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Дата изменения: Wed Feb 3 21:00:58 2016
Дата индексирования: Sun Apr 10 02:13:30 2016
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The Sunspot Observer - The solar regions - The description of the solar regions

Statistics of sunspot activity

NOAA 10000 - NOAA 10999
The description of the solar regions

NOAA 10000The fine bipolar sunspots were observed at the mid latitudes of the Northern hemisphere since 14.06 to 21.06.02.
 
NOAA 10001The perceptible bipolar group crossed the Sun disc since 14.06 to 26.06.02 along the high latitudes of the Northern hemisphere. The bipole consisted of the developed head sunspot with simmetrical penumbra and tail pores. The total region's area reached 150-200 m.s.h.
 
NOAA 10002The one-day pore was noticed at the 24th parallel of the Southern hemisphere on 16.06.02, to the West from the central meridian.
 
NOAA 10003The insignificant bipole was observed at the Sun equator since 15.06 to 17.06.02, in the Eastern part of the Sun disc.
 
NOAA 10004The fine bipolar group was observed at the mid latitudes of the Southern hemisphere since 14.06 to 21.06.02. From time to time it was counted 10-15 sunspots in the bipole.
 
NOAA 10005The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 16.06 to 29.06.02 along the mid latitudes of the Northern hemisphere. Fine sunspots and pores with opposite magnetic polarity appeared and disappeared neighbouring the sunspot. The total region's area exceeded 150 m.s.h.
 
NOAA 10006The fine sunspots were observed at the low latitudes of the Southern hemisphere since 18.06 to 21.06.02, in the Western part of the Sun disc.
 
NOAA 10007The fine bipolar group was observed since 18.06 to 21.06.02 to the South from the region 10001.
 
NOAA 10008The big sunspot with imposing symmetrical penumbra crossed the Sun disc since 18.06 to 1.07.02 along the tenth parallel of the Southern hemisphere. Fine sunspots and pores appeared and disappeared neighbouring the sunspot. From time to time the total region's area exceeded 500 m.s.h.
 
NOAA 10009The bipolar pores were marked on 20.06 and 21.06.02 in the Western limb.
 
NOAA 10010The short-time sunspots were noticed since 22.06 to 24.06.02 in the central part of the Sun disc.
 
NOAA 10011The small bipolar group crossed the Sun disc since 21.06 to 3.07.02 along the tenth parallel of the Southern hemisphere. From time to time the total region's area reached 100 m.s.h.
 
NOAA 10012The short-time pores were observed at the high latitudes of the Northern hemisphere since 23.06 to 25.06.02, neighbouring the central meridian.
 
NOAA 10013The bipolar pores were noticed since 23.06 to 25.06.02 in the central part of the Sun disc.
 
NOAA 10014The mid latitude pores were marked in the Southern hemisphere on 23.06 and 24.06.02, near the Eastern limb.
 
NOAA 10015The insignificant bipolar sunspots were observed at the 27th parallel of the Southern hemisphere since 24.06 to 28.06.02.
 
NOAA 10016The small sunspot with symmetrical penumbra crossed the Sun disc since 25.06 to 7.07.02 along the mid latitudes of the Southern hemisphere. From time to time pores with opposite magnetic polarity were observed neighbouring the sunspot.
 
NOAA 10017The new bipolar group had appeared at the high latitudes of the Southern hemisphere on 27.06.02, to the East from the central meridian. The bipole was assuming triangle form and gradually extending. On 5.07 the new region had reached the Western limb, and before it the total area exceeded 600 m.s.h.
 
NOAA 10018The small bipolar group was marked at the Western limb since 29.06 to 1.07.02.
 
NOAA 10019The triangle combination of several developed sunspots with penumbraes was observed at the mid latitudes of the Southern hemisphere since 29.06 to 11.07.02. The greater sunspot in the group was slowly bifurcating into two nuclears with penumbraes. From time to time the total region's area exceeded 500 m.s.h.
 
