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On the 160 Minute Oscillation

  • P. L. Pallé
  • T. Roca Cortés
Conference paper
Part of the International Astronomical Union / Union Astronomique Internationale book series (IAUS, volume 123)

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.

Keywords

Peculiar Behaviour Annual Series Resonant Scattering Integrate Power Harmonic Degree 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

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    Brookes J.R.; Isaak G.R.; van der Raay H.B.; (1976), Nature; 259, 92ADSCrossRefGoogle Scholar
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    Severny A.R.; Kotov V.A.; Tsap T.T.; (1976); Nature. 259,87ADSCrossRefGoogle Scholar
  3. (3).
    Kotov V.A.; Severny A.R.; Tasp T.T.; (1984); Mem. S.A.Tt.. 55, 117ADSGoogle Scholar
  4. (4).
    PallS P.L.; Ph.D. Thesis; (1986); Universidad de La Laguna. Spain.Google Scholar

Copyright information

© International Astronomical Union 1988

Authors and Affiliations

  • P. L. Pallé
    • 1
  • T. Roca Cortés
    • 1
  1. 1.Instituto de Astrofisica de CanariasUniversidad de La LagunaTenerifeSpain

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