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Дата изменения: Wed Feb 3 21:01:15 2016
Дата индексирования: Sun Apr 10 02:17:49 2016
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Поисковые слова: solar eclipse
The Sunspot Observer - The <b style="color:black;background-color:#ffff66">solar</b> regions - The description of the <b style="color:black;background-color:#ffff66">solar</b> regions

Statistics of sunspot activity

NOAA 11300 - NOAA 11399
The description of the solar regions

NOAA 11300The small bipolar group was noticed at the 24th parallel of the Northern hemisphere since 18.09 to 22.09 near the Western limb. The head sunspot had a symmetrycal penumbra.
 
NOAA 11301The extended chain of small spots crossed the Sun disc since 18.09 to 1.10 along the middle latitudes of the Northern hemisphere.
 
NOAA 11302The big multipolar group crossed the Sun disc since 22.09 to 5.10 along the middle latitudes of the Northern hemisphere. The multipole consisted of big head sunspots with a large extended penumbra, tail sunspots with a common big penumbra and developed sunspots since a common penumbra in a middle part of the group which were gradually merging the head sunspots. As approaching the Western limb the head group's part had again forked and the tail sunspots had gradually decayed. Neighboring the central meridian the total region's area exceeded 1000 m.h.s., it was counted about forty sunspots in the group.
 
NOAA 11303The fast-growing bipolar group was marked at the 28th parallel of the Southern hemisphere since 24.09 to 26.09 near the Western limb.
 
NOAA 11304The fine bipolar sunspots were observed at the middle latitudes of the Northern hemisphere since 24.09 to 30.09 to the West from the central meridian.
 
NOAA 11305The stable sunspot with a symmetrycal penumbra crossed the Sun disc since 25.09 to 7.10 along the 12th parallel of the Northern hemisphere. Pores and fine sunspots were observed neighboring the sunspot. Before the Western limb the sunspot began grow, the total region's area reached 250 m.h.s.
 
NOAA 11306The fine sunspot with a symmetrycal penumbra crossed the Sun disc since 26.09 to 8.10 along the middle latitudes of the Northern hemisphere.
 
NOAA 11307The fine bipolar sunspots were observed since 28.09 to 6.10 at the middle latitudes of the Northern hemisphere.
 
NOAA 11308The fine sunspot with a penumbra was noticed at the 25th parallel of the Southern hemisphere since 1.10 to 3.10 in the Eastern part of the Sun disc.
 
NOAA 11309The small bipolar group crossed the Sun disc since 2.10 to 14.10 along the high latitudes of the Northern hemisphere. The head sunspot had a noticeable symmetrycal penumbra.
 
NOAA 11310The fine bipolar sunspots were marked at the 33rd parallel of the Southern hemisphere since 3.10 to 10.10 in the Western part of the Sun disc.
 
NOAA 11311The small bipolar sunspots were observed at the 11th parallel of the Southern hemisphere since 4.10 to 12.10 in the Western part of the Sun disc. The head sunspot had a stable symmetrycal penumbra.
 
NOAA 11312The noticeable sunspot with a stable symmetrycal penumbra crossed the Sun disc since 4.10 to 17.10 along the 22nd parallel of the Northern hemisphere. Time to time the sunspot's area exceeded 250 m.h.s.
 
NOAA 11313The small bipolar group crossed the Sun disc since 5.10 to 17.10 along the 15th parallel of the Southern hemisphere.
 
NOAA 11314The big sunspot with a stable symmetrycal penumbra crossed the Sun disc since 9.10 to 22.10 along the 27th parallel of the Northern hemisphere. Time to time the total region's area reached 300 m.h.s., and pores and fine sunspots of an opposite magnetic polarity appeared neighboring the sunspot.
 
NOAA 11315The fine bipolar sunspots were noticed since 10.10 to 15.10 to the East from the region 11312.
 