NOAA 10020The near equatorial pores were noticed since 2.07 to 4.07.02 not far from the Eastern limb.
 
NOAA 10021The fine bipolar chain was marked at the 29th parallel of the Southern hemisphere since 3.07 to 10.07.02, in the Western part of the Sun disc.
 
NOAA 10022The insignificant bipolar sunspots were observed since 3.07 to 10.07.02 to the East from the region 10019.
 
NOAA 10023The insignificant sunspots were settled at the high latitudes of the Southern hemisphere since 2.07 to 10.07.02.
 
NOAA 10024The fast development of a bipolar group had plase at the 34th parallel of the Southern hemisphere since 3.07 to 10.07.02. From time to time the total region's area reached 200 m.s.h.
 
NOAA 10025The fine sunspot with symmetrical penumbra crossed the Sun disc since 4.06 to 16.06.02 along the high latitudes of the Southern hemisphere.
 
NOAA 10026The fine sunspots were marked on 5.07 and 6.07.02 at the Western limb.
 
NOAA 10027The bipolar one-day pores were noticed on 7.07.02 in the central part of the Sun disc.
 
NOAA 10028The fine bipolar formation was observed at the mid latitudes of the Southern hemisphere since 8.07 to 17.07.02.
 
NOAA 10029The fine bipolar formation was observed at the mid latitudes of the Southern hemisphere since 8.07 to 17.07.02.
 
NOAA 10030The large multipolar group crossed the Sun disc since 9.07 to 23.07.02 along the high latitudes of the Northern hemisphere. The maximal total area of the region exceeded 1300 m.s.h., and it was counted 90 sunspots in the group. The multipole consisted of three big parts. In the first days the head sunspots were more developed part of the group. But then these sunspots began decay, and in the same time the central and tail parts of the group turned to the process of slow collapse.
 
NOAA 10031The insignificant pores were observed since 11.07 to 16.07.02 to the South-East from the large region 10030.
 
NOAA 10032The recurrent pores were marked at the high latitudes of the Southern hemisphere on 13.07 and 16.07.02, in the Western part of the Sun disc.
 
NOAA 10033The insignificant sunspots were observed since 13.07 to 16.07.02 to the South-West from the large region 10030.
 
NOAA 10034The short-time bipolar formation was noticed at the high latitudes of the Southern hemisphere since 13.07 to 15.07.02, neighbouring the central meridian.
 
NOAA 10035The bipolar chain of small sunspots was observed to the West from the large region 10036 since 15.07 to 25.07.02.
 
NOAA 10036The large multipolar group crossed the Sun disc since 15.07 to 27.07.02 along the low latitudes of the Southern hemisphere. In the evolution's peak the total region's area exceeded 1000 m.s.h., and it was more 60 sunspots in the group. The multipole consisted of many developed sunspots with were united by several large pieces of penumbra. After intersection the central meridian the tail part of the group began slowly decay.
 
NOAA 10037The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 16.07 to 28.07.02 along the mid latitudes of the Northern hemisphere. The total sunspot's area reached 150-200 m.s.h.
 
NOAA 10038The fine bipolar group was observed at the mid latitudes of the Northern hemisphere since 19.07 to 29.07.02.
 
NOAA 10039The large multipolar group crossed the Sun disc since 21.07 to 3.08.02 along the mid latitudes of the Southern hemisphere. From time to time the total region's area reached 1000 m.s.h. In the first days the head sunspots were more developed part of the group. After intersection of the central meridian the head sunspots began slowly decay, and the group was lining.
 
NOAA 10040The short-time pores were marked since 22.07 to 25.07.02 to the South-East from the big region 10036.
 
NOAA 10041The insignificant bipolar sunspots were observed at the mid latitudes of the Northern hemisphere since 22.07 to 25.07.02.
 
