Moving magnetic features around a pore

A. J. Kaithakkal et. al.

Detalles Bibliográficos
Autores: Kaithakkal, A. J., Toro, José Carlos del, Orozco Suárez, David, Knölker, M.
Tipo de recurso: artículo
Estado:Versión enviada para evaluación y publicación
Fecha de publicación:2017
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/147520
Acceso en línea:http://hdl.handle.net/10261/147520
Access Level:acceso abierto
Palabra clave:Sun: magnetic fields
Sun: photosphere
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spelling Moving magnetic features around a poreKaithakkal, A. J.Toro, José Carlos delOrozco Suárez, DavidKnölker, M.Sun: magnetic fieldsSun: photosphereA. J. Kaithakkal et. al.©2017 The American Astronomical Society. All rights reserved.Spectropolarimetric observations from Sunrise/IMaX, obtained in 2013 June, are used for a statistical analysis to determine the physical properties of moving magnetic features (MMFs) observed near a pore. MMFs of the same and opposite polarity, with respect to the pore, are found to stream from its border at an average speed of 1.3 km s−1 and 1.2 km s−1, respectively, with mainly same-polarity MMFs found further away from the pore. MMFs of both polarities are found to harbor rather weak, inclined magnetic fields. Opposite-polarity MMFs are blueshifted, whereas same-polarity MMFs do not show any preference for up- or downflows. Most of the MMFs are found to be of sub-arcsecond size and carry a mean flux of ~1.2 × 1017 Mx.The German contribution to Sunrise and its reflight was funded by the Max Planck Foundation, the Strategic Innovations Fund of the President of the Max Planck Society (MPG), DLR, and private donations by supporting members of the Max Planck Society, which is gratefully acknowledged. The Spanish contribution was funded by the Ministerio de Economía y Competitividad under Projects ESP2013-47349-C6 and ESP2014-56169-C6, partially using European FEDER funds. The HAO contribution was partly funded through NASA grant number NNX13AE95G. This work was partly supported by the BK21 plus program through the National Research Foundation (NRF) funded by the Ministry of Education of Korea.Peer reviewedAmerican Astronomical SocietyInstitute of Physics (Great Britain)Max Planck SocietyMinisterio de Economía y Competitividad (España)NASANational Research Foundation of KoreaConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]201720172017info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Preprintinfo:eu-repo/semantics/submittedVersionhttp://hdl.handle.net/10261/147520reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/ESP2013-47349-C6-1-Rinfo:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/ESP2014-56169-C6-1-Rhttps://doi.org/10.3847/1538-4365/229/1/13Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/1475202026-05-22T06:33:51Z
dc.title.none.fl_str_mv Moving magnetic features around a pore
title Moving magnetic features around a pore
spellingShingle Moving magnetic features around a pore
Kaithakkal, A. J.
Sun: magnetic fields
Sun: photosphere
title_short Moving magnetic features around a pore
title_full Moving magnetic features around a pore
title_fullStr Moving magnetic features around a pore
title_full_unstemmed Moving magnetic features around a pore
title_sort Moving magnetic features around a pore
dc.creator.none.fl_str_mv Kaithakkal, A. J.
Toro, José Carlos del
Orozco Suárez, David
Knölker, M.
author Kaithakkal, A. J.
author_facet Kaithakkal, A. J.
Toro, José Carlos del
Orozco Suárez, David
Knölker, M.
author_role author
author2 Toro, José Carlos del
Orozco Suárez, David
Knölker, M.
author2_role author
author
author
dc.contributor.none.fl_str_mv Max Planck Society
Ministerio de Economía y Competitividad (España)
NASA
National Research Foundation of Korea
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Sun: magnetic fields
Sun: photosphere
topic Sun: magnetic fields
Sun: photosphere
description A. J. Kaithakkal et. al.
publishDate 2017
dc.date.none.fl_str_mv 2017
2017
2017
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
Preprint
info:eu-repo/semantics/submittedVersion
format article
status_str submittedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/147520
url http://hdl.handle.net/10261/147520
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv #PLACEHOLDER_PARENT_METADATA_VALUE#
#PLACEHOLDER_PARENT_METADATA_VALUE#
info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/ESP2013-47349-C6-1-R
info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/ESP2014-56169-C6-1-R
https://doi.org/10.3847/1538-4365/229/1/13
Sí
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv American Astronomical Society
Institute of Physics (Great Britain)
publisher.none.fl_str_mv American Astronomical Society
Institute of Physics (Great Britain)
dc.source.none.fl_str_mv reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC
instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str DIGITAL.CSIC. Repositorio Institucional del CSIC
collection DIGITAL.CSIC. Repositorio Institucional del CSIC
repository.name.fl_str_mv
repository.mail.fl_str_mv
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score 15,812429

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