The distribution of peculiar active regions along two solar cycles
We perform a statistical study of the spatial and temporal distribution of "peculiar" active regions (ARs) along solar cycles 21 and 22. ARs usually appear in the photosphere in the form of bipolar concentrations of magnetic flux, by "peculiar" we mean regions in which the main p...
Guardado en:
Publicado: |
2002
|
---|---|
Materias: | |
Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03796566_v_n477_p27_Mandrini http://hdl.handle.net/20.500.12110/paper_03796566_v_n477_p27_Mandrini |
Aporte de: |
id |
paper:paper_03796566_v_n477_p27_Mandrini |
---|---|
record_format |
dspace |
spelling |
paper:paper_03796566_v_n477_p27_Mandrini2023-06-08T15:40:39Z The distribution of peculiar active regions along two solar cycles Active regions Magnetic fields Solar cycle Geomagnetism Magnetic flux Sun Solar cycles Space research We perform a statistical study of the spatial and temporal distribution of "peculiar" active regions (ARs) along solar cycles 21 and 22. ARs usually appear in the photosphere in the form of bipolar concentrations of magnetic flux, by "peculiar" we mean regions in which the main polarities rotate one around the other along several solar rotations. Our results show that these regions are spatially distributed as usual ARs when no selection on their magnetic flux is applied. When classified according to their flux, the latitudinal distribution of ARs above 1022 Mx closely follow the butterfly diagram; while those with lower flux are more randomly distributed. The number of rotating ARs follow the activity cycle, with a tendency to dual-peak maxima. 2002 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03796566_v_n477_p27_Mandrini http://hdl.handle.net/20.500.12110/paper_03796566_v_n477_p27_Mandrini |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Active regions Magnetic fields Solar cycle Geomagnetism Magnetic flux Sun Solar cycles Space research |
spellingShingle |
Active regions Magnetic fields Solar cycle Geomagnetism Magnetic flux Sun Solar cycles Space research The distribution of peculiar active regions along two solar cycles |
topic_facet |
Active regions Magnetic fields Solar cycle Geomagnetism Magnetic flux Sun Solar cycles Space research |
description |
We perform a statistical study of the spatial and temporal distribution of "peculiar" active regions (ARs) along solar cycles 21 and 22. ARs usually appear in the photosphere in the form of bipolar concentrations of magnetic flux, by "peculiar" we mean regions in which the main polarities rotate one around the other along several solar rotations. Our results show that these regions are spatially distributed as usual ARs when no selection on their magnetic flux is applied. When classified according to their flux, the latitudinal distribution of ARs above 1022 Mx closely follow the butterfly diagram; while those with lower flux are more randomly distributed. The number of rotating ARs follow the activity cycle, with a tendency to dual-peak maxima. |
title |
The distribution of peculiar active regions along two solar cycles |
title_short |
The distribution of peculiar active regions along two solar cycles |
title_full |
The distribution of peculiar active regions along two solar cycles |
title_fullStr |
The distribution of peculiar active regions along two solar cycles |
title_full_unstemmed |
The distribution of peculiar active regions along two solar cycles |
title_sort |
distribution of peculiar active regions along two solar cycles |
publishDate |
2002 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03796566_v_n477_p27_Mandrini http://hdl.handle.net/20.500.12110/paper_03796566_v_n477_p27_Mandrini |
_version_ |
1768543805195157504 |