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dc.date.accessioned 2019-10-28T13:15:53Z
dc.date.available 2019-10-28T13:15:53Z
dc.date.issued 2011
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/84144
dc.description.abstract Recently, Wolff & Patrone (2010), have developed a simple but very interesting model by which the movement of the Sun around the barycentre of the Solar system could create potential energy that could be released by flows pre-existing inside the Sun. The authors claim that it is the first mechanism showing how planetary movements can modify internal structure in the Sun that can be related to solar cycle. In this work we point out limitations of mentioned mechanism (which is based on interchange arguments), which could be inapplicable to a real star. Then, we calculate the temporal evolution of potential energy stored in zones of Sun's interior in which the potential energy could be most efficiently stored taking into account detailed barycentric Sun dynamics. We show strong variations of potential energy related to Maunder Minimum, Dalton Minimum and the maximum of Cycle 22, around 1990. We discuss briefly possible implications of this putative mechanism to solar cycle specially Grand Minima events. en
dc.format.extent 410-413 es
dc.language en es
dc.subject Sun: activity es
dc.subject sunspots es
dc.subject Sun: interior es
dc.title Potential energy stored by planets and grand minima events en
dc.type Articulo es
sedici.identifier.other doi:10.1017/S1743921312005157 es
sedici.identifier.other eid:2-s2.0-84864374244 es
sedici.identifier.issn 1743-9213 es
sedici.creator.person Cionco, Rodolfo Gustavo es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.event IAU Symposium 286 (Mendoza, Argentina, 3-7 October, 2011) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Proceedings of the International Astronomical Union es
sedici.relation.journalVolumeAndIssue vol. 7, no. S286 es
sedici.rights.sherpa * Color: verde* Pre-print del autor: si* Post-print del autor: si* Versión de editor/PDF:no* Condiciones:>>Author's Pre-print on author's personal website, departmental website, social media websites, institutional repository, non-commercial subject-based repositories, such as PubMed Central, Europe PMC or arXiv>>Author's post-print on author's personal website on acceptance of publication>>Author's post-print on departmental website, institutional repository, non-commercial subject-based repositories, such as PubMed Central, Europe PMC or arXiv, after a 6 months embargo>>La versión de editor/PDF no puede utilizarse>>Published abstract may be deposited>>El pre-print debe registrar la aceptación para su publicación>>Deben reconocerse el copyright y la fuente editorial>>Must link to publisher version or journal website>>Authors may choose to use a Creative Commons Attribution Non-Commercial No Derivatives License>>Publisher last reviewed on 09/10/2014* Link a Sherpa: http://sherpa.ac.uk/romeo/issn/1743-9213/es/


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)