Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.alexeyryback.ru/en/solar_regions/11000.htm
Дата изменения: Wed Feb 3 21:01:11 2016
Дата индексирования: Sun Apr 10 02:15:48 2016
Кодировка:
The Sunspot Observer - The solar regions - The description of the solar regions

Statistics of sunspot activity

NOAA 11000 - NOAA 11099
The description of the solar regions

NOAA 11000The short-time sunspots were fixed on 18.07 and 19.07.2008 in the central part of the Sun disc.
 
NOAA 11001The bipolar one-day pores were noticed on 12.09 in the center of the Sun disc.
 
NOAA 11002The fine bipolar sunspots were observed at the mid latuitudes of the Northern hemisphere since 22.09 to 24.09, to the West of the Sun disc.
 
NOAA 11003The high latitude one-day pore was noticed on 5.10 in the Southern hemisphere, to the East from the central meridian.
 
NOAA 11004The short-time pore was marked on 10.10 and 11.10 in the central part of the Sun disc.
 
NOAA 11005The small bipolar group crossed the Sun disc since 11.10 to 17.10 along the high latitudes of the Northern hemisphere. The head sunspot had a fine penumbra.
 
NOAA 11006The high latitude pores were noticed on 17.10 in the Southern hemisphere near the West limb.
 
NOAA 11007The small opened bipole was observed at the 35th parallel of the Northern hemisphere since 31.10 to 6.11, in the Western part of the Sun disc.
 
NOAA 11008The small bipolar group crossed the Sun disc since 11.11 to 17.11 along the 33rd parallel of the Northern hemishere. The main spots had symmetrical penumbraes.
 
NOAA 11009The high latitude bipolar group was noticed in the Southern hemisphere since 11.12 to 13.12, not far from Western limb.
 
NOAA 11010The bipolar combination of fine sunspots whish was remarking at the middle latitudes of the Northern hemisphere since 10.01 to 14.01.09.
 
NOAA 11012The short-time near equatorial pore which was noticing in the Eastern part of the Sun disc since 11.02 to 13.02.
 
NOAA 11013The high latitude bipolar sunspots which were observing in the Northern hemisphere since 24.02 to 26.02 near the central meridian.
 
NOAA 11014The short-time pores were noticing to the West from the center from the Sun disc on 6.03 and 7.03.
 
NOAA 11015The high latitude pore was remarked in the Northern hemisphere on 21.04 and 22.04 near the West limb.
 
NOAA 11016The low latitude sunspots were noticed in the Southern hemisphere on 29.04 and 30.04 near the West limb.
 
NOAA 11017The bipolar sunspot's cloud was observing at the middle latitudes of the Northern hemisphere since 13.05 to 20.05 in the West part of the Sun disc.
 
NOAA 11018The bipolar one-day pores were noticed at the high latitudes of the Southern hemisphere on 23.05 and 24.05 in the Eastern part of the Sun disc.
 
NOAA 11019The bipolar pores were observing at the high latitudes of the Northern hemisphere since 1.06 to 5.06 in Eastern part of the Sun disc.
 
NOAA 11020The bipolar pores were marking at the high latitudes of the Northern hemisphere since 9.06 to 15.06 in the Western part of the Sun disc.
 
NOAA 11021The middle latitude pore was noticed in the Southern hemisphere on 16.06 and 17.06 near the Western limb.
 
NOAA 11022The high latitude pores were observing in the Southern hemisphere since 22.06 to 28.06 in the Western part of the Sun disc.
 
NOAA 11023The fine bipolar sunspots were marking to the East from the region 11022 since 23.06 to 1.07. The head sunspot had fine symmetric penumbra.
 
NOAA 11024The small bipolar group was crossing the Sun disc since 4.07 to 11.07 along the high latitudes of the Southern hemisphere. The head sunspot had fine symmetric penumbra, and tail sunspots had undeveloped structure. There were pores appeared and disappeared between the main sunspots. In the peak of activity it was counted 10-15 sunspots in the group, and the total region area reached 200 m.h.s.
 
NOAA 11025The phantom pores were marking at the middle latitudes of the Northern hemisphere since 1.09 to 10.09.
 
NOAA 11026The delaying sunspot with symmetrical penumbra was crossing the Sun disc along the highest latitudes of the Southern hemisphere since 22.09 to 30.09.
 
