Abstract
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.
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PallS P.L.; Ph.D. Thesis; (1986); Universidad de La Laguna. Spain.
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© 1988 International Astronomical Union
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Pallé, P.L., Roca Cortés, T. (1988). On the 160 Minute Oscillation. In: Christensen-Dalsgaard, J., Frandsen, S. (eds) Advances in Helio- and Asteroseismology. International Astronomical Union / Union Astronomique Internationale, vol 123. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4009-3_15
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DOI: https://doi.org/10.1007/978-94-009-4009-3_15
Publisher Name: Springer, Dordrecht
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