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 rpodes of degree ℓ ⩽3.
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© 1988 International Astronomical Union
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Pallé, P.L., Roca Cortés, T. (1988). Search For Solar G-Modes from 1981 to 1985. In: Christensen-Dalsgaard, J., Frandsen, S. (eds) Advances in Helio- and Asteroseismology. International Astronomical Union / Union Astronomique Internationale, vol 123. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4009-3_16
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DOI: https://doi.org/10.1007/978-94-009-4009-3_16
Publisher Name: Springer, Dordrecht
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