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On the 160 minute oscillation

Published online by Cambridge University Press:  03 August 2017

Pallé P.L.  and
T. Roca Cortés
Pallé P.L.
Affiliation:
Instituto de Astrofisica de Canarias, Universidad de La Laguna, Tenerife, Spain
T. Roca Cortés
Affiliation:
Instituto de Astrofisica de Canarias, Universidad de La Laguna, Tenerife, Spain

Abstract

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Solar velocity data collected at Izaña (Tenerife) over the years 1980–1985 have been used to search for the 160 minute oscillation. The peculiar behaviour of the ninth harmonic of a day, in amplitude and phase, suggests the existence of a solar signal with a 160.02 ± .01 minute period, which can be interpreted as a g-mode.

Type
Chapter 1: Observations of Solar Oscillations
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 75 - 78
Copyright
Copyright © Reidel 1988 

References

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4. Pallé, P.L.; Ph.D. Thesis; (1986); Universidad de La Laguna. Spain.Google Scholar