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Дата изменения: Wed Feb 3 21:01:01 2016
Дата индексирования: Sun Apr 10 02:17:00 2016
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Поисковые слова: redshift survey
The Sunspot Observer - The solar regions - The description of the solar regions

Statistics of sunspot activity

NOAA 10200 - NOAA 10299
The description of the solar regions

NOAA 10200The small sunspot with symmetrical penumbra crossed the Sun disc since 20.11 to 30.11.02, along the equator.
 
NOAA 10201The small bipolar formation was noticed to the West from the big region 10198 since 21.11 to 25.11.02.
 
NOAA 10202The fine bipolar sunspots crossed the Sun disc since 24.11 to 3.12.02, along the mid latitudes of the Northern hemisphere.
 
NOAA 10203The insignificant pores were observed at the tenth parallel of the Northern hemisphere since 26.11 to 4.12.02.
 
NOAA 10204The insignificant bipolar sunspots were observed at the mid latitudes of the Northern hemisphere since 27.11 to 2.12.02.
 
NOAA 10205The fine sunspot with symmetrical penumbra crossed the Sun disc since 26.11 to 9.12.02, along the high latitudes of the Northern hemisphere.
 
NOAA 10206The short-time sunspots were marked at the high latitudes of the Southern hemisphere on 27.11 and 28.11.02, not far from the Eastern limb.
 
NOAA 10207The long bipolar configuration of several perceptible sunspots with penumbraes crossed the Sun disc since 26.11 to 9.12.02, along the high latitudes of the Southern hemisphere. In the first days the head and tail parts of the group consisted of several sunspots but later there was a sunspot each in the parts which assumed symmetrical form. The maximal total region's area exceeded 300 m.s.h.
 
NOAA 10208The shapeless bipolar formation crossed the Sun disc since 29.11 to 8.12.02, along the tenth parallel of the Northern hemisphere. The total region's area exceeded 100 m.s.h.
 
NOAA 10209The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 29.11 to 11.12.02, along the high latitudes of the Southern hemisphere. The hardly visible tail sunspots were in the first days. The maximal total region's area exceeded 150 m.s.h.
 
NOAA 10210The bipolar sunspots with penumbraes were noticed at the Western limb on 30.11 and 1.12.02.
 
NOAA 10211The bipolar pores were marked on 2.12.02 in the Sun disc's center.
 
NOAA 10212The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 2.12 to 11.12.02, along the mid latitudes of the Northern hemisphere. Small sunspots and pores appeared and disappeared neighbouring the sunspot. In the first days the total region's area reached 200 m.s.h. After intersection of the central meridian the group began decay.
 
NOAA 10213The small bipolar group crossed the Sun disc since 3.12 to 13.12.02, along the mid latitudes of the Northern hemisphere. The head sunspot had fine symmetrical penumbra.
 
NOAA 10214The new bipolar group was observed at the mid latitudes of the Southern hemisphere since 5.12 to 10.12.02, in the Western part of the Sun disc. The head sunspot had perceptible symmetrical penumbra, and the tail sunspot had fine penumbra. Many pores were scattered between the sunspots.
 
NOAA 10215The rest of the big bipolar region 10191 crossed the Sun disc since 5.12 to 14.12.02 along the high latitudes of the Southern hemisphere. On 8.12 the sunspot with symmetrical penumbra had bifurcated and began slowly decay.
 
NOAA 10216The small bipolar formation was noticed at the high latitudes of the Southern hemisphere since 7.12 to 10.12.02, in the Western part of the Sun disc. The main sunspots had rudiments of penumbra.
 
NOAA 10217The insignificant sunspots were observed at the mid latitudes of the Northern hemisphere since 7.12 to 12.12.02, in the Eastern part of the Sun disc.
 
NOAA 10218The fine high latitude sunspot with symmetrical penumbra was observed to the South-East from the region 10220 since 7.12 to 19.12.02. Single pores appeared and disappeared behind the sunspot.
 
NOAA 10219The fine near equatorial sunspot with penumbra was marked in the Western part of the Sun disc since 9.12 to 11.12.02.
 
