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Solar cycle dependence of solar p nodes
Published online by Cambridge University Press: 03 August 2017
Abstract
Data obtained at Izana (Tenerife) and Haleakala (Maui), using optical resonant scattering with a potassium vapour cell over the years 1980–84, are used to determine the frequencies of the low ℓ p modes. Possible variation in these frequencies with the solar cycle are investigated.
- Type
- Chapter 3: Longterm Variations in the Sun
- Information
- Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 201 - 204
- Copyright
- Copyright © Reidel 1988