NOAA 11316The big bipolar group crossed the Sun disc since 11.10 to 22.10 along the 12th parallel of the Southern hemisphere. The head sunspot had a developed symmertycal penumbra which was gradually extended lengthways a parallel owing to umbra's bifurcation. The tail group's part consisted of three umbraes with a common triangle penumbra. Then this construction was scattered on spots with separated penumbraes. Neighboring the central meridian the total bipole's area had exceeded 300 m.h.s. As approaching the Western limb the group's sunspots were gradually decreased.
 
NOAA 11317The small sunspot with a stable symmetrycal penumbra crossed the Sun disc since 11.10 to 23.10 along the 26th parallel of the Southern hemisphere.
 
NOAA 11318The fine bipolar sunspots were noticed since 12.10 to 19.10 to the East from the region 11318.
 
NOAA 11319The growing sunspot's shain was observed since 12.10 to 22.10 at the tenth parallel of the Northern hemisphere. In the evolution's peak the total bipole's area reached 400 m.h.s., and in the group it was counted more thirty sunspots.
 
NOAA 11320The fine sunspots were noticed to the South from the region 11313 since 13.10 to 17.10.
 
NOAA 11321The fine sunspots were marked at the middle latitudes of the Southern hemisphere since 15.10 to 22.10.
 
NOAA 11322The fine bipolar sunspots were observed at the 27th parallel of the Southern hemisphere since 15.10 to 18.10, not far from the Western limb.
 
NOAA 11323The recurrent sunspots were observed at the high latitudes of the Northern hemisphere since 17.10 to 23.10.
 
NOAA 11324The big bipolar group crossed the Sun disc since 17.10 to 31.10 along 12th parallel of the Northern hemisphere. The multipole represented a solid chain of small sunspots with developed penumbraes. As approaching the central meridian this construction began collapse, and few sunspot reached the Western limb. In the evolution's peak the total region's area exceeded 350 m.h.s., and it was counted about thirty sunspots in the group.
 
NOAA 11325The collapsing bipolar group was observed since 20.10 to 20.10 at the middle latitudes of the Northern hemisphere. In the first days the head bipole's part consisted of two closer sunspots with symmetrycal penumbraes. Then the spots began disperse from each other and decrease in sizes. The maximal total region's area exceeded 250 m.h.s.
 
NOAA 11326The undistinguished bipolar sunspots were observed at the middle latitudes of tne Northern hemisphere since 20.10 to 22.10, not far from the Western limb.
 
NOAA 11327The small bipolar group was marked at the high latitudes of the Southern hemisphere since 20.10 to 28.10, in the Western part of the Sun disc. The tail sunspot had a stable penumbra. Time to time the total bipole's area reached 200 m.h.s.
 
NOAA 11328The short-time bipolar sunspots were noticed at the middle latitudes of the Northern hemisphere since 20.10 to 23.10, neighboring the central meridian.
 
NOAA 11329The fine sunspots were marked at the thirty parallel of the Southern hemisphere since 21.10 to 23.10, not far from the Western limb.
 
NOAA 11330The opened bipolar group crossed the Sun disc since 22.10 to 4.11 along the low latitudes of the Northern hemisphere. The head sunspot represented a big umbra with a stable penumbra. In the first days the tail saunspots had a common curved penumbra, then this group's part returned in slow desintegration. Neighboring the central meridian the total bipole's area reached 500 m.h.s., and it was counted ten-twenty sunspots in the group.
 
NOAA 11331The fine bipolar sunspots were marked at the tenth parallel of the Northern hemisphere since 23.10 to 26.10 near the Western limb.
 
NOAA 11332The fine sunspot with a symmetrycal penumbra crossed the Sun disc since 24.10 to 4.11 along the 31st parallel of the Northern hemisphere.
 
NOAA 11333The fine bipolar sunspots were observed since 27.10 to 3.11 to the North from the tail part of the group 11330.
 
NOAA 11334The fine bipolar group was marked at the 12th parallel of the Northern hemisphere since 30.10 to 8.11, in the Western part of the Sun disc.
 
NOAA 11335The bipolar pores were observed since 31.10 to 4.11 to the North from the group 11335.
 
NOAA 11336The recurrent sunspots were noticed at the middle latitudes of the Northern hemisphere since 31.10 to 10.11.
 