NOAA 10042The insignificant bipolar sunspots were observed at the high latitudes of the Southern hemisphere since 21.07 to 30.07.02.
 
NOAA 10043The perceptible bipolar chain was observed at the mid latitudes of the Northern hemisphere since 23.07 to 1.08.02. The total region's area reached 150-200 m.s.h. In the first days the tail sunspots were more developed part of the group. But slow decay of the tail part was simultaneously happened with gradual development of the head sunspots. In result the decay's process touched the whole group.
 
NOAA 10044The big bipolar group crossed the Sun disc since 23.07 to 3.08.02 along the high latitudes of the Southern hemisphere. The group appeared in immediate nearness from the big region 10039. Its were parallelly situated. The new bipole was lining, and newly originating sunspots extended. From time to time the total region's area exceeded 500 m.s.h., and it was counted more 50 sunspots in the group.
 
NOAA 10045The fast development of a bipolar group took place at the low latitudes of the Northern hemisphere since 24.07 to 29.07.02.
 
NOAA 10046The short-time sunspots were marked on 24.07 and 25.07.02 between the regions 10038 and 10043.
 
NOAA 10047The fine bipolar formation was noticed since 25.07 to 27.07.02 not far from the Western limb.
 
NOAA 10048The fine bipolar group was observed at the high latitudes of the Northern hemisphere since 26.07 to 2.08.02.
 
NOAA 10049The short-time bipolar sunspots were marked on 26.07 and 27.07.02 in the Western part of the Sun disc.
 
NOAA 10050The new multipolar group had appeared at the low latitudes of the Southern hemisphere on 26.07.02, in the Eastern part of the Sun disc. In three days the total region's area increased in tens times and exceeded 500 m.s.h. Several seats of sunspot formation were observed in the group, therefore it extended and developed "from the inside". In the evolution's peak the total multipole's area had reached 700 m.s.h., and the sunspot's quantity had 50-60 units. On 4.08 the new group had come to the Western limb.
 
NOAA 10051The small sunspot with symmetrical penumbra crossed the Sun disc since 27.07 to 8.08.02 along the mid latitudes of the Southern hemisphere.
 
NOAA 10052The insignificant bipolar formation was marked at the low latitudes of the Northern hemisphere on 28.07 and 29.07.02, neighbouring the central meridian.
 
NOAA 10053The fine bipolar formation was noticed since 28.07 to 30.07.02 to the South-East from the big region 10050.
 
NOAA 10054The fine sunspots were marked since 28.07 to 2.08.02 to the South-East from the sunspot 10051.
 
NOAA 10055The fine bipolar group crossed the Sun disc since 29.07 to 8.08.02 along the mid latitudes of the Northern hemisphere.
 
NOAA 10056The insignificant bipolar formation was observed on 1.08 and 2.08.02 in the Eastern part of the Sun disc.
 
NOAA 10057The developing bipolar chain of sunspots was observed at the low latitudes of the Southern hemisphere since 1.08 to 8.08.02, in the Western part of the Sun disc. The newly arising sunspots developed and extended. Not long before set for the limb the new group assumed closed magnetic configuration, and the total area reached 400 m.s.h. It was counted more 30 sunspots in the region.
 
NOAA 10058The fine bipolar group crossed the Sun disc since 1.08 to 13.08.02 along the low latitudes of the Southern hemisphere.
 
NOAA 10059The small bipolar group crossed the Sun disc since 2.08 to 10.08.02 along the mid latitudes of the Northern hemisphere. The head sunspot had fine asymmetrical penumbra.
 
NOAA 10060The short-time bipolar sunspots were marked at the 28th parallel of the Southern hemisphere since 3.08 to 5.08.02, in the Western part of the Sun disc.
 
NOAA 10061The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 3.08 to 16.08.02 along the low latitudes of the Northern hemisphere. The rapid development of sunspots and pores with opposite magnetic polarity was observed behind the sunspot. In the evolution's peak the total region's area exceeded 300 m.s.h.
 