NOAA 10220The perceptible bipolar group crossed the Sun disc since 7.12 to 19.12.02, along the mid latitudes of the Southern hemisphere. In the first days the tail part of the group was developed and consisted of several perceptible sunspots with penumbraes and pores. In next days the head sunspot with asymmetrical penumbra was extending, and the tail sunspots began decay. In the evolution's peak the total region's area had exceeded 300 m.s.h., and it was counted 20-25 sunspots in the group.
 
NOAA 10221The insignificant sunspots were observed at the high latitudes of the Northern hemisphere since 8.12 to 14.12.02, in the Eastern part of the Sun disc.
 
NOAA 10222The short-time sunspots were marked in the Southern hemisphere since 10.12 to 13.12.02.
 
NOAA 10223The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 12.12 to 24.12.02, along the high latitudes of the Northern hemisphere. Fine sunspots and pores appeared and disappeared around it.
 
NOAA 10224The spreading bipolar configuration of small sunspots and pores was observed to the North from the big region 10226 since 12.12 to 26.12.02.
 
NOAA 10225The perceptible bipolar group was observed at the Western district of the big region 10229 since 12.12 to 23.12.02. In the evolution's peak the total bipole's area had reached 100 m.s.h., and it was counted 15-20 sunspots in the group.
 
NOAA 10226The big bipolar group crossed the Sun disc since 13.12 to 24.12.02, along the high latitudes of the Southern hemisphere. In result of the development the region turned into very long and solid chain of sunspots with penumbraes which was like a giant sword. The maximal total area of the chain reached the 700 m.s.h., and it was counted 50 sunspots in the group.
 
NOAA 10227The small bipolar formation was marked at the low latitudes of the Northern hemisphere since 13.12 to 21.12.02. The main sunspots had fine penumbraes.
 
NOAA 10228The insignificant sunspots were observed at the mid latitudes of the Southern hemisphere since 14.12 to 20.12.02.
 
NOAA 10229The big multipolar group crossed the Sun disc since 14.12 to 26.12.02, along the mid and high latitudes of the Northern hemisphere. The head part of the group was settled at the mid latitudes and consisted of two nearby sunspots with perceptible asymmetrical penumbraes. The tail part of the group was situated at the high latitudes and was made by two duplex nuclears with general oblong penumbra. Many small sunspots with asymmetrical penumbraes and pores were scattered in the intermediate part of the group. The maximal total area of the region exceeded 400 m.s.h., and it was counted 40-45 sunspots in the group. All parts of the group were gradually diminished and decayed.
 
NOAA 10230The perceptible bipolar group crossed the Sun disc since 17.12 to 28.12.02, along the low latitudes of the Southern hemisphere. The bipole consisted of the head sunspot with stable symmetrical penumbra and woven string of many small sunspots with penumbraes. Neighbouring the central meridian the total region's area reached 300 m.s.h. Later the tail part of the group had decayed, and the head sunspot reached the Western limb.
 
NOAA 10231The small bipolar group crossed the Sun disc since 19.12 to 27.12.02, along the 25th parallel of the Southern hemisphere. The main sunspots had fine penumbraes.
 
NOAA 10232The short-time sunspots were noticed at the mid latitudes of the Northern hemisphere on 21.12 and 22.12.02, to the West from the central meridian.
 
NOAA 10233The short-time sunspots were marked at the mid latitudes of the Northern hemisphere since 22.12 to 25.12.02, in the Eastern part of the Sun disc.
 
NOAA 10234The small sunspot with symmetrical penumbra crossed the Sun disc since 24.12 to 30.12.02, along the high latitudes of the Northern hemisphere. The rest of the region 10205.
 
NOAA 10235The insignificant recurrent sunspots were situated at the mid latitudes of the Northern hemisphere since 24.12 to 30.12.02.
 
NOAA 10236The fine bipolar group was observed at the mid latitudes of the Northern hemisphere since 27.12 to 29.12.02, in the Western part of the Sun disc.
 
