Filament interaction modeled by flux rope reconnection
- Autores
- Török, T.; Chandra, R.; Pariat, E.; Démoulin, Pascal; Schmieder, B.; Aulanier, G.; Linton, M.; Mandrini, Cristina Hemilse
- Año de publicación
- 2011
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Hα observations of solar active region NOAA 10501 on 2003 November 20 revealed a very uncommon dynamic process: during the development of a nearby flare, two adjacent elongated filaments approached each other, merged at their middle sections, and separated again, thereby forming stable configurations with new footpoint connections. The observed dynamic pattern is indicative of “slingshot” reconnection between two magnetic flux ropes. We test this scenario by means of a three-dimensional zero β magnetohydrodynamic simulation, using a modified version of the coronal flux rope model by Titov and Demoulin as the initial condition for the magnetic field. To this end, a ´ configuration is constructed that contains two flux ropes which are oriented side-by-side and are embedded in an ambient potential field. The choice of the magnetic orientation of the flux ropes and of the topology of the potential field is guided by the observations. Quasi-static boundary flows are then imposed to bring the middle sections of the flux ropes into contact. After sufficient driving, the ropes reconnect and two new flux ropes are formed, which now connect the former adjacent flux rope footpoints of opposite polarity. The corresponding evolution of filament material is modeled by calculating the positions of field line dips at all times. The dips follow the morphological evolution of the flux ropes, in qualitative agreement with the observed filaments.
Fil: Török, T.. Université Paris Diderot - Paris 7; Francia
Fil: Chandra, R.. Université Paris Diderot - Paris 7; Francia
Fil: Pariat, E.. Université Paris Diderot - Paris 7; Francia
Fil: Démoulin, Pascal. Université Paris Diderot - Paris 7; Francia
Fil: Schmieder, B.. Université Paris Diderot - Paris 7; Francia
Fil: Aulanier, G.. Université Paris Diderot - Paris 7; Francia
Fil: Linton, M.. Spece Sciences División. Naval Research Laboratory; Estados Unidos
Fil: Mandrini, Cristina Hemilse. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina - Materia
-
Sun - Corona
Sun - Prominences -Filaments
Numerical Methods - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/19621
Ver los metadatos del registro completo
id |
CONICETDig_9c9e5778c14f47debfd121ba95b6e6af |
---|---|
oai_identifier_str |
oai:ri.conicet.gov.ar:11336/19621 |
network_acronym_str |
CONICETDig |
repository_id_str |
3498 |
network_name_str |
CONICET Digital (CONICET) |
spelling |
Filament interaction modeled by flux rope reconnectionTörök, T.Chandra, R.Pariat, E.Démoulin, PascalSchmieder, B.Aulanier, G.Linton, M.Mandrini, Cristina HemilseSun - CoronaSun - Prominences -FilamentsNumerical Methodshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Hα observations of solar active region NOAA 10501 on 2003 November 20 revealed a very uncommon dynamic process: during the development of a nearby flare, two adjacent elongated filaments approached each other, merged at their middle sections, and separated again, thereby forming stable configurations with new footpoint connections. The observed dynamic pattern is indicative of “slingshot” reconnection between two magnetic flux ropes. We test this scenario by means of a three-dimensional zero β magnetohydrodynamic simulation, using a modified version of the coronal flux rope model by Titov and Demoulin as the initial condition for the magnetic field. To this end, a ´ configuration is constructed that contains two flux ropes which are oriented side-by-side and are embedded in an ambient potential field. The choice of the magnetic orientation of the flux ropes and of the topology of the potential field is guided by the observations. Quasi-static boundary flows are then imposed to bring the middle sections of the flux ropes into contact. After sufficient driving, the ropes reconnect and two new flux ropes are formed, which now connect the former adjacent flux rope footpoints of opposite polarity. The corresponding evolution of filament material is modeled by calculating the positions of field line dips at all times. The dips follow the morphological evolution of the flux ropes, in qualitative agreement with the observed filaments.Fil: Török, T.. Université Paris Diderot - Paris 7; FranciaFil: Chandra, R.. Université Paris Diderot - Paris 7; FranciaFil: Pariat, E.. Université Paris Diderot - Paris 7; FranciaFil: Démoulin, Pascal. Université Paris Diderot - Paris 7; FranciaFil: Schmieder, B.. Université Paris Diderot - Paris 7; FranciaFil: Aulanier, G.. Université Paris Diderot - Paris 7; FranciaFil: Linton, M.. Spece Sciences División. Naval Research Laboratory; Estados UnidosFil: Mandrini, Cristina Hemilse. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaIOP Publishing2011-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/19621Török, T.; Chandra, R.; Pariat, E.; Démoulin, Pascal; Schmieder, B.; et al.; Filament interaction modeled by flux rope reconnection; IOP Publishing; Astrophysical Journal; 728; 1; 2-2011; 1-6; 650004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/728/1/65info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/728/1/65/metainfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:16:41Zoai:ri.conicet.gov.ar:11336/19621instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:16:41.295CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Filament interaction modeled by flux rope reconnection |
