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

Statistics of sunspot activity

NOAA 09800 - NOAA 09899
The description of the solar regions

NOAA 09800The long bipolar group crossed the Sun disc since 25.01 to 5.02.02 along the low latitudes of the Northern hemisphere. The total region's area reached 600 m.s.h., and it was counted 50-60 sunspot in the group. The head and tail parts of the group consisted of developed sunspots with asymmetrical penumbra, and many fine sunspots and pores were settled between its.
 
NOAA 09801The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 25.01 to 6.02.02 along the equator. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot. The total region's area reached 100 m.s.h.
 
NOAA 09802The big bipolar group crossed the Sun disc since 26.01 to 8.02.02 along the mid latitudes of the Southern hemisphere. The total region's area reached 600 m.s.h., and it was counted 50-60 sunspots in the group. The multipole consisted of several big penumbra's pieces with embedded sunspots. The group was continuously changing the form.
 
NOAA 09803The high latitude bipolar sunspots were observed in the Southern hemisphere since 27.01 to 30.01.02, in the Western part of the Sun disc.
 
NOAA 09804The recurrent sunspots were noticed at the high latitudes of the Southern hemisphere since 28.01 to 1.02.02.
 
NOAA 09805The fine bipolar sunspots were marked at the mid latitudes of the Northern hemisphere since 28.01 to 31.01.02, in the Eastern part of the Sun disc.
 
NOAA 09806The fine sunspot with symmetrical penumbra crossed the Sun disc since 28.01 to 8.02.02 along the tenth parallel of the Northern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
 
NOAA 09807The crumbled chain of small sunspots were marked at the 27th parallel of the Southern hemisphere since 31.01 to 8.02.02. In the first days the total region's area exceeded 300 m.s.h.
 
NOAA 09808The short chain of fine sunspots was observed at the mid latitudes of the Northern hemisphere since 31.01 to 9.02.02.
 
NOAA 09809The opened bipolar group crossed the Sun disc since 30.01 to 12.02.02 along the low latitudes of the Southern hemisphere. The tail sunspot had symmetrical penumbra. In the first days the total region's area reached 150 m.s.h.
 
NOAA 09810The big sunspot with symmetrical penumbra crossed the Sun disc since 1.02 to 14.02.02 along the tenth parallel of the Northern hemisphere. The total region's area reached 250 m.s.h. From time to time pores with opposite magnetic polarity were observed neighbouring the sunspot.
 
NOAA 09811The bipolar group crossed the Sun disc since 2.02 to 14.02.02 along the 26th parallel of the Southern hemisphere. The total region's area reached 200 m.s.h. The bipole consisted of the perceptible head sunspot with asymmetrical penumbra and fine tail sunspots.
 
NOAA 09812The fine bipolar formation was observed at the mid latitudes of the Northern hemisphere since 2.02 to 6.02.02, in the Western part of the Sun disc. The head sunspot had symmetrical penumbra.
 
NOAA 09813The fine sunspot with symmetrical penumbra was noticed on 3.02 and 4.02.02 to the South-East from the big region 09802.
 
NOAA 09814The insignificant sunspots were situated at the low latitudes of the Northern hemisphere since 3.02 to 9.02.02.
 
NOAA 09815The small bipolar group was marked since 3.02 to 10.02.02 to the East from the big sunspot 09810.
 
NOAA 09816The fine bipolar sunspots were observed since 29.01 to 8.02.02 at the Eastern district of the big region 09802.
 
NOAA 09817The short-time bipolar pores were noticed on 5.02 and 6.02.02 in the central part of the Sun disc.
 
NOAA 09818The recurrent pores were marked near the Sun equator since 5.02 to 9.02.02, in the Eastern part of the Sun disc.
 
NOAA 09819The insignificant sunspots crossed the Sun disc since 5.02 to 17.02.02 along the high latitudes of the Southern hemisphere.
 
NOAA 09820The insignificant bipolar sunspots were situated at the mid latitudes of the Northern hemisphere since 7.02 to 10.02.02, in the Eastern part of the Sun disc.
 
NOAA 09821The perceptible bipolar group was observed at the mid latitudes of the Southern hemisphere since 8.02 to 15.02.02. The total region's area reached 350 m.s.h., and it was counted 25-30 sunspots in the group. The bipole consisted of the large head sunspot with asymmetrical penumbra and string of many fine sunspots and pores.
 
NOAA 09822The fine bipolar formation crossed the Sun disc since 8.02 to 17.02.02 along the mid latitudes of the Northern hemisphere.
 
NOAA 09823The fine bipolar formation was settled at the Sun equator since 9.02 to 15.02.02.
 
NOAA 09824The perceptible sunspot with symmetrical penumbra was situated to the North from the big region 09825 since 9.02 to 21.02.02. The total sunspot's area reached 200 m.s.h.
 