NOAA 11337The recurrent sunspots were marked since 31.10 to 9.11 to the North-East from the sunspots 11336.
 
NOAA 11338The opened bipolar group crossed the Sun disc since 1.11 to 13.11 along the middle latitudes of the Southern hemisphere. The head and tail sunspots had stable symmetrycal penumbraes. The group's axis had a considerable inclination to the parallel. The total bipole's area exceeded 200 m.h.s.
 
NOAA 11339The big multipolar group crossed the Sun disc since 2.11 to 15.11 along the 20th parallel of the Northern hemisphere. The head sunspot had a large stable penumbra and the group had a closed configuration. Time to time the total region's area 1500 m.h.s. and it was to fifty sunspots in the group.
 
NOAA 11340The small sunspot with a symmetrycal penumbra crossed the Sun disc since 5.11 to 17.11 along the tenth parallel of the Southern hemisphere.
 
NOAA 11341The small bipolar group crossed the Sun disc since 5.11 to 18.11 along the tenth parallel of the Northern hemisphere. The head sunspot had a stable symmetrycal penumbra and the tail group's part consisted of recurrent sunspots.
 
NOAA 11342The opened bipolar group was observed since 5.11 to 18.11 to the North-West from the group 11341. The head sunspot had a stable symmetrycal penumbra and the tail group's part consisted of recurrent sunspots. Time to time the total bipole's area reached 300 m.h.s.
 
NOAA 11343The small sunspot with a stable symmetrycal penumbra crossed the Sun disc since 6.11 to 19.11 along the 27th parallel of the Northern hemisphere.
 
NOAA 11344The growing bipolar group was observed at the 20th parallel of the Southern hemishere since 7.11 to 15.11 in the Western part of the Sun disc. Before the Western limb the total bipole's area reached 200 m.h.s.
 
NOAA 11345The fine bipolar sunspots were marked since 9.11 to 15.11 to the South-East from the group 11344.
 
NOAA 11346The fine bipolar group crossed the Sun disc since 12.11 to 24.11 along the middle latitudes of the Southern hemisphere. The head sunspot had a stable symmetrycal penumbra.
 
NOAA 11347The fine sunspots were noticed since 13.11 to 20.11 at the low latitudes of the Northern hemisphere.
 
NOAA 11348The small bipolar sunspots were noticed at the 20th parallel of the Northern hemisphere since 14.11 to 16.11, near the Western limb.
 
NOAA 11349The bipolar pores were observed at the middle latitudes of the Northern hemisphere since 14.11 to 20.11, in the Western part of the Sun disc.
 
NOAA 11350The small bipolar group was marked at the 26th parallel of the Northern hemisphere since 14.11 to 20.11.
 
NOAA 11351The recurrent sunspots were noticed since 14.11 to 20.11 to the South-East from the region 11346.
 
NOAA 11352The small bipolar group crossed the Sun disc since 16.11 to 28.11 along the high latitudes of the Southern hemisphere. The head sunspot had a stable symmetrycal penumbra. The tail pores were gradually collapsed.
 
NOAA 11353The fine sunspot with an unstable symmetrycal penumbra was observed since 17.11 to 28.11 at the low latitudes of the Northern hemisphere. Time to time pores of an opposite magnetic polarity appeared neighboring the sunspot.
 
NOAA 11354The small bipolar group crossed the Sun disc since 17.11 to 27.11 along the middle latitudes of the Southern hemisphere. In the first days the bipole presented as a rhombus made from small sunspots with developed penumbraes, the total area reached 200 m.h.s. The group was slowly collapsing.
 
NOAA 11355The small stable sunspot with a symmetrycal penumbra crossed the Sun disc since 18.11 to 1.12 along the 14th parallel of the Northern hemisphere. Time to time pores and fine sunspots appeared neighboring the sunspot.
 
NOAA 11356The big bipolar group crossed the Sun disc since 19.11 to 2.12 along the middle latitudes of the Northern hemisphere. The head and the tail sunspots had stable symmetrycal penumbraes. The tail sunspot was gradually bifurcaing. In the evolution's peak the total bipole's area reached 400 m.h.s.
 