title |
Filament interaction modeled by flux rope reconnection |
spellingShingle |
Filament interaction modeled by flux rope reconnection Török, T. Sun - Corona Sun - Prominences -Filaments Numerical Methods |
title_short |
Filament interaction modeled by flux rope reconnection |
title_full |
Filament interaction modeled by flux rope reconnection |
title_fullStr |
Filament interaction modeled by flux rope reconnection |
title_full_unstemmed |
Filament interaction modeled by flux rope reconnection |
title_sort |
Filament interaction modeled by flux rope reconnection |
dc.creator.none.fl_str_mv |
Török, T. Chandra, R. Pariat, E. Démoulin, Pascal Schmieder, B. Aulanier, G. Linton, M. Mandrini, Cristina Hemilse |
author |
Török, T. |
author_facet |
Török, T. Chandra, R. Pariat, E. Démoulin, Pascal Schmieder, B. Aulanier, G. Linton, M. Mandrini, Cristina Hemilse |
author_role |
author |
author2 |
Chandra, R. Pariat, E. Démoulin, Pascal Schmieder, B. Aulanier, G. Linton, M. Mandrini, Cristina Hemilse |
author2_role |
author author author author author author author |
dc.subject.none.fl_str_mv |
Sun - Corona Sun - Prominences -Filaments Numerical Methods |
topic |
Sun - Corona Sun - Prominences -Filaments Numerical Methods |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Hα observations of solar active region NOAA 10501 on 2003 November 20 revealed a very uncommon dynamic process: during the development of a nearby flare, two adjacent elongated filaments approached each other, merged at their middle sections, and separated again, thereby forming stable configurations with new footpoint connections. The observed dynamic pattern is indicative of “slingshot” reconnection between two magnetic flux ropes. We test this scenario by means of a three-dimensional zero β magnetohydrodynamic simulation, using a modified version of the coronal flux rope model by Titov and Demoulin as the initial condition for the magnetic field. To this end, a ´ configuration is constructed that contains two flux ropes which are oriented side-by-side and are embedded in an ambient potential field. The choice of the magnetic orientation of the flux ropes and of the topology of the potential field is guided by the observations. Quasi-static boundary flows are then imposed to bring the middle sections of the flux ropes into contact. After sufficient driving, the ropes reconnect and two new flux ropes are formed, which now connect the former adjacent flux rope footpoints of opposite polarity. The corresponding evolution of filament material is modeled by calculating the positions of field line dips at all times. The dips follow the morphological evolution of the flux ropes, in qualitative agreement with the observed filaments. Fil: Török, T.. Université Paris Diderot - Paris 7; Francia Fil: Chandra, R.. Université Paris Diderot - Paris 7; Francia Fil: Pariat, E.. Université Paris Diderot - Paris 7; Francia Fil: Démoulin, Pascal. Université Paris Diderot - Paris 7; Francia Fil: Schmieder, B.. Université Paris Diderot - Paris 7; Francia Fil: Aulanier, G.. Université Paris Diderot - Paris 7; Francia Fil: Linton, M.. Spece Sciences División. Naval Research Laboratory; Estados Unidos Fil: Mandrini, Cristina Hemilse. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina |
description |
Hα observations of solar active region NOAA 10501 on 2003 November 20 revealed a very uncommon dynamic process: during the development of a nearby flare, two adjacent elongated filaments approached each other, merged at their middle sections, and separated again, thereby forming stable configurations with new footpoint connections. The observed dynamic pattern is indicative of “slingshot” reconnection between two magnetic flux ropes. We test this scenario by means of a three-dimensional zero β magnetohydrodynamic simulation, using a modified version of the coronal flux rope model by Titov and Demoulin as the initial condition for the magnetic field. To this end, a ´ configuration is constructed that contains two flux ropes which are oriented side-by-side and are embedded in an ambient potential field. The choice of the magnetic orientation of the flux ropes and of the topology of the potential field is guided by the observations. Quasi-static boundary flows are then imposed to bring the middle sections of the flux ropes into contact. After sufficient driving, the ropes reconnect and two new flux ropes are formed, which now connect the former adjacent flux rope footpoints of opposite polarity. The corresponding evolution of filament material is modeled by calculating the positions of field line dips at all times. The dips follow the morphological evolution of the flux ropes, in qualitative agreement with the observed filaments. |
publishDate |
2011 |
dc.date.none.fl_str_mv |
2011-02 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/19621 Török, T.; Chandra, R.; Pariat, E.; Démoulin, Pascal; Schmieder, B.; et al.; Filament interaction modeled by flux rope reconnection; IOP Publishing; Astrophysical Journal; 728; 1; 2-2011; 1-6; 65 0004-637X CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/19621 |
identifier_str_mv |
Török, T.; Chandra, R.; Pariat, E.; Démoulin, Pascal; Schmieder, B.; et al.; Filament interaction modeled by flux rope reconnection; IOP Publishing; Astrophysical Journal; 728; 1; 2-2011; 1-6; 65 0004-637X CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/728/1/65 info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/728/1/65/meta |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
_version_ |
1844614113693532160 |
score |
13.070432 |