NOAA 09825The long bipolar group crossed the Sun disc since 8.02 to 21.02.02 along the mid latitudes of the Southern hemisphere. The total region's area reached 500 m.s.h., and it was counted 50-60 sunspots in the group. The group consisted of two big sunspots with asymmetrical penumbraes which were connected by a short pore's chain. Another two chains of many fine sunspots and pores adjoined to the main sunspots from the East and the West.
 
NOAA 09826The fine bipolar sunspots were observed at the high latitudes of the Southern hemisphere since 10.02 to 14.02.02, in the Eastern part of the Sun disc.
 
NOAA 09827The one-day pore was noticed on 11.02.02 to the West from the region 09811.
 
NOAA 09828The recurrent sunspots were marked at the mid latitudes of the Southern hemisphere since 11.02 to 16.02.02.
 
NOAA 09829The fine bipolar sunspots were observed at the low latitudes of the Southern hemisphere since 14.02 to 17.02.02, in the Eastern part of the Sun disc.
 
NOAA 09830The big bipolar group crossed the Sun disc since 14.02 to 26.02.02 along the high latitudes of the Southern hemisphere. The total region's area reached 700 m.s.h., and it was counted 40-50 sunspots in the group. The leading part of the group consisted of sunspot's solid chain, and the tail sunspot with penumbra was situated hardly to North.
 
NOAA 09831The short-time sunspots were noticed on 16.02 and 17.02.02 in the Western part of the Sun disc.
 
NOAA 09832The fine bipolar sunspots were marked at the mid latitudes of the Southern hemisphere since 18.02 to 21.02.02, to the East from the central meridian.
 
NOAA 09834The fine near equatorial sunspots were observed since 19.02 to 22.02.02 in the Eastern part of the Sun disc.
 
NOAA 09835The new bipolar group was noticed at the Western limb since 20.02 to 22.02.02.
 
NOAA 09837The small bipolar group was marked at the low latitudes since 20.02 to 28.02.02. In the first days the total region's area reached 150 m.s.h. The head sunspot with asymmetrical penumbra was gradually bifurcating and decaying.
 
NOAA 09838The fine bipolar sunspots were observed at the Sun equator since 21.02 to 23.02.02, in the Western part of the Sun disc.
 
NOAA 09839The growing bipolar group was observed at the mid latitudes of the Southern hemisphere since 20.02 to 28.02.02. The group consisted of many small sunspots which were regular changing the combination. Before set for the limb the total bipole's area reached 250 m.s.h.
 
NOAA 09840The recurrent sunspot with symmetrical penumbra was marked at the tenth parallel of the Southern hemisphere since 21.02 to 4.03.02.
 
NOAA 09841The fine bipolar group was noticed to the East from the big region 09830 since 22.02 to 26.02.02.
 
NOAA 09842The growing bipolar group was observed at the high latitudes of the Southern hemisphere since 22.02 to 1.03.02. Before set for the limb the total bipole's area reached 250 m.s.h.
 
NOAA 09843The fine bipolar sunspots crossed the Sun disc since 22.02 to 5.03.02 along the 26th parallel of the Southern hemisphere.
 
NOAA 09844The bipolar combination of many small sunspots was observed at the high latitudes of the Northern hemisphere since 23.02 to 4.03.02. The sunspot's quantity, the sunspot's form and the sunspot's combination had regular changes. The total region's area reached 150-200 m.s.h., and it was counted 20-25 sunspots in the group.
 
NOAA 09845The big bipolar group crossed the Sun disc since 23.02 to 7.03.02 along the mid latitudes of the Northern hemisphere. In the first days the group consisted of three parts: the small head sunspot with symmetrical penumbra, and two tail sunspots with asymmetrical penumbraes which were connected by a short chain of pores. In next days the tail sunspots began extend and dispersed. Many fine sunspots with penumbraes appeared at the head sunspot's place. In the evolution's peak the total region's area reached 500 m.s.h., and it was counted 25-30 sunspots in the group.
 
NOAA 09846The growing bipolar group was observed at the low latitudes of the Southern hemisphere since 22.02 to 28.02.02, in the Western part of the Sun disc. Before set for the limb the total region area reached 200 m.s.h.
 
NOAA 09847The small bipolar group was decaying ath the mid latitudes of the Southern hemisphere since 24.02 to 2.03.02, in the Eastern part of the Sun disc.
 
NOAA 09848The fine bipolar sunspots were noticed since 25.02 to 3.03.02 hardly to the South-West from the region 09847.
 
NOAA 09849The fine high latitude sunspots were noticed in the Northern hemisphere on 25.02 and 26.02.02, near the Eastern limb.
 
