Topological Analysis of Emerging Bipole Clusters Producing Violent Solar Events

During the rising phase of Solar Cycle 24 tremendous activity occurred on the Sun with rapid and compact emergence of magnetic flux leading to bursts of flares (C to M and even X-class). We investigate the violent events occurring in the cluster of two active regions (ARs), NOAA numbers 11121 and 11...

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Autores principales: Mandrini, C.H., Schmieder, B., Démoulin, P., Guo, Y., Cristiani, G.D.
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00380938_v289_n6_p2041_Mandrini
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spelling todo:paper_00380938_v289_n6_p2041_Mandrini2023-10-03T14:48:50Z Topological Analysis of Emerging Bipole Clusters Producing Violent Solar Events Mandrini, C.H. Schmieder, B. Démoulin, P. Guo, Y. Cristiani, G.D. Sun: filament eruptions Sun: flares Sun: magnetic fields During the rising phase of Solar Cycle 24 tremendous activity occurred on the Sun with rapid and compact emergence of magnetic flux leading to bursts of flares (C to M and even X-class). We investigate the violent events occurring in the cluster of two active regions (ARs), NOAA numbers 11121 and 11123, observed in November 2010 with instruments onboard the Solar Dynamics Observatory and from Earth. Within one day the total magnetic flux increased by 70 % with the emergence of new groups of bipoles in AR 11123. From all the events on 11 November, we study, in particular, the ones starting at around 07:16 UT in GOES soft X-ray data and the brightenings preceding them. A magnetic-field topological analysis indicates the presence of null points, associated separatrices, and quasi-separatrix layers (QSLs) where magnetic reconnection is prone to occur. The presence of null points is confirmed by a linear and a non-linear force-free magnetic-field model. Their locations and general characteristics are similar in both modelling approaches, which supports their robustness. However, in order to explain the full extension of the analysed event brightenings, which are not restricted to the photospheric traces of the null separatrices, we compute the locations of QSLs. Based on this more complete topological analysis, we propose a scenario to explain the origin of a low-energy event preceding a filament eruption, which is accompanied by a two-ribbon flare, and a consecutive confined flare in AR 11123. The results of our topology computation can also explain the locations of flare ribbons in two other events, one preceding and one following the ones at 07:16 UT. Finally, this study provides further examples where flare-ribbon locations can be explained when compared to QSLs and only, partially, when using separatrices. © 2013 Springer Science+Business Media Dordrecht. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00380938_v289_n6_p2041_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 Sun: filament eruptions
Sun: flares
Sun: magnetic fields
spellingShingle Sun: filament eruptions
Sun: flares
Sun: magnetic fields
Mandrini, C.H.
Schmieder, B.
Démoulin, P.
Guo, Y.
Cristiani, G.D.
Topological Analysis of Emerging Bipole Clusters Producing Violent Solar Events
topic_facet Sun: filament eruptions
Sun: flares
Sun: magnetic fields
description During the rising phase of Solar Cycle 24 tremendous activity occurred on the Sun with rapid and compact emergence of magnetic flux leading to bursts of flares (C to M and even X-class). We investigate the violent events occurring in the cluster of two active regions (ARs), NOAA numbers 11121 and 11123, observed in November 2010 with instruments onboard the Solar Dynamics Observatory and from Earth. Within one day the total magnetic flux increased by 70 % with the emergence of new groups of bipoles in AR 11123. From all the events on 11 November, we study, in particular, the ones starting at around 07:16 UT in GOES soft X-ray data and the brightenings preceding them. A magnetic-field topological analysis indicates the presence of null points, associated separatrices, and quasi-separatrix layers (QSLs) where magnetic reconnection is prone to occur. The presence of null points is confirmed by a linear and a non-linear force-free magnetic-field model. Their locations and general characteristics are similar in both modelling approaches, which supports their robustness. However, in order to explain the full extension of the analysed event brightenings, which are not restricted to the photospheric traces of the null separatrices, we compute the locations of QSLs. Based on this more complete topological analysis, we propose a scenario to explain the origin of a low-energy event preceding a filament eruption, which is accompanied by a two-ribbon flare, and a consecutive confined flare in AR 11123. The results of our topology computation can also explain the locations of flare ribbons in two other events, one preceding and one following the ones at 07:16 UT. Finally, this study provides further examples where flare-ribbon locations can be explained when compared to QSLs and only, partially, when using separatrices. © 2013 Springer Science+Business Media Dordrecht.
format JOUR
author Mandrini, C.H.
Schmieder, B.
Démoulin, P.
Guo, Y.
Cristiani, G.D.
author_facet Mandrini, C.H.
Schmieder, B.
Démoulin, P.
Guo, Y.
Cristiani, G.D.
author_sort Mandrini, C.H.
title Topological Analysis of Emerging Bipole Clusters Producing Violent Solar Events
title_short Topological Analysis of Emerging Bipole Clusters Producing Violent Solar Events
title_full Topological Analysis of Emerging Bipole Clusters Producing Violent Solar Events
title_fullStr Topological Analysis of Emerging Bipole Clusters Producing Violent Solar Events
title_full_unstemmed Topological Analysis of Emerging Bipole Clusters Producing Violent Solar Events
title_sort topological analysis of emerging bipole clusters producing violent solar events
url http://hdl.handle.net/20.500.12110/paper_00380938_v289_n6_p2041_Mandrini
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AT schmiederb topologicalanalysisofemergingbipoleclustersproducingviolentsolarevents
AT demoulinp topologicalanalysisofemergingbipoleclustersproducingviolentsolarevents
AT guoy topologicalanalysisofemergingbipoleclustersproducingviolentsolarevents
AT cristianigd topologicalanalysisofemergingbipoleclustersproducingviolentsolarevents
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