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Determination of tidal h Love number parameters in the diurnal band using an extensive VLBI data setWe use over a decade of geodetic Very Long Baseline Interferometry (VLBI) data to estimate parameters in a resonance expansion of the frequency dependence of the tidal h(sub 2) Love number within the diurnal band. The resonance is associated with the retrograde free core nutation (RFCN). We obtain a value for the real part of the resonance strength of (-0.27 +/- 0.03) x 10(exp -3); a value of -0.19 x 10(exp -3) is predicted theoretically. Uncertainties in the VLBI estimates of the body tide radial displacement amplitudes are approximately 0.5 mm (1.1 mm for the K1 frequency), but they do not yield sufficiently small Love number uncertainties for placing useful constraints on the frequency of the RFCN, given the much smaller uncertainties obtained from independent analyses using nutation or gravimetric data. We also consider the imaginary part of the tidal h(sub 2) Love number. The estimated imaginary part of the resonance strength is (0.00 +/- 0.02) x 10(exp -3). The estimated imaginary part of the nonresonant component of the Love number implies a phase angle in the diurnal tidal response of the Earth of 0.7 deg +/- 0.5 deg (lag).
Document ID
19950034084
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Mitrovica, J. X.
(Univ. of Toronto Toronto, Ontario, Canada)
Davis, J. L.
(Harvard-Smithsonian Center for Astrophysics, Cambridge, MA United States)
Mathews, P. M.
(Harvard-Smithsonian Center for Astrophysics, Cambridge, MA United States)
Shapiro, I. I.
(Harvard-Smithsonian Center for Astrophysics, Cambridge, MA United States)
Date Acquired
August 16, 2013
Publication Date
April 15, 1994
Publication Information
Publication: Geophysical Research Letters
Volume: 21
Issue: 8
ISSN: 0094-8276
Subject Category
Geophysics
Accession Number
95A65683
Funding Number(s)
CONTRACT_GRANT: NSF EAR-92-06663
CONTRACT_GRANT: NAG5-1930
Distribution Limits
Public
Copyright
Other

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