The influence of planetary attractions on the solar tachocline

Autores
Callebaut, Dirk K.; de Jager, Cornelis; Duhau, Silvia Noemi C.
Año de publicación
2012
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present a physical analysis of the occasionally forwarded hypothesis that solar variability, as shown in the various photospheric and outer solar layer activities, might be due to the Newtonian attraction by the planets. We calculate the planetary forces exerted on the tachocline and thereby not only include the immediate forces but we also take into account that these planetary or dynamo actions occur during some time, which demands integration. As an improvement to earlier research on this topic we reconsider the internal convective velocities and we examine several other effects, in particular those due to magnetic buoyancy and to the Coriolis force. The main conclusion is that in its essence: planetary influences are too small to be more than a small modulation of the solar cycle. We do not exclude the possibility that the long term combined action of the planets may induce small internal motions in the sun, which may have indirectly an effect on the solar dynamo after a long time.
Fil: Callebaut, Dirk K.. Universiteit Antwerp; Bélgica
Fil: de Jager, Cornelis. Royal Netherlands Institute for Sea Research; Países Bajos
Fil: Duhau, Silvia Noemi C.. Universidad de Buenos Aires. Facultad de Ingeniería. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Materia
DYNAMO
PLANETARY ATTRACTIONS
SOLAR VARIABILITY
TACHOCLINE
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/139031
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/139031
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling The influence of planetary attractions on the solar tachoclineCallebaut, Dirk K.de Jager, CornelisDuhau, Silvia Noemi C.DYNAMOPLANETARY ATTRACTIONSSOLAR VARIABILITYTACHOCLINEhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present a physical analysis of the occasionally forwarded hypothesis that solar variability, as shown in the various photospheric and outer solar layer activities, might be due to the Newtonian attraction by the planets. We calculate the planetary forces exerted on the tachocline and thereby not only include the immediate forces but we also take into account that these planetary or dynamo actions occur during some time, which demands integration. As an improvement to earlier research on this topic we reconsider the internal convective velocities and we examine several other effects, in particular those due to magnetic buoyancy and to the Coriolis force. The main conclusion is that in its essence: planetary influences are too small to be more than a small modulation of the solar cycle. We do not exclude the possibility that the long term combined action of the planets may induce small internal motions in the sun, which may have indirectly an effect on the solar dynamo after a long time.Fil: Callebaut, Dirk K.. Universiteit Antwerp; BélgicaFil: de Jager, Cornelis. Royal Netherlands Institute for Sea Research; Países BajosFil: Duhau, Silvia Noemi C.. Universidad de Buenos Aires. Facultad de Ingeniería. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaElsevier2012-05info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/139031Callebaut, Dirk K.; de Jager, Cornelis; Duhau, Silvia Noemi C.; The influence of planetary attractions on the solar tachocline; Elsevier; Journal of Atmospheric and Solar-Terrestrial Physics; 80; 5-2012; 73-781364-6826CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1016/j.jastp.2012.03.005info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/abs/pii/S1364682612000892info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:55:47Zoai:ri.conicet.gov.ar:11336/139031instacron: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 09:55:47.415CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The influence of planetary attractions on the solar tachocline
title The influence of planetary attractions on the solar tachocline
spellingShingle The influence of planetary attractions on the solar tachocline
Callebaut, Dirk K.
DYNAMO
PLANETARY ATTRACTIONS
SOLAR VARIABILITY
TACHOCLINE
title_short The influence of planetary attractions on the solar tachocline
title_full The influence of planetary attractions on the solar tachocline
title_fullStr The influence of planetary attractions on the solar tachocline
title_full_unstemmed The influence of planetary attractions on the solar tachocline
title_sort The influence of planetary attractions on the solar tachocline
dc.creator.none.fl_str_mv Callebaut, Dirk K.
de Jager, Cornelis
Duhau, Silvia Noemi C.
author Callebaut, Dirk K.
author_facet Callebaut, Dirk K.
de Jager, Cornelis
Duhau, Silvia Noemi C.
author_role author
author2 de Jager, Cornelis
Duhau, Silvia Noemi C.
author2_role author
author
dc.subject.none.fl_str_mv DYNAMO
PLANETARY ATTRACTIONS
SOLAR VARIABILITY
TACHOCLINE
topic DYNAMO
PLANETARY ATTRACTIONS
SOLAR VARIABILITY
TACHOCLINE
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We present a physical analysis of the occasionally forwarded hypothesis that solar variability, as shown in the various photospheric and outer solar layer activities, might be due to the Newtonian attraction by the planets. We calculate the planetary forces exerted on the tachocline and thereby not only include the immediate forces but we also take into account that these planetary or dynamo actions occur during some time, which demands integration. As an improvement to earlier research on this topic we reconsider the internal convective velocities and we examine several other effects, in particular those due to magnetic buoyancy and to the Coriolis force. The main conclusion is that in its essence: planetary influences are too small to be more than a small modulation of the solar cycle. We do not exclude the possibility that the long term combined action of the planets may induce small internal motions in the sun, which may have indirectly an effect on the solar dynamo after a long time.
Fil: Callebaut, Dirk K.. Universiteit Antwerp; Bélgica
Fil: de Jager, Cornelis. Royal Netherlands Institute for Sea Research; Países Bajos
Fil: Duhau, Silvia Noemi C.. Universidad de Buenos Aires. Facultad de Ingeniería. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
description We present a physical analysis of the occasionally forwarded hypothesis that solar variability, as shown in the various photospheric and outer solar layer activities, might be due to the Newtonian attraction by the planets. We calculate the planetary forces exerted on the tachocline and thereby not only include the immediate forces but we also take into account that these planetary or dynamo actions occur during some time, which demands integration. As an improvement to earlier research on this topic we reconsider the internal convective velocities and we examine several other effects, in particular those due to magnetic buoyancy and to the Coriolis force. The main conclusion is that in its essence: planetary influences are too small to be more than a small modulation of the solar cycle. We do not exclude the possibility that the long term combined action of the planets may induce small internal motions in the sun, which may have indirectly an effect on the solar dynamo after a long time.
publishDate 2012
dc.date.none.fl_str_mv 2012-05
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/11336/139031
Callebaut, Dirk K.; de Jager, Cornelis; Duhau, Silvia Noemi C.; The influence of planetary attractions on the solar tachocline; Elsevier; Journal of Atmospheric and Solar-Terrestrial Physics; 80; 5-2012; 73-78
1364-6826
CONICET Digital
CONICET
url http://hdl.handle.net/11336/139031
identifier_str_mv Callebaut, Dirk K.; de Jager, Cornelis; Duhau, Silvia Noemi C.; The influence of planetary attractions on the solar tachocline; Elsevier; Journal of Atmospheric and Solar-Terrestrial Physics; 80; 5-2012; 73-78
1364-6826
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1016/j.jastp.2012.03.005
info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/abs/pii/S1364682612000892
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 Elsevier
publisher.none.fl_str_mv Elsevier
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
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score 13.070432

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