NOAA 10062The one-day sunspots were noticed at the Sun equator on 5.08.02, in the Western part of the Sun disc.
 
NOAA 10063The opened bipolar group crossed the Sun disc since 6.08 to 19.08.02 along the mid latitudes of the Northern hemisphere. The bipole consisted of head and tail sunspots with penumbraes of moderate sizes. The head sunspot had oblong form, and after intersection of the central meridian it bifurcated and gradually decayed. The tail sunspot had stable symmetrical form. Neighbouring the central meridian a chain of pores was observed to the South from the tail sunspot. From time to time the total region's area reached 200 m.s.h.
 
NOAA 10064The short-time sunspots were marked at the high latitudes of the Southern hemisphere since 7.08 to 9.08.02.
 
NOAA 10065The recurrent pores were observed at the tenth parallel of the Southern hemisphere since 7.08 to 14.08.02.
 
NOAA 10066The shapeless bipolar formation crossed the Sun disc since 9.08 to 21.08.02 along the mid latitudes of the Northern hemisphere. Neighbouring the central meridian the total region's area reached 100-150 m.s.h.
 
NOAA 10067The unstable bipolar chain of sunspots crossed the Sun disc since 10.08 to 23.08.02 along the tenth parallel of the Northern hemisphere. Neighbouring the central meridian the total region's area reached 300 m.s.h., and it was counted 40 sunspots in the group.
 
NOAA 10068The bipolar combination of small sunspots was parted by considerable longitude's distance. The group was observed since 10.08 to 19.08 to the West from the large region 10069.
 
NOAA 10069The large multipole crossed the Sun disc since 11.08 to 24.08.02 along the low latitudes of the Southern hemisphere. The greater part of sunspots was embedded into giant irregular penumbra. Neighbouring the central meridian the total region's area reached 2000 m.s.h., and it was counted more 60 sunspots in the group.
 
NOAA 10070The short-time pores were marked on 11.08 and 12.08.02 in the central part of the Sun disc.
 
NOAA 10071The fine sunspot was noticed at the tenth parallel of the Northern hemisphere since 11.08 to 13.08.02, in the Eastern part of the Sun disc.
 
NOAA 10072The growing bipolar group was observed at the mid latitudes of the Southern hemisphere since 11.08 to 16.08.02, in the Western part of the Sun disc. Before set for the limb the total region's area had reached 300 m.s.h.
 
NOAA 10073The one-day pores were noticed on 12.08.02 to the West from the bipolar region 10063.
 
NOAA 10074The one-day pores were marked at the high latitudes of the Northern hemisphere on 12.08.02, neighbouring the central meridian.
 
NOAA 10075The fine bipolar group was observed at the tenth parallel of the Southern hemisphere since 12.08 to 15.08.02, neighbouring the central meridian.
 
NOAA 10076The fine sunspot with symmetrical penumbra crossed the Sun disc since 12.08 to 21.08.02 along the mid latitudes of the Northern hemisphere.
 
NOAA 10077The short-time pore was noticed on 13.08 and 14.08.02 to the North from the large region 10069.
 
NOAA 10078The small bipolar group was marked at the mid latitudes of the Southern hemisphere since 13.08 to 17.08.02, in the Western part of the Sun disc.
 
NOAA 10079The developing bipolar group crossed the Sun disc since 14.08 to 25.08.02 along the high latitudes of the Southern hemisphere. The main seats of sunspot's formation were scattered on the whole group. Neighbouring the central meridian the group had assumed closed configuration, and the total region's area had exceeded 300 m.s.h. It was counted more 30 sunspots in the group. Then the tail part of the group began impetuously decay, and the head sunspots reached the Western limb.
 
NOAA 10080The small bipolar group crossed the Sun disc since 13.08 to 26.08.02 along the mid latitudes of the Northern hemisphere. The tail sunspot had aswymmetrical penumbra and was gradually decaying. In the first days the total region's area exceeded 100 m.s.h.
 