NOAA 11357The growing bipolar group was marked at the 17th parallel of the Northern hemisphere since 20.11 to 26.11, in the Western part of the Sun disc.
 
NOAA 11358The small bipolar group crossed the Sun disc since 22.11 to 5.12 along the 20th parallel of the Northern hemisphere. The head sunspot had a stable symmetrycal penumbra. The tail sunspots were gradually collapsing.
 
NOAA 11359The fine bipolar sunspots were noticed at the middle latitudes of the Northern hemisphere since 24.11 to 27.11, near the Western limb.
 
NOAA 11360The fine bipolar sunspots were noticed since 25.11 to 29.11 to the East from the region 11356.
 
NOAA 11361The small bipolar group crossed the Sun disc since 25.11 to 7.12 along 19th parallel of the Northern hemisphere.
 
NOAA 11362The opened bipolar group crossed the Sun disc since 27.11 to 10.12 along the low latitudes of the Northern hemisphere. The head and the tail sunspots had stable symmetrycal penumbraes. The head sunspot was gradually bifurcating.
 
NOAA 11363The big bipolar group crossed the Sun disc since 29.11 to 10.12 along the 20th parallel of the Southern hemisphere. The isolated sunspot with a stable symmetrycal penumbra was feature of the group which was situated to the North from the head group's part. This sunspot was gradually decreasing. The head group's part consisted of two closely located sunspot with a common oblong penumbra. The tail sunspots were gradually collapsing. Neighboring the central meridian the total region's area reached 600 m.h.s., and it was counted more thirty sunspots in the group.
 
NOAA 11364The small sunspot with a stable symmetrycal penumbra crossed the Sun disc since 29.11 to 11.12 along the 18th parallel of the Northern hemisphere. Time to time pores and fine sunspots of an opposite magnetic polarity appeared neighboring the sunspot.
 
NOAA 11365The fine bipolar sunspots were marked since 2.12 to 9.12 to the North from the group 11362.
 
NOAA 11366The fine sunspots crossed the Sun disc since 3.12 to 14.12 along the 18th parallel of the Northern hemisphere. The main sunspot had a stable symmetrycal penumbra.
 
NOAA 11367The fine bipolar sunspots crossed the Sun disc since 4.12 to 13.12 along the 18th parallel of the Southern hemisphere.
 
NOAA 11368The short-time bipolar sunspots were noticed at the middle latitudes of the Southern hemisphere since 5.12 to 7.12, in the Eastern part of the Sun disc.
 
NOAA 11369The short-time bipolar sunspots were noticed 6.12 and 7.12 to the North-East from the group 11366.
 
NOAA 11370The bipolar one-day pores were notiiced 8.12 to the North from the sunspots 11367.
 
NOAA 11371The fine one-day sunspot was marked 8.12 in the center of the Sun disc.
 
NOAA 11372The fine bipolar sunspots were observed since 7.12 to 14.12 at the low latitudes of the Northern hemisphere.
 
NOAA 11373The short-time bipolar sunspots were noticed at the 30th parallel of the Southern hemisphere since 8.12 to 10.12, in the Western part of the Sun disc.
 
NOAA 11374The double sunspot with common penumbra crossed the Sun disc since 8.12 to 20.12 along the middle latitudes of the Southern hemisphere. Neighboring the central meridian the total bipole's area reached 200 m.h.s.
 
NOAA 11375The small sunspots crossed the Sun disc since 8.12 to 20.12 along the eighth parallel of the Northern hemisphere. In the first days the group had a bipolar configuration. The head sunspot had a stable symmetrycal penumbra. The tail pores had quickly collapsed.
 
NOAA 11376The recurrent sunspots were observed since 13.12 to 24.12 at the 20th parallel of the Northern hemisphere.
 
NOAA 11377The fine bipolar sunspots were marked since 13.12 to 21.12 at the 12th parallel of the Northern hemisphere.
 
