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On the 160 minute oscillation
Published online by Cambridge University Press: 03 August 2017
Abstract
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