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Rotational Splitting of ℓ=1 Modes

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Seismology of the Sun and the Distant Stars

Part of the book series: NATO ASI Series ((ASIC,volume 169))

Abstract

An analysis of the amplitude modulation of specific ℓ=1 p modes, has revealed a mean splitting of 0.74 µHz over the frequency range 2.4 to 4.0 mHz. The effects of large scale surface phenomena rotating at the −27 day surface rotation rate are also detected. The lifetime of the ℓ=1 modes is seen to vary from ›120 days at 2425.1 µHz to −50 days at 3912.2 µHz.

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References

  1. J.R. Brookes, G.R. Isaak and H.B. van der Raay, Mon. Not. R. astr Soc. 185 (1978) 1

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  2. H.B. van der Raay, P.L. Palle and T. Roca Cortez, Loc.sit.

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Author information

Authors and Affiliations

  1. Department of Physics, University of Birmingham, UK

    H. B. van der Raay

  2. I. A.C., Universidad de la Laguna, Tenerife, Spain

    P. L. Palle & T. Roca Cortez

Authors
  1. H. B. van der Raay
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  2. P. L. Palle
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  3. T. Roca Cortez
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Editor information

Editors and Affiliations

  1. Institute of Astronomy and Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Cambridge, UK

    D. O. Gough

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© 1986 D. Reidel Publishing Company, Dordrecht, Holland

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van der Raay, H.B., Palle, P.L., Roca Cortez, T. (1986). Rotational Splitting of ℓ=1 Modes. In: Gough, D.O. (eds) Seismology of the Sun and the Distant Stars. NATO ASI Series, vol 169. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4608-8_20

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  • DOI: https://doi.org/10.1007/978-94-009-4608-8_20

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-8547-2

  • Online ISBN: 978-94-009-4608-8

  • eBook Packages: Springer Book Archive

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