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)


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.


Peculiar Behaviour Annual Series Resonant Scattering Integrate Power Harmonic Degree 
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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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