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Observations of solar pulsations

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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Bibliographic Details
Published in:Nature (London) 1976-01, Vol.259 (5539), p.87-89
Main Authors: Severny, A. B., Kotov, V. A., Tsap, T. T.
Format: Article
Language:English
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Summary: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.
ISSN:0028-0836
1476-4687
DOI:10.1038/259087a0