On the 160-MINUTE Oscillation
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±0.01 minute period, which can be interpreted as a g-mode.
Palle, P. L. et al.
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1988