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Search for solar g-modes from 1981 to 1985
Published online by Cambridge University Press: 03 August 2017
Abstract
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