Evolution of a very complex active region during the decay phase of Cycle 23

We study the emergence and evolution of AR NOAA 10314, observed on the solar disk during March 13-19, 2003. This extremely complex AR is of particular interest due to its unusual magnetic flux distribution and the clear rotation of the polarities of a d-spot within the AR. Using SOHO/MDI magnetogram...

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Autores principales: Poisson, M., Fuentes, M.L., Mandrini, C.H., Démoulin, P., Pariat, E.
Formato: SER
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_17439213_v7_nS286_p246_Poisson
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spelling todo:paper_17439213_v7_nS286_p246_Poisson2023-10-03T16:31:40Z Evolution of a very complex active region during the decay phase of Cycle 23 Poisson, M. Fuentes, M.L. Mandrini, C.H. Démoulin, P. Pariat, E. Sun: magnetic fields Sun: photosphere We study the emergence and evolution of AR NOAA 10314, observed on the solar disk during March 13-19, 2003. This extremely complex AR is of particular interest due to its unusual magnetic flux distribution and the clear rotation of the polarities of a d-spot within the AR. Using SOHO/MDI magnetograms we follow the evolution of the photospheric magnetic flux to infer the morphology of the structure that originates the AR. We determine the tilt angle variation for the d-spot and find a counter-clockwise rotation corresponding to a positive writhed flux tube. We compute the magnetic helicity injection and the total accumulated helicity in the AR and find a correlation with the observed rotation. © 2012 International Astronomical Union. Fil:Poisson, M. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Mandrini, C.H. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. SER info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_17439213_v7_nS286_p246_Poisson
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Sun: magnetic fields
Sun: photosphere
spellingShingle Sun: magnetic fields
Sun: photosphere
Poisson, M.
Fuentes, M.L.
Mandrini, C.H.
Démoulin, P.
Pariat, E.
Evolution of a very complex active region during the decay phase of Cycle 23
topic_facet Sun: magnetic fields
Sun: photosphere
description We study the emergence and evolution of AR NOAA 10314, observed on the solar disk during March 13-19, 2003. This extremely complex AR is of particular interest due to its unusual magnetic flux distribution and the clear rotation of the polarities of a d-spot within the AR. Using SOHO/MDI magnetograms we follow the evolution of the photospheric magnetic flux to infer the morphology of the structure that originates the AR. We determine the tilt angle variation for the d-spot and find a counter-clockwise rotation corresponding to a positive writhed flux tube. We compute the magnetic helicity injection and the total accumulated helicity in the AR and find a correlation with the observed rotation. © 2012 International Astronomical Union.
format SER
author Poisson, M.
Fuentes, M.L.
Mandrini, C.H.
Démoulin, P.
Pariat, E.
author_facet Poisson, M.
Fuentes, M.L.
Mandrini, C.H.
Démoulin, P.
Pariat, E.
author_sort Poisson, M.
title Evolution of a very complex active region during the decay phase of Cycle 23
title_short Evolution of a very complex active region during the decay phase of Cycle 23
title_full Evolution of a very complex active region during the decay phase of Cycle 23
title_fullStr Evolution of a very complex active region during the decay phase of Cycle 23
title_full_unstemmed Evolution of a very complex active region during the decay phase of Cycle 23
title_sort evolution of a very complex active region during the decay phase of cycle 23
url http://hdl.handle.net/20.500.12110/paper_17439213_v7_nS286_p246_Poisson
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