NOAA 09850The fine sunspots were observed at the 27th parallel of the Northern hemisphere since 27.02 to 1.03.02, not far from the Western limb.
 
NOAA 09851The long chain of fine sunspots crossed the Sun disc since 28.02 to 11.03.02 along the low latitudes of the Southern hemisphere. From time to time the total region's area reached 100 m.s.h.
 
NOAA 09852The short-time pore was noticed on 1.03 and 2.03.02 in the Eastern part of the Sun disc.
 
NOAA 09853The decaying bipolar sunspots were observed at the 24th parallel of the Southern hemisphere since 2.03 to 10.03.02.
 
NOAA 09854The short-time bipolar sunspots were marked at the tenth parallel of the Northern hemisphere since 2.03 to 4.03.02, neighbouring the central meridian.
 
NOAA 09855The short-time bipolar sunspots were observed at the mid latitudes of the Northern hemisphere on 3.03 and 4.03.02, to the East from the central meridian.
 
NOAA 09856The perceptible sunspot with oblong penumbra crossed the Sun disc since 3.03 to 15.03.02 along the low latitudes of the Southern hemisphere. From time to time pores with opposite magnetic polarity were observed neighbouring the sunspot. The total region's area reached 200 m.s.h.
 
NOAA 09857The fine sunspots were noticed since 4.03 to 6.03.02 near the Western limb.
 
NOAA 09858The short-time bipolar formation was marked at the thirtieth parallel of the Southern hemisphere since 4.03 to 6.03.02, neighbouring the central meridian.
 
NOAA 09859The insignificant bipolar formation was observed to the South-West from the sunspot 09856 since 2.03 to 14.03.02.
 
NOAA 09860The fine recurrent sunspots were observed on 5.03 and 6.03.02 at the Eastern limb, and 14.03 and 15.03 - not far from the Western limb.
 
NOAA 09861The fine sunspot with symmetrical penumbra was noticed at the Eastern limb since 5.03 to 7.03.02.
 
NOAA 09862The new bipolar group was observed at the Western limb since 6.03 to 8.03.02. The main sunspot had symmetrical penumbra.
 
NOAA 09863The recurrent pores were noticed at the high latitudes of the Northern hemisphere since 3.03 to 8.03.02.
 
NOAA 09864The small sunspot with symmetrical penumbra was observed at the high latitudes of the Northern hemisphere since 7.03 to 19.03.02. From time to time fine tail sunspots with opposite magnetic polarity were marked.
 
NOAA 09865The fine sunspot was marked at the mid latitudes of the Northern hemisphere since 8.03 to 12.03.02, in the Eastern part of the Sun disc.
 
NOAA 09866The big bipolar group crossed the Sun disc since 8.03 to 22.03.02 along the tenth parallel of the Southern hemisphere. The head and tail parts of the group consisted of large sunspots with powerful penumbraes, and space between its was free for sunspots. In the first days the total region's area reached 1000 m.s.h.
 
NOAA 09867The short-time high latitude pores were observed in the Southern hemisphere since 10.03 to 12.03.02, to the East from the central meridian.
 
NOAA 09868The fine bipolar group was noticed at the high latitudes of the Southern hemisphere since 11.03 to 16.03.02.
 
NOAA 09969The short-time pores were marked at the 24th parallel of the Southern hemisphere since 11.03 to 15.03.02, in the Eastern part of the Sun disc.
 
NOAA 09970The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 10.03 to 22.03.02 along the high latitudes of the Southern hemisphere. The fine tail sunspots were settled from the head sunspot on the considerable distance. The total region's area reached 150 m.s.h.
 
NOAA 09971The opened bipolar group crossed the Sun disc since 13.03 to 25.03.02 along the high latitudes of the Southern hemisphere. The bipole consisted of two sunspots with symmetrical penumbraes. In the first days the tail sunspot was perceptibly more than the head sunspot. But the leading sunspot was gradually extending with siimultaneous curtailment of the supporting sunspot. The total region's area reached 300 m.s.h. Fine sunspots and pores appeared and disappeared neighbouring the main sunspots.
 
NOAA 09972The fine bipolar group was noticed at the 31st parallel of the Southern hemisphere since 14.03 to 19.03.02.
 
NOAA 09973The small bipolar group was marked at the mid latitudes of the Southern hemisphere since 16.03 to 23.03.02. In the first days the total region's area reached 100 m.s.h.
 
NOAA 09974The insignificant sunspots were observed at the mid latitudes of the Northern hemisphere since 15.03 to 22.03.02.
 
NOAA 09975The decaying bipolar group crossed the Sun disc since 19.03 to 28.03.02 along the high latitudes of the Southern hemisphere. In the first days the total region's area reached 150 m.s.h.
 