NOAA 11378The short-time sunspots were noticed at the 17th parallel of the Southern hemisphere on 17.12 and 18.12, in the Western part of the Sun disc.
 
NOAA 11379The short-time sunspots were noticed at the 29th parallel of the Southern hemisphere since 17.12 to 20.12, in the Western part of the Sun disc.
 
NOAA 11380The recurrent sunspots were observed since 17.12 to 28.12 at the 20th parallel of the Southern hemisphere.
 
NOAA 11381The fine bipolar sunspots were marked since 18.12 to 27.12 at the middle latitudes of the Southern hemisphere.
 
NOAA 11382The small bipolar group was observed since 18.12 to 27.12 to the East from the group 11381. The head sunspot had a stable penumbra, and tail sunspots were gradually collapsing.
 
NOAA 11383The fine sunspots were observed at the Sun equator since 19.12 to 30.12.
 
NOAA 11384The opened bipolar group crossed the Sun disc since 20.12 to 31.12 along the middle latitudes of the Northern hemisphere. The bipole consisted of a large head sunspot with a penumbra and fine tail sunspots which were gradually collapsing. Neighboring the central meridian the total region's area reached 500 m.h.s.
 
NOAA 11385The fine bipolar sunspots were noticed at the 32nd parallel of the Southern hemisphere since 23.12 to 28.12, in the Western part of the Sun disc.
 
NOAA 11386The small bipolar group crossed the Sun disc since 23.12.11 to 5.01.12 along the 18th parallel of the Southern hemisphere. The bipole changed a configuration, but the sunspot in the middle group's part had a stable penumbra. Neighboring the central meridian the total region's area reached 200 m.h.s.
 
NOAA 11387The growing bipolar group was observed at the 20th parallel of the Southern hemisphere since 25.12 to 30.12, in the Western part of the Sun disc. Before the Western part the total bipole's area had reached 300 m.h.s.
 
NOAA 11388The single sunspot with a symmetrycal penumbra crossed the Sun disc since 27.12.2011 to 9.01.2012 along 24th parallel of the Southern hemisphere.
 
NOAA 11389The big bipolar group crossed the Sun disc since 28.12 to 10.01 along the 23rd parallel of the Southern hemisphere. The head sunspot had a large penumbra, and the group's axis had considerable inclination to a parallel. Tail sunspots were gradually collapsing. In the evolution's peak the total region area reached 500 m.h.s.
 
NOAA 11390The fine bipolar sunspots were marked since 28.12 to 7.01 at the tenth parallel of the Northern hemisphere.
 
NOAA 11391The noteciable bipolar group crossed the Sun disc since 2.01.12 to 15.01.12 along the 13th parallel of the Northern hemisphere. The head sunspot had a large penumbra, and the tail group's part consisted of fine sunspots. The maximal bipole's area reached 500 m.h.s.
 
NOAA 11392The fine bipolar sunspots were marked at the 20th parallel of the Northern hemisphere since 3.01 to 10.01, in the Western part of the Sun disc.
 
NOAA 11393The growing bipolar group was observed at the midlle latitudes of the Northern hemisphere since 5.01 to 12.01, in the Western part of the Sun disc. Before the Western limb the total region's area exceeded 500 m.h.s.
 
NOAA 11394The short-time pores were noticed at the 18th parallel of the Northern hemisphere since 6.01 to 8.01, to the East from the central meridian.
 
NOAA 11395The fine sunspot with a symmetrycal penumbra was observed since 8.01 to 17.01 at the 21st parallel of the Northern hemisphere.
 
NOAA 11396The fine bipolar sunspots were marked since 12.01 to 19.01 at the high latitudes of the Northern hemisphere.
 
NOAA 11397The short-time bipolar sunspots were noticed at the 20th parallel of the Southern hemisphere since 13.01 to 16.01, neighboring the central meridian.
 
NOAA 11398The fine bipolar sunspots were marked since 13.01 to 19.01 to the South-West from the group 11399.
 
NOAA 11399The fine sunspots were observed at the high latitudes of the Southern hemisphere since 14.01 to 20.01, in the Eastern part of the Sun disc.
 












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