NOAA 10237The short-time bipolar pores were marked at the high latitudes of the Southern hemisphere on 28.12.02, neighbouring the central meridian.
 
NOAA 10238The short-time pore was marked on 28.12.02 in the central part of the Sun disc.
 
NOAA 10239The fine bipolar group crossed the Sun disc since 29.12.02 to 7.01.03, along the low latitudes of the Southern hemisphere.
 
NOAA 10240The insignificant bipolar group was situated at the low latitudes of the Southern hemisphere since 31.12.02 to 7.01.03.
 
NOAA 10241The small high latitude sunspots were observed in the Southern hemisphere since 2.01 to 4.01.03, not far from the Western limb.
 
NOAA 10242The perceptible bipolar group crossed the Sun disc since 2.01 to 13.01.03, along the low latitudes of the Southern hemisphere. In the evolution's peak the total region's area exceeded 300 m.s.h.
 
NOAA 10243The new quick-growing group was observed at the high latitudes of the Southern hemisphere since 3.01 to 8.01.03, in the Western part of the Sun disc.
 
NOAA 10244The small bipolar group crossed the Sun disc since 2.01 to 12.01.03, along the high latitudes of the Southern hemisphere. The bipole consisted of the head sunspot with asymmetrical penumbra and the string of the few fine spots behind it. In the first days the total region's area exceeded 100 m.s.h.
 
NOAA 10245The fine sunspot with asymmetrical penumbra crossed the Sun disc since 3.01 to 10.01.03, along the mid latitudes of the Northern hemisphere.
 
NOAA 10246The short-time sunspots were noticed in the central part of the Sun disc on 6.01 and 7.01.03.
 
NOAA 10247The new bipolar group crossed the Sun disc since 6.01 to 18.01.03, along the mid latitudes of the Southern hemisphere. The group was quick developing but it had not stable form. In the evolution's peak the total region's area had exceeded 300 m.s.h., and it was counted 40-50 sunspots in the group.
 
NOAA 10248The short-time sunspots were marked at the tenth parallel of the Southern hemisphere since 6.01 to 9.01.03, in the Western part of the Sun disc.
 
NOAA 10249The insignificant bipolar sunspots were situated at the mid latitudes of the Southern hemisphere since 4.01 to 15.01.03.
 
NOAA 10250The perceptible sunspot with oblong penumbra crossed the Sun disc since 7.01 to 20.01, along the high latitudes of the Southern hemisphere. The total region's area exceeded 100 m.s.h.
 
NOAA 10251The perceptible bipolar group crossed the Sun disc since 7.01 to 18.01.03, along the mid latitudes of the Southern hemisphere. In the first days the total region's area reached 400 m.s.h. The head sunspot had big assymetrical penumbra. Three small tail sunspots with symmetrical penumbraes were lined. These sunsspots were slowly decayed.
 
NOAA 10252The short-time sunspots were marked to the North from the region 10251 since 9.01 to 12.01.03.
 
NOAA 10253The new bipolar group was noticed since 10.01 to 13.01.03 not far the Western limb. The head sunspot had fine symmetrical penumbra.
 
NOAA 10254The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 10.01 to 22.01.03, along the mid latitudes of the Southern hemisphere. The total region's area exceeded 100 m.s.h.
 
NOAA 10255The Western district of the region 10251 crossed the Sun disc since 8.01 to 20.01.03, along the mid latitudes of the Southern hemisphere. In the first days the total region's area exceeded 400 m.s.h. The sunspot had big asymmetrical penumbra which had bifurcated later. The greater part assumed symmetrical form, and the lesser sunspot was slowly decaying.
 
NOAA 10256The small sunspot with symmetrical penumbra was marked to the East from the region 10254 since 12.01 to 20.01.03.
 
NOAA 10257The insignificant bipolar group crossed the Sun disc since 13.01 to 21.01.03, along the mid latitudes of the Northern hemisphere.
 
NOAA 10258The small sunspot with symmetrical penumbra crossed the Sun disc since 13.01 to 25.01.03, along the low latitudes of the Northern hemisphere.
 
