Hostname: page-component-cc8bf7c57-ksm4s Total loading time: 0 Render date: 2024-12-12T04:46:45.099Z Has data issue: false hasContentIssue false
  • English
  • Français

On the 160 minute oscillation

Published online by Cambridge University Press:  03 August 2017

Pallé P.L.  and
T. Roca Cortés
Pallé P.L.
Affiliation:
Instituto de Astrofisica de Canarias, Universidad de La Laguna, Tenerife, Spain
T. Roca Cortés
Affiliation:
Instituto de Astrofisica de Canarias, Universidad de La Laguna, Tenerife, Spain

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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 ± .01 minute period, which can be interpreted as a g-mode.

Type
Chapter 1: Observations of Solar Oscillations
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 75 - 78
Copyright
Copyright © Reidel 1988 

References

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