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Spectrum of Latitude Variations in the Frequency Range 1.4-2.2 cpy and a Search for Nearly Diurnal Free Polar Motion
Published online by Cambridge University Press: 14 August 2015
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Astronomical latitude observations of the ILS stations seem to indicate the existence of both a retrograde and a direct component of nearly diurnal polar motion with close frequencies (Yatskiv et al. 1975). The latter would manifest itself as a latitude variation with a period of about 204 mean days (m.d.) and with a phase depending on the double longitude of station.
- Type
- Session II
- Information
- Symposium - International Astronomical Union , Volume 78: Nutation and the Earth's Rotation , 1980 , pp. 75 - 79
- Copyright
- Copyright © Reidel 1980
References
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