NOAA 10259The bipolar chain of fine sunspots crossed the Sun disc since 14.01 to 22.01.03, along the tenth parallel of the Northern hemisphere. The chain was slowly crumbling.
 
NOAA 10260The fine sunspots crossed the Sun disc since 15.01 to 26.01.03, along the mid latitudes of the Northern hemisphere.
 
NOAA 10261The fine formation was notices at the high latitudes of the Northern hemisphere since 19.01 to 21.01.03, in the Western part of the Sun disc.
 
NOAA 10262The fine bipolar group was marked since 19.01 to 21.01.03, near the Western limb.
 
NOAA 10263The new bipolar group had appeared at the mid latitudes of the Southern hemisphere on 19.01.03, neighbouring the central meridian. In two days the sunspots began extend. On 25.01 the new region had come to the Western limb.
 
NOAA 10264The one-day pore was marked on 20.01.03, in the central part of the Sun disc.
 
NOAA 10265The one-day pores were marked on 20.01.03, in the central part of the Sun disc.
 
NOAA 10266The long sunspot's chain crossed the Sun disc since 19.01 to 31.01.03, along the high latitudes of the Southern hemisphere. Neighbouring the central meridian the head sunspot was divided into parts which began extend. In several days the sunspots retutned in the decay's process. From time to time the total region's area reached 200 m.s.h., and it was counted 25-30 sunspots in the group.
 
NOAA 10267The small sunspot had symmetrical penumbra, and a long string of the few fine sunspots streched behind it. In the first days the total region's area exceeded 150 m.s.h.
 
NOAA 10268The solid congestion of small sunspots was slowly streching and decaying. The group was observed at the mid latitudes of the Northern hemisphere since 21.01 to 29.01.03. From time to time the total region's area exceeded 100 m.s.h.
 
NOAA 10269The perceptible bipolar group crossed the Sun disc since 21.01 to 2.02.03, along the low latitudes of the Southern hemisphere. The bipole consisted of two nearby sunspots with penumbraes. The head sunspot had stable symmetrical penumbra. The tail sunspot was slowly decaying. In the first days the total region's area reached 150-200 m.s.h.
 
NOAA 10270The insignificant bipolar formation was situated at the low latitudes of the Southern hemisphere since 25.01 to 30.01.03, in the Western part of the Sun disc.
 
NOAA 10271The fine bipolar group was marked at the low latitudes of the Southern hemisphere since 26.01 to 31.01.03, in the Western part of the Sun disc.
 
NOAA 10272The bipolar configuration of fine sunspots and pores crossed the Sun disc since 26.01 to 3.02.03, along the low latitudes of the Southern hemisphere. On 30.01 it was counted 20 sunspots in the group.
 
NOAA 10273The new bipolar group was observed at the low latitudes of the Northern hemisphere since 27.01 to 1.02.03, in the Western part of the Sun disc. The total region's area exceeded 100 m.s.h.
 
NOAA 10274The small eruptive group crossed the Sun disc since 28.01 to 9.02.03, along the low latitudes of the Southern hemisphere. In the first days the group was as single sunspot with symmetrical penumbra. On 1.02 the sunspot had acquired a satellite with the opposite magnetic polarity. The bipole consisted of two small sunspots with symmetrical penumbraes. From time to time the total region's area exceeded 100 m.s.h.
 
NOAA 10275The short-time sunspots were marked on 29.01 and 30.01.03, to the South-East from the bipolar region 10272.
 
NOAA 10276The long chain of small sunspots crossed the Sun disc since 1.02 to 14.02.03, along the mid latitudes of the Southern hemisphere. In the first days the total region's area reached 300 m.s.h. The sunspots were slowly dissolving against the Sun disc.
 
NOAA 10277The insignificant bipolar formation crossed the Sun disc since 4.02 to 14.02.03, along the high latitudes of the Southern hemisphere.
 
