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Observations of solar pulsations

Abstract

We have modified our solar magnetograph to measure velocities at the solar surface, rather than magnetic fields. Using this apparatus, we have observed fluctuations of period 2 h 40 min, which are remarkably stable. The interpretation of this phenomenon seems to cause much theoretical difficulty.

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Severny, A., Kotov, V. & Tsap, T. Observations of solar pulsations. Nature 259, 87–89 (1976). https://doi.org/10.1038/259087a0

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  • DOI: https://doi.org/10.1038/259087a0

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