NOAA 09976The spreading bipolar group crossed the Sun disc since 19.03 to 1.04.02 along the mid latitudes of the Southern hemisphere. The total region's area reached 200 m.s.h., and it was counted 25-30 sunspots in the group.
 
NOAA 09977The new bipolar group was observed at the mid latitudes of the Northern hemisphere since 20.03 to 23.03.02, in the Western part of the Sun disc.
 
NOAA 09978The bipolar chain of small sunspots crossed the Sun disc since 20.03 to 1.04.02 along the low latitudes of the Northern hemisphere. The total region's area reached 150 m.s.h.
 
NOAA 09979The new bipolar group was noticed since 21.03 to 24.03.02 near the Western limb.
 
NOAA 09980The new eruptive group had appeared at the low latitudes of the Northern hemisphere on 20.03.02, in the Eastern part of the Sun disc. In the first days the group did not display perceptible activity. On 27.03 the new bipole began extend. In two days the total region's area exceeded 300 m.s.h. On 30.03 the new group reached the Western limb.
 
NOAA 09881The small bipolar group was observed at the low latitudes of the Southern hemisphere since 22.03 to 28.03.02, in the Western part of the Sun disc. The tail sunspot had developed penumbra. The total region's area reached 150 m.s.h.
 
NOAA 09882The fine bipolar group was noticed at the mid latitudes of the Northern hemisphere since 22.03 to 27.03.02, in the Eastern part of the Sun disc.
 
NOAA 09883The small sunspot with symmetrical penumbra was observed at the low latitudes of the Northern hemisphere since 23.03 to 30.03.02, in the Eastern part of the Sun disc.
 
NOAA 09884The small bipolar group was observed at the mid latitudes of the Southern hemisphere since 27.03 to 6.04.02. From time to time the total region's area reached 100 m.s.h.
 
NOAA 09885The big bipolar group crossed the Sun disc since 27.03 to 8.04.02 along the mid latitudes of the Northern hemisphere. The group consisted of developed head and tail sunspots which were connected by long and solid chain of more fine sunspots. Neighbouring the central meridian the total region's area exceeded 700 m.s.h., and it was counted more 30 sunspots in the group.
 
NOAA 09886The perceptible bipolar group was situated between the big regions 09885 and 09887 since 29.03 to 8.04.02. The total region's area reached 100-150 m.s.h., and it was counted more twenty sunspots in the group.
 
NOAA 09887The multipolar sunspot's development was observed at the Sun equator since 29.03 to 10.04.02. The group's extension began in the head sunspot, and then it enveloped all the group. Neighbouring the central meridian the total region's area had exceeded 700 m.s.h. In next days slow collapse of the multipolar structure was outlined.
 
NOAA 09888The perceptible bipolar group crossed the Sun disc since 29.03 to 10.04.02 along the mid latitudes of the Southern hemisphere. The bipole consisted of the developed head sunspot with asymmetrical penumbra and gradually decaying tail sunspots. The total region's area exceeded 200 m.s.h.
 
NOAA 09889The fine sunspots were noticed since 30.03 to 4.04.02 to the South from the bipolar region 09888.
 
NOAA 09890The one-day pore was observed on 2.04.02 to the North-West from the bipolar region 09884.
 
NOAA 09891The short-time pores were marked on 2.04 and 3.04.02 in the Sun disc's center.
 
NOAA 09892The fine bipolar group was noticed at the low latitudes of the Northern hemisphere since 2.04 to 8.04.02, in the Eastern part of the Sun disc.
 
NOAA 09893The long multipolar chain crossed the Sun disc since 3.04 to 16.04.02 along the high latitudes of the Northern hemisphere. The group consisted of the large head sunspots and string of more fine sunspots. The total region's area reached 500 m.s.h., and it was counted more 30 sunspots in the group.
 
NOAA 09894The short-time sunspots were observed at the mid latitudes of the Northern hemisphere since 4.04 to 6.04.02, neighbouring the central meridian.
 
NOAA 09895The short-time pores were marked since 4.04 to 6.04.02 near the Eastern limb.
 
NOAA 09896The small sunspot with symmetrical penumbra crossed the Sun disc since 5.04 to 17.04.02 along the tenth parallel of the Southern hemisphere.
 
NOAA 09897The fine bipolar group was observed at the Sun equator since 6.04 to 11.04.02, in the Western part of the Sun disc.
 
NOAA 09898The fine bipolar sunspots were noticed since 5.04 to 11.04.02 hardly to the South from the sunspot 09896.
 
NOAA 09899The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 6.04 to 18.04.02 along the high latitudes of the Northern hemisphere. Fine sunspots and pores with opposite magnetic polarity were observed neighbouring the sunspot. The total region's area reached 200-300 m.s.h.
 












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