NOAA 11027The fine bipolar group of sunspots with undeveloped penumbraes and an open configuration was crossing the Sun disc along the high latitudes of the Northern hemisphere since 23.09 to 1.10.
 
NOAA 11028The phantom pores were marking at the high latitudes of the Northern hemisphere since 21.10 to 2.11.
 
NOAA 11029The erruptive bipolar structure was arisen on 24.10 to the South from the region 11028. In the peak of activity in the group it was counted twenty sunspots almost, and the total region area exseeded 150 m.h.s.
 
NOAA 11030The high latitude pores were marking since 6.11 to 13.11 in the Western part of the Northern hemisphere.
 
NOAA 11031The phantom pores were noticing at the high latitudes of tne Northern hemisphere since 16.11 to 24.11 in the Western part of the Sun disc.
 
NOAA 11032The phantom pores were noticing at the middle latitudes of tne Northern hemisphere since 19.11 to 28.11 in the Western part of the Sun disc.
NOAA 11033The bipolar pores were following behind the region 11032 since 19.11 to 30.11.
 
NOAA 11034The bipolar pores were crossing the Sun disc along the middle latitudes of the Northern hemisphere since 10.12 to 21.12.
 
NOAA 11035The high latitude erruptive structure had arisen 15.12 to the North from the region 11034. In the peak of activity the group reached closed configuration, it was counted twenty sunspots almost, and the total region area exceeded 200 m.h.s.
 
NOAA 11036The small bipolar sunspots were observing at the high latitudes of the Southern hemisphere since 20.12 to 25.12 in ther Western part of the Sun disc. Time to time main sunspots had fine symmetrical penumbraes.
 
NOAA 11037The phantom pores were crossing the Sun disc along the middle latitudes of the Northern hemisphere since 20.12 to 30.12.
 
NOAA 11038The fine sunspots were noticing at the middle latitudes of the Northern hemisphere since 21.12 to 25.12 not far from the Western limb.
 
NOAA 11039The small bipolar group was crossing the Sun disc along the high latitudes of the Southern hemisphere since 27.12.09 to 6.01.10. The group had an open structure, and main sunspots had fine penumbraes.
 
NOAA 11040The one of the power events for new cycle. On 8.01 there were bipolar pores had arisen at the high latitudes of the Northern hemisphere, not far from the Eastern limb. In next days the group developed to the large bipole with solid head and tail sunspots. Neighboring the central meridian it was counted 25 sunspots in the group, and the total region area exceeded 300 m.h.s. On 18.01 the group had come to the Western limb turning slow dacay.
 
NOAA 11041The simple bipolar group had arisen on 20.01 in the opposite area of the Sun disc than the region 11040. The bipole consisted of an head sunspot with stable penumbra and small tail sunspots. After crossing the central meridian the head sunspot assumed symmetrical form turning to slow decay.
 
NOAA 11042The small bipole had marking at the high latitudes of the Northern hemisphere since 22.01 to 27.01 in the Western part of the Sun disc.
 
NOAA 11043The small sunspot was observed at the 25th parallel of the Northern hemisphere since 01.02 to 07.02. Time to time there were tail pores of the opposite magnetic polarity.
 
NOAA 11044The single pore was noticed 06.02 in the Northern hemisphere, not far the Western limb.
 
NOAA 11045The long sunspot chain was gradually disintegrated at the high latitudes of the Northern hemisphere since 07.02 to 14.02, to the West from the central meridian. In the evolution peak it was more 30 sunspots in the group, and the total region area was exceeded 400 m.h.s.
 
NOAA 11046The high-growth bipolar sunspots was crossing the sunspot disc since 8.02 to 18.02 along high latitudes of the Northern hemisphere. The group consisted of a small head sunspot and small tail sunspot cluster. Neighboring the central meridian it was counted more twenty small sunspots and total region area reached 200 m.h.s.
 
NOAA 11047The single pore was noticed at the middle latitudes of the Southern hemisphere since 8.02 to 10.02, to the East from the central meridian.
 
NOAA 11048The small pores were noticed at the middle latitudes of the Northern hemisphere since 14.02 to 17.02 to the East from the central meridian.
 
NOAA 11049The small bipolar sunspots were observed at the middle latitudes of the Southern hemisphere since 17.02 to 23.02 to the West from the central meridian.
 
