Hostname: page-component-cc8bf7c57-pd9xq Total loading time: 0 Render date: 2024-12-12T05:04:50.882Z Has data issue: false hasContentIssue false
  • English
  • Français

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

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.

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

1. Delache, P.; Scherrer, P.; (1983). Nature; 306. 661 Google Scholar
2. Isaak, G.R.; van der Raay, H.B.; Pallé, P.L.; Roca Cortés, T.; (1984). Mem. S. A. It.; 55, 91 Google Scholar
3. Brookes, J.R.; Isaak, G.R.; van der Raay, H.B.; (1978). M.N.R.A.S., 185, 1 Google Scholar
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