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Structure of the 5-minute solar oscillations 1976–1980

  • The Sun:Structure Oscillations, Magnetic Cycle, Surface Variations
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Abstract

The discrete structure in the 5 min velocity oscillations of the solar surface has been confirmed by a re-analysis of data obtained between 1976 and 1979, and in addition a preliminary analysis of 1980 data show excellent consistency of the determined frequencies over the five year period. It is further shown that atmospheric transparency, as measured by the power in the solar intensity fluctuations, shows no correlation with the measured amplitude of the velocity fluctuations, over 2 orders of magnitude.

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References

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Authors and Affiliations

  1. University of Birmingham, UK

    A. Claverie, G. R. Isaak, C. P. McLeod & H. B. Van Der Raay

  2. Instituto de Astrofisica de Canarias, La Laguna, Spain

    T. Roca Cortès

Authors
  1. A. Claverie
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  2. G. R. Isaak
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  3. C. P. McLeod
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  4. H. B. Van Der Raay
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  5. T. Roca Cortès
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Additional information

Proceedings of the 14th ESLAB Symposium on Physics of Solar Variations, 16–19 September 1980, Scheveningen, The Netherlands.

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Claverie, A., Isaak, G.R., McLeod, C.P. et al. Structure of the 5-minute solar oscillations 1976–1980. Sol Phys 74, 51–57 (1981). https://doi.org/10.1007/BF00151273

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  • DOI: https://doi.org/10.1007/BF00151273

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