Rotational splitting of helioseismic modes influenced by a magnetic atmosphere

PINTER, B., NEW, R. and ERDELYI, R. (2001). Rotational splitting of helioseismic modes influenced by a magnetic atmosphere. Astronomy and Astrophysics Supplement Series, 378 (1), L1-L4.

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    Abstract

    In the present paper the splitting of sectoral (m = +/- l) helioseismic eigenmodes (f- andp-modes) is studied in the presence of a magnetic atmosphere. The solar interior is in a steady state, with sub-photospheric plasma ow along the equator representing solar rotation. The Cartesian geometry employed restricts the present study to sectoral modes, m = +/- l. We work with l greater than or equal to 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.

    Item Type: Article
    Research Institute, Centre or Group - Does NOT include content added after October 2018: Materials and Engineering Research Institute > Thin Films Research Centre > Nanotechnology Centre for PVD Research
    Page Range: L1-L4
    Depositing User: Ann Betterton
    Date Deposited: 19 May 2010 16:36
    Last Modified: 18 Mar 2021 09:30
    URI: http://shura.shu.ac.uk/id/eprint/2081

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