NOAA 11050The small pores were noticed at the middle latitudes of the Southern hemisphere since 23.02 to 28.02 to the West from the central meridian.
 
NOAA 11051The small sunspot with symmetrical penumbra crossed the Sun disc since 24.02 to 5.03 across middle latitudes. Time to time tail sunspots were observed.
 
NOAA 11052The bipolar pores were noticed at the middle latitudes of the Southern hemisphere since 2.03 to 5.03, not far from the West limb.
 
NOAA 11053The bipolar pores were noticed at the high latitudes of the Southern hemisphere since 2.03 to 5.03, not far from the West limb.
 
NOAA 11054The noticeable bipolar group crossed the Sun disc since 10.03 to 20.03 along the middle latitudes of the Northern hemisphere. The head group's part consisted of several small sunspots interspersed in assymmetrical penumbra which was gradually breaking up. Tail sunspots had small sunpots, its were quickly disintegrated. Neighboring the central meridian the total region area exceeded 200 m.h.s., it counts more 20 sunspots in group.
 
NOAA 11055The short-time bipolar sunspots were noticed at the high latitudes of the Southern hemisphere since 12.03 to 13.03 to the West from the central meridian.
 
NOAA 11056The bipolar pores crossed the Sun disc since 17.03 to 23.03 along the middle latitudes of the Northern hemisphere.
 
NOAA 11057The noticeable bipolar group crossed the Sun disc since 23.03 to 3.04 along the middle latitudes of the Northern hemisphere. The bipole consisted of a head sunspot with small symmetrical penumbra and a tail sunspot with big symmetrical penumbra. The head sunspot was gradually shattered and disappeared. The tail sunspot had lost symmetry and than it was scattered on smaller sunspots. Neighboring the central meridian the total region area reached 400 m.h.s., it was counted ten sunspots in the group.
 
NOAA 11058The short-time pore was noticed at the high latitudes of the Northern hemisphere 26.03 and 27.03 to the West from central meridian.
 
NOAA 11059The small sunspot with penumbra crossed the Sun disc since 27.03 to 6.04 along the high latitudes of the Southern hemisphere. Time to time there were pores neighboring the sunspot./TR>
 
NOAA 11060The small sunspots were observed since 4.04 to 8.04 at the high latitudes of the Northern hemisphere.
 
NOAA 11061The open bipolar group was observed at the middle latitudes of the Northern hemisphere since 06.04 to 10.04, to the West from the central meridian. The head sunspot had symmetrical penumbra.
 
NOAA 11062The short-time bipolar pores were noticed at the middle latitudes of the Southern hemisphere since 13.04 to 15.04 to the West from the central meridian.
 
NOAA 11063The recurrent pores were noticed at the middle latitudes of the Northern hemisphere since 29.04 to 05.05 to the West from the central meridian.
 
NOAA 11064The recurrent pores crossed the Sun disc since 01.05 to 10.05 along the middle latitudes of the Northern hemisphere.
 
NOAA 11065The recurrent pores were noticed at the high latitudes of the Southern hemisphere since 02.05 to 09.05 to the West from the central meridian.
 
NOAA 11066The recurrent pores were noticed at the high latitudes of the Southern hemisphere since 02.05 to 10.05.
 
NOAA 11067The recurrent pores crossed the Sun disc along the high latitudes of the Northern hemisphere since 03.05 to 13.05.
 
NOAA 11068The recurrent pores crossed the Sun disc along the high latitudes of the Southern hemisphere since 03.05 to 16.05.
 
NOAA 11069The small bipolar sunspots were observed at the 42nd parallel of tne Northern hemisphere since 05.05 to 09.05, not far from the Western limb.
 
NOAA 11070The recurrent pores were noticed at the high latitudes of the Northern hemisphere since 05.05 to 11.05 to the West from the central meridian.
 
NOAA 11071The one-day pore was noticed on 9.05 at the 20th parallel of the Southern hemisphere to the West from the central meridian.
 
NOAA 11072The small bipolar group had appeared on 21.05 at the middle latitudes of the Southern hemisphere to the East from the central meridian. The head sunspot had a small symmetrical penumbra and the tail sunspots were gradually disappeared. On 28.05 the leading sunspot had reached the Western limb.
 
