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Parametrizing the time variation of the `surface term' of stellar p-mode frequencies: application to helioseismic data

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Ball,  W. H.
Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society;

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Howe, R., Basu, S., Davies, G. R., Ball, W. H., Chaplin, W. J., Elsworth, Y., et al. (2016). Parametrizing the time variation of the `surface term' of stellar p-mode frequencies: application to helioseismic data. Mon. Not. Roy. Astron. Soc., 464, 4777-4788. doi:10.1093/mnras/stw2668.


Cite as: http://hdl.handle.net/11858/00-001M-0000-002C-C1BD-D
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