The high latitude fine sunspots were noticed in the Northern hemisphere on 5.03 and 6.03, near the Western limb.
 
NOAA 11169The noticeable bipolar group crossed the Sun disc since 7.03 to 17.03 along the 20th parallel of the Northern hemisphere. The bipole consisted of several clusters of small sunspots which were rearranged relatively each other. Head sunspots were gradually increased, other parts of the group broke up. Before the western limb the total area of the head sunspots exceeded 300 m.h.s., and neighboring the central meridian in the group it was counted more twenty sunspots.
 
NOAA 11170The high latitude bipolar pores were noticed in the Western hemisphere on 9.03 and 10.03, near the Western limb.
 
NOAA 11172The middle latitude pores were marked in the Northern hemisphere since 12.03 to 17.03.
 
NOAA 11173The fine bipolar sunspots were noticed at the 30th parallel of the Southern hemisphere since 17.03 to 20.03.
 
NOAA 11174The recurrent pores were marked at the high latitudes of the Northern hemisphere since 18.03 to 22.03, in the Western part of the Sun disc.
 
NOAA 11175The small bipolar group was observed at the middle latitudes of the Northern hemisphere since 19.03 to 24.03, in the Western part of the Sun disc.
 
NOAA 11176The big bipolar group crossed the Sun disc since 22.03 to 3.04 along the middle latitudes of the Southern hemisphere. The bipole consisted of the head sunspot with a stable penumbra and the tail sunspots with a oblong penumbra which had separated from each other. In the evolution process intermediate sunspots disappeared, and in the tail part there was one sunspot with a penumbra. In the evolution's peak the total region's area exceeded 400 m.h.s., and in the group it was counted thirty sunspots about.
 
NOAA 11177The fine bipolar sunspots crossed the Sun disc since 24.03 to 30.03 alomg the 20th parallel of the Northern hemisphere.
 
NOAA 11178The fine bipolar sunspots crossed the Sun disc since 25.03 to 1.04 alomg the 15th parallel of the Southern hemisphere.
 
NOAA 11179The bipolar pores were noticed at the low latitudes of the Northern hemisphere since 25.03 to 28.03, near the Western limb.
 
NOAA 11180The fine sunspot with a symmetrical penumbra crossed the Sun disc since 26.03 to 5.04 along the 25th parallel of the Northern hemisphere.
 
NOAA 11181The fine sunspot crossed the Sun disc since 26.03 to 1.04 along the 25th parallel of the Southern hemisphere.
 
NOAA 11182The short-time pore was noticed on 28.03 to the South from the region 11177.
 
NOAA 11183The noteciable bipolar group crossed the Sun disc since 28.03 to 7.04 along the 15th parallel of the Northern hemisphere. A spot which was situated in the middle part of the group was gradually approached and merge with the head sunspot. Tail sunspots formated a triangle configuration, then its desintegrated. In the evolution's peak the total region's area exceeded 300 m.h.s., and in the group it was counted not over twenty sunspots.
 
NOAA 11184The small bipolar group was observed at the 15th parallel of the Northern hemisphere since 2.04 to 10.04. Before the Western limb its tail part had collapsed.
 
NOAA 11185The fine bipolar sunspots were slowly drifting from the high latitudes of the Northern hemisphere to the Sun equator since 5.04 to 15.04.
 
NOAA 11186The fine bipolar sunspots crossed the Sun disc along the 23rd parallel of the Northern hemisphere since 6.04 to 16.04.
 
NOAA 11187The undistinguished sunspots were observed at the high latitudes of the Southern hemisphere since 8.04 to 15.04.
 
NOAA 11188The short-time sunspots were noticed at the high latitides of the Southern hemisphere on 9.04 and 10.04, to the West from the central meridian.
 
NOAA 11189The short-time sunspots were noticed at the high latitudes of the Northern hemisphere on 9.04 and 10.04, to the West from the central meridian.
 
NOAA 11190The fast-growing group was observed at the middle latitudes of the Northern hemisphere since 12.04 to 19.04, in the Western part of the Sun disc. The multipole appeared neighboring the central meridian and consisted of three sunspot's clusters. Head and intermediate parts of the group united subsequently and continued growth. Tail sunspots had no development and turned in disintegration. In the evolution peak the total region's area exceeded 400 m.h.s., and in the group it was counted more thirty sunspots.
 
NOAA 11191The fine sunspot with a symmetrical penumbra crossed the Sun disc along the low latitdes of the Northern hemisphere since 13.04 to 24.04. Time to time there were pores with an opposite magnetic polarity neighboring the sunspot.
 
NOAA 11192The low latitude pores were marked in the Northern hemisphere since 13.04 to 17.04, in the Western part of the Sun disc.
 
NOAA 11193The noticeable bipolar group crossed the Sun disc since 14.04 to 26.04 along the middle latitudes of the Northern hemisphere. The head sunspot had a stable symmetrical penumbra. Neighboring the central meridian the total region's area reached 400 m.h.s., and in the group it was counted twenty sunspots about.
 
NOAA 11194The high latitude pores were noticed in the Southern hemisphere since 15.04 to 17.04, not far from the Western limb.
 
NOAA 11195The noteciable bipolar group crossed the Sun disc since 20.04 to 1.05 along the middle latitudes of the Southern hemisphere. In first days the group consisted of three parts. Intermediate sunspots disappeared, and head and tail sunspots continued the growth. Over time the tail part was scattered, and the head sunspot got a symmetrical form. Time to time the total region's area reached 400 m.h.s.
 
NOAA 11196The fine bipolar group was marked at the high latitudes of the Southern hemisphere since 21.04 to 27.04.
 
NOAA 11197The one day pore was observed on 22.04 at the middle latitudes of the Southern hemisphere, in the Eastern part of the Sun disc.
 
NOAA 11198The bipolar pores were marked at the 25th parallel of the Southern hemisphere on 22.04 and 23.04, not far from the Western limb.
 
NOAA 11199The new bipolar group was developing at the 21st parallel of the Northern hemisphere since 27.04 to 2.05, in the Western part of the Sun disc. Before the Western limb the total region's area reached 200 m.h.s.
 












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