NOAA 10081The fine sunspots were observed since 15.08 to 18.08.02 to the East from the bipolar region 10080.
 
NOAA 10082The fine sunspots were marked at the high latitudes of the Northern hemisphere since 17.08 to 20.08.02, neighbouring the central meridian.
 
NOAA 10083The spreading bipolar group crossed the Sun disc since 17.08 to 28.08.03 along the high latitudes of the Southern hemisphere. The region had not regular configuration of sunspots, from time to time the total area exceeded 150 m.s.h.
 
NOAA 10084The small sunspot with symmetrical penumbra was observed to the South-West from the big region 10085 since 17.08 to 29.08.02. There were fine sunspots and pores of opposite magnetic polarity neighbouring the sunspot.
 
NOAA 10085The big sunspot with imposing penumbra crossed the Sun disc since 18.08 to 31.08 along the tenth parallel of the Southern hemisphere. Fine sunspots and pores appeared and disappeared neighbouring the sunspot. The total region's area exceeded 500 m.s.h.
 
NOAA 10086The high latitude pores were marked in the Southern hemisphere since 21.08 to 24.08.02.
 
NOAA 10087The big sunspot crossed the Sun disc since 22.08 to 3.09.02 along the low latitudes of the Southern hemisphere. In the first days the total region's area reached 400 m.s.h. Neighbouring the central meridian the sunspot began crumbled. In result the sunspot had diminished in several times.
 
NOAA 10088The new bipolar group had appeared at the high latitudes of the Southern hemisphere on 23.08.02, to the West from the central meridian. The bipole was dynamic developing, in three days the total area exceeded 200 m.s.h. On 27.08 the new region had come to the Western limb.
 
NOAA 10089The short-time pore was marked on 24.08 and 25.08.02 to the South-East from the big region 10087.
 
NOAA 10090The fine bipolar sunspots crossed the Sun disc since 25.08 to 4.09.02 along the equator.
 
NOAA 10091The one-day pores were noticed on 27.08.02 to the North frrom the region 10090.
 
NOAA 10092The insignificant sunspots were observed since 27.08 to 30.08.02 to the South from the region 10087.
 
NOAA 10093The fine sunspot with rudiments of penumbra was marked on 29.08.02 to the South from the region 10090.
 
NOAA 10094The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 29.08 to 9.09.02 along the high latitudes of the Southern hemisphere. In the first days sunspots of opposite magnetic polarity were observed behind the sunspot. The total region's area exceeded 100 m.s.h.
 
NOAA 10095The long bipolar group crossed the Sun disc since 29.08 to 10.09.02 along the low latitudes of the Northern hemisphere. The bipole consisted of developed sunspots with penumbraes and pores stretching on the twenty degrees at a longitude and more. Maximal total area of the region exceeded 800 m.s.h., and it was counted more 50 sunspots in the group.
 
NOAA 10096The developing bipolar group crossed the Sun disc since 30.08 to 10.09.02 along the mid latitudes of the Southern hemisphere. The bipole consisted of the head sunspot with stable symmetrical penumbra and the string of developing sunspots. In the evolution's peak the total region's area exceeded 200 m.s.h., and it was counted more twenty sunspots and pores in the group.
 
NOAA 10097The perceptible bipolar chain of small sunspots with penumbraes was marked to the West from the big region 10095 since 1.09 to 8.09.02. From time to time the total region's area exceeded 100 m.s.h., and it was counted more twenty sunspots and pores in the group.
 
NOAA 10098The insignificant sunspots were observed at the tenth parallel of the Southern hemisphere since 1.09 to 5.09.02, in the Eastern part of the Sun disc.
 
NOAA 10099The small bipolar group crosssed the Sun disc since 1.09 to 8.09.02 along the equator. The head sunspot had fine penumbra.
 












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