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Search for solar g-modes from 1981 to 1985

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

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Analysis of solar velocity data obtained at Izaña (Tenerife) over the years 1981–1985, has shown the existence of significant signals in the frequency range 25–125 μHz. Several ways of analyzing the data have been used in order to interpret these as solar internal gravity modes of degree ℓ≤ 3.

Type
Chapter 1: Observations of Solar Oscillations
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 79 - 82
Copyright
Copyright © Reidel 1988 

References

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4. Pallé, P.L.; (1986). Ph. D. Thesis, Universidad de La Laguna.Google Scholar
5. Delache, P.; (1984). Mem. S. A. It.; 55, 75 Google Scholar