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Structure of the 5-Minute Solar Oscillations 1976–1980

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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.

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

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© 1981 Springer Science+Business Media Dordrecht

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Claverie, A., Isaak, G.R., McLeod, C.P., Van der Raay, H.B., Cortès, T.R. (1981). Structure of the 5-Minute Solar Oscillations 1976–1980. In: Domingo, V. (eds) Physics of Solar Variations. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-9633-1_7

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  • DOI: https://doi.org/10.1007/978-94-010-9633-1_7

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-9635-5

  • Online ISBN: 978-94-010-9633-1

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