Rotational splitting of helioseismic modes influenced by a magnetic atmosphere

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dc.contributor.author Pintér, Balázs
dc.contributor.author New, R.
dc.contributor.author Erdélyi, R.
dc.date.accessioned 2007-10-11T09:38:21Z
dc.date.available 2007-10-11T09:38:21Z
dc.date.issued 2001-10
dc.identifier.citation Pintér, B.; New, R.; Erdélyi, R., Rotational splitting of helioseismic modes influenced by a magnetic atmosphere, Astronomy and Astrophysics, v.378, p.L1-L4 (2001) en
dc.identifier.uri http://hdl.handle.net/2160/340
dc.description.abstract In the present paper the splitting of sectoral (m=+/- l) helioseismic eigenmodes (f- and p-modes) is studied in the presence of a magnetic atmosphere. The solar interior is in a steady state, with sub-photospheric plasma flow along the equator representing solar rotation. The Cartesian geometry employed restricts the present study to sectoral modes, m=+/- l. We work with l >= 50, which guarantees that the modes do not deeply penetrate into the solar interior and therefore experience an approximately uniform rotation. Potentially observable effects are predicted and developments of the model to aid detections are discussed. en
dc.format.extent 271448 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher EDP Sciences en
dc.relation.isreferencedby http://www.aanda.org/ en
dc.title Rotational splitting of helioseismic modes influenced by a magnetic atmosphere en
dc.type Text en
dc.type.publicationtype refereed published journal paper en
dc.identifier.duplicate True


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