NOAA 11073The law latitude bipolar pores were noticed in the Northern hemisphere since 30.05 to 1.06 to the East from the central meridian.
 
NOAA 11074The law latitude pores were observed in the Northern hemisphere on 30.05 and 31.05 near the Western llimb.
 
NOAA 11075The short-time pores were noticed at the 20th parallel of the Southern hemisphere since 30.05 to 1.06 to the West from the central meridian.
 
NOAA 11076The small bipolar group had appeared on 1.06 at the 20th parallel of the Southern hemisphere neighboring the central meridian. The main sunspots had small penumbraes. On 6.06 the bipole had reached the Western limb.
 
NOAA 11077The one-day pore was noticed on 6.06 at the 20th of the Northern hemisphere not far from the Western limb.
 
NOAA 11078The growing bipolar group was observed since 9.06 to 11.06 at the high latitudes of the Southern hemisphere near the Western limb.
 
NOAA 11079The high latitudes pores were noticed in the Southern hemisphere on 10.06 and 11.06 not far from the Western limb.
 
NOAA 11080The small bipolar group was observed at the high latitudes of the Southern hemisphere since 11.06 to 13.06 near the Western limb.
 
NOAA 11081The small bipolar sunspots were noticed at the high latitudes of the Northern hemisphere since 12.06 to 14.06 not far from the Western limb.
 
NOAA 11082The small bipolar sunspots crossed the Sun disc since 17.06 to 25.06 along 28th parallel of the Northern hemisphere.
 
NOAA 11083The bipolar one day pores were noticed on 20.06 at the high latitudes of the Northern hemisphere to the West from the central meridian.
 
NOAA 11084The small sunspots with symmetrical penumbra crossed the Sun disc since 28.06 to 8.07 along the 20th parallel of the Southern hemisphere.
 
NOAA 11085The short-time bipolar sunspots were noticed on 30.06 at the 23rd parallel of the Southern hemisphere to the West from the central meridian.
 
NOAA 11086The bipolar pores were noticed at the middle latitudes of the Northern hemisphere since 6.07 to 8.07 near the Western limb.
 
NOAA 11087The small bipolar group crossed the Sun disc since 10.07 to 21.07 along the 20th parallel of the Northern hemisphere. The head sunspot had a stable penumbra.
 
NOAA 11088The high latitude oneday sunspot was noticed in the Southern hemisphere on 14.07 and 15.07 neighboring the central meridian.
 
NOAA 11089The noticeable bipolar group crossed the Sun disc since 20.07 to 1.08 along the 24th parallel of the Southern hemisphere. The main sunspots had small penumbraes and combined a triangle configuration. In process of advance on the Sun disc the tail sunspot had collapsed. In the peak's evolution the total region area reached 300 m.h.s., and it counted more twenty sunspots in the group.
 
NOAA 11090The short-time pores were noticed at the high latitudes of the Northern hemisphere since 25.07 to 27.07 to the East from the central meridian.
 
NOAA 11091The high latitude pore was noticed on 27.07 at the Western limb of the Northern hemisphere.
 
NOAA 11092The noticeable sunspot with symmetrical penumbra crossed the Sun disc since 28.07 to 9.08 along the middle latitudes of the Northern hemisphere. Time to time there were pores of the opposit magnetic polarity.
 
NOAA 11093The small sunspot with symmetrical penumbra crossed the Sun disc since 3.08 to 15.08 along the tenth parallel of the Northern hemisphere.
 
NOAA 11094The bipolar pores were noticed on 8.08 at the Western limb, at the 25th parallel of the Northern hemisphere.
 
NOAA 11095The small sunspot was noticed at the middle latitudes of the Southern hemisphere, to the West from the central meridian.
 
NOAA 11096The high latitude pores were noticed in the Northern hemisphere since 9.08 to 13.08 to the West from the central meridian.
 
NOAA 11097The short-time pore was noticed at the 33rd parallel since 11.08 to 13.08 to the East from the central meridian.
 
NOAA 11098The short-time sunspots were noticed at the middle latitudes of the Northern hemisphere since 12.08 to 14.08 neighboring the central meridian.
 
NOAA 11099The small bipolar sunspots were observed since 14.06 to 16.08 at the middle latitudes of the Northern hemisphere, near the Western limb.
 












Locations of visitors to this page