NOAA 10278The amorph bipolar formation crossed the Sun disc since 4.02 to 13.02.03, along the mid latitudes of the Northern hemisphere. The continuation of the region 10257. In the first days the total group's area exceeded 100 m.s.h.
 
NOAA 10279The short-time pores were marked in the central part of the Sun disc since 4.02 to 8.02.03.
 
NOAA 10280The fine bipolar formation crossed the Sun disc since 4.02 to 13.02.03, along the low latitudes of the Southern hemisphere.
 
NOAA 10281The fine sunspot with symmetrical penumbra crossed the Sun disc since 6.02 to 15.02.03, along the mid latitudes of the Southern hemisphere. The rest of the bipolar region 10263.
 
NOAA 10282The small group was noticed to the South-West from the region 10278 since 5.02 to 16.02.03. In the first days the group was as a single pore, later a small bipolar configuration appeared in the place.
 
NOAA 10283The fine bipolar chain crossed the Sun disc since 7.02 to 15.02.03 along the equator. The sunspots were slowly decaying.
 
NOAA 10284The fine bipolar sunspots were observed at the mid latitudes of the Northern hmisphere since 7.02 to 11.02.03, to the West from the central meridian.
 
NOAA 10285The small sunspot with symmetrical penumbra crossed the Sun disc since 8.02 to 16.02.03, along the tenth parallel of the Southern hemisphere. The rest of the bipolar region 10263. The sunspot was slowly diminished.
 
NOAA 10286The short-time sunspots were marked on 9.02 and 10.02.03 between the regions 10276 and 10280.
 
NOAA 10287The new sunspots were noticed at the Western limb on 15.02 and 16.02.03.
 
NOAA 10288The fine sunspot with symmetrical penumbra crossed the Sun disc since 15.02 to 27.02.03, along the mid latitudes of the Northern hemisphere. More fine sunspots and pores appeared and disappeared behind the sunspot.
 
NOAA 10289The new quick-growing group was observed at the tenth parallel of the Northern hemisphere since 18.02 to 21.02.03, near the Western limb. The total region's area exceeded 200 m.s.h.
 
NOAA 10290The new bipolar group had appeared at the mid latitudes of the Southern hemisphere on 18.02.03, in the Eastern part of the Sun disc. The group was rapidly extending and developing. Neighbouring the central meridian the total area reached 400 m.s.h. It was counted 25-30 sunspots and pores in the bipole. The head and tail sunspots had developed penumbraes and were connected by a chain of fine sunspots and pores. Then the tail sunspots began slowly decay, and the head part of the group had come to the Western limb on 1.03.
 
NOAA 10291The short-time high latitude sunspots were noticed in the Southern hemisphere on 21.02 and 22.02.03, neighbouring the central meridian.
 
NOAA 10292The fine law latitude group was observed in the Southern hemisphere since 25.02 to 3.03, in the Western part of the Sun disc.
 
NOAA 10293The short-time bipolar sunspots were observed at the high latitudes of the Southern hemisphere since 26.02 to 1.03.03, in the Eastern part of the Sun disc.
 
NOAA 10294The fine bipolar formation crossed the Sun disc since 26.02 to 6.03.03, along the low latitudes of the Southern hemisphere.
 
NOAA 10295The small sunspot with symmetrical penumbra crossed the Sun disc since 26.02 to 8.03.03, along the mid latitudes of the Southern hemisphere. On 5.03 the sunspot had bifurcated and began decay.
 
NOAA 10296The sunspot with large penumbra crossed the Sun disc since 28.02 to 12.03.03, along the mid latitudes of the Northern hemisphere. Several small spots were observed behind the sunspot. The total region's area reached 600-700 m.s.h.
 
NOAA 10297The fine bipolar group crossed the Sun disc since 1.03 to 12.03.03, along the mid latitudes of the Southern hemisphere.
 
NOAA 10298The short-time bipolar formation was marked at the low latitudes of the Southern hemisphere since 3.03 to 5.03.03.
 
NOAA 10299The small bipolar group was noticed to the East from the big sunspot 10296 since 1.03 to 10.03.03.
 












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