On the 160 Minute Oscillation
Solar velocity data collected at Izafia (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.
KeywordsPeculiar Behaviour Annual Series Resonant Scattering Integrate Power Harmonic Degree
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- (4).PallS P.L.; Ph.D. Thesis; (1986); Universidad de La Laguna. Spain.Google Scholar