Show simple item record New, R. Pintér, Balázs Erdélyi, R. 2008-12-04T16:46:29Z 2008-12-04T16:46:29Z 2001-10-15
dc.identifier.citation New , R , Pintér , B & Erdélyi , R 2001 , ' Rotational splitting of helioseismic modes influenced by a magnetic atmosphere ' Astronomy and Astrophysics , vol 378 , no. 1 , pp. 1-4 . DOI: 10.1051/0004-6361:20011061 en
dc.identifier.issn 0004-6361
dc.identifier.other PURE: 90336
dc.identifier.other PURE UUID: 39f93df3-468f-46b7-b6bf-6bbb1673c43f
dc.identifier.other dspace: 2160/1384
dc.identifier.other DSpace_20121128.csv: row: 1172
dc.identifier.other Scopus: 0035471520
dc.description Pintér, B.; New, R.; Erdélyi, R., (2001) 'Rotational splitting of helioseismic modes influenced by a magnetic atmosphere', Astronomy and Astrophysics 378 pp.1-4 RAE2008 en
dc.description.abstract In the present paper the splitting of sectoral () 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, . We work with , 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 4 en
dc.language.iso eng
dc.relation.ispartof Astronomy and Astrophysics en
dc.rights en
dc.subject Sun: helioseismology en
dc.subject Sun: oscillations en
dc.subject Sun: interior en
dc.subject Sun: atmosphere en
dc.subject Sun: magnetic fields en
dc.subject Sun: rotation en
dc.title Rotational splitting of helioseismic modes influenced by a magnetic atmosphere en
dc.type /dk/atira/pure/researchoutput/researchoutputtypes/contributiontojournal/article en
dc.contributor.institution Department of Physics en
dc.contributor.institution Mathematics and Physics en
dc.description